Effective Field Theory for Many-Body Systems

Size: px
Start display at page:

Download "Effective Field Theory for Many-Body Systems"

Transcription

1 Outline Systems EFT Dilute DFT Future Effective Field Theory for Many-Body Systems Department of Physics Ohio State University February 19, 2004

2 Outline Systems EFT Dilute DFT Future Principles of Effective Low-Energy Theories

3 Outline Systems EFT Dilute DFT Future Principles of Effective Low-Energy Theories If system is probed at low energies, fine details not resolved

4 Outline Systems EFT Dilute DFT Future Principles of Effective Low-Energy Theories If system is probed at low energies, fine details not resolved use low-energy dof s for low-energy processes short-distance structure can be replaced by something simpler without distorting low-energy observables

5 Outline Systems EFT Dilute DFT Future Outline Nuclear and Other Many-Body Problems Basic Effective Field Theory (EFT) Concepts EFT for Dilute Fermi Systems Density Functional Theory (DFT) Future: Challenges for

6 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Nuclear and Cold Atom Many-Body Problems Lennard-Jones and nucleon-nucleon potentials O -O potential (mev) n-n potential (MeV) n-n system O -O system n-n distance (fm) O 2-O 2 distance (nm) [figure borrowed from J. Dobaczewski] How can we deal with hard cores in many-body systems? Are there universal features of such many-body systems?

7 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Effective Range Expansion Total cross section: σ total = 4π k 2 (2l + 1) sin 2 δ l (k) l=0 What happens at low energy (k 1/R)? k cot δ 0 (k) k 0 1 a r 0k a 0 is the scattering length and r 0 is the effective range

8 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Near-Zero-Energy Bound States Bound-state or near-bound state at zero energy = large scattering lengths (a 0 ± )

9 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Near-Zero-Energy Bound States Bound-state or near-bound state at zero energy = large scattering lengths (a 0 ± ) For kr 0, the total cross section is { 4πa0 2 4πa 2 σ total = σ l=0 = 1 + (ka 0 ) 2 = 0 for ka 0 1 4π k 2 for ka 0 1 (unitarity limit)

10 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT How Are Trapped Atoms Like Neutron Stars? Regal et al., ultracold fermions Chandra X-Ray Observatory image of pulsar in 3C58

11 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Trapped Fermion Atoms Low densities and temperatures = only a 0 enters Use Feshbach resonances to tune scattering length a 0 ± Universal behavior? Superfluidity? BCS-BEC crossover?

12 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Neutron Stars n-n a 0 range of V NN (r) Dilute neutron gas at surface = neutron superfluid High density core: color superconductor? (see T. Schafer for EFT discussion)

13 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Quantum Chromodynamics and Nuclear Physics Quark Mass (m q ) Dependence of Observables S. Beane and M. Savage, Nucl. Phys. A717 (2003) 91. Crude (naive?) estimate of nonrelativistic bound state: E B p2 typical M f 2 π M 10 MeV E deuteron

14 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Is the Fine-Tuning Accidental? E. Epelbaum, U. Meißner, and W. Glöckle, Nucl. Phys. A714 (2003) B D [MeV] M π [MeV] Footnote from S. Weinberg paper [Nucl. Phys. B363 (1991) 3]: E. Witten says that large N c arguments... suggest that the very small binding energy of the deuteron is a fortuitous cancellation of potential and kinetic energies for the physical value N c = 3.

15 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Rare Isotope Accelerator (RIA) Physics Nucleosynthesis, halo nuclei, pairing,... Stable nuclei 126 Known nuclei 82 r-process Protons rp-process Terra incognita Neutron stars Neutrons Figure The nuclear landscape, defining the territory of nuclear physics research. On this chart of the nuclides, black squares represent stable nuclei and nuclei with half-lives comparable to or longer than the age of the Earth.

16 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Coulomb vs. Nuclear Many-Body Systems Common approaches to the many-body problem: Mean-field approaches (independent-particle picture) Monte Carlo methods (variational, GFMC) Hamiltonian diagonalization (CI, shell model) Density functional theory (DFT)

17 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Coulomb vs. Nuclear Many-Body Systems Common approaches to the many-body problem: Mean-field approaches (independent-particle picture) Monte Carlo methods (variational, GFMC) Hamiltonian diagonalization (CI, shell model) Density functional theory (DFT) Some important differences: Knowledge of interaction Spin-isospin dependence of interaction Importance of pairing Hartree-Fock as a starting point

18 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Coulomb vs. Nuclear Many-Body Systems Common approaches to the many-body problem: Mean-field approaches (independent-particle picture) Monte Carlo methods (variational, GFMC) Hamiltonian diagonalization (CI, shell model) Density functional theory (DFT) Some important differences: Knowledge of interaction Spin-isospin dependence of interaction Importance of pairing Hartree-Fock as a starting point Ab initio calculations?

19 Figure 2: Top: the nuclear landscape - the territory of RIA Many-Body physics. The EFT black squares represent the stable Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Different Approaches for Different Regions Limits of nuclear existence r-process protons rp-process neutrons

20 Figure 2: Top: the nuclear landscape - the territory of RIA Many-Body physics. The EFT black squares represent the stable Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Different Approaches for Different Regions Limits of nuclear existence r-process protons rp-process A=10 A=12 50 neutrons A~60 82 Density Functional Theory Selfconsistent Mean Field Ab initio few-body calculations 0Ñω Shell Model No-Core Shell Model G-matrix Many-body approaches for ordinary nuclei

21 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Density Functional Theory (DFT) Hohenberg-Kohn: There exists an energy functional E v [n]... E v [n] = F HK [n] + d 3 x v(x)n(x) F HK is universal (same for any external v) = H 2 to DNA!

22 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Density Functional Theory (DFT) Hohenberg-Kohn: There exists an energy functional E v [n]... E v [n] = F HK [n] + d 3 x v(x)n(x) F HK is universal (same for any external v) = H 2 to DNA! Useful if you can approximate the energy functional

23 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Density Functional Theory (DFT) Hohenberg-Kohn: There exists an energy functional E v [n]... E v [n] = F HK [n] + d 3 x v(x)n(x) F HK is universal (same for any external v) = H 2 to DNA! Useful if you can approximate the energy functional Kohn-Sham procedure similar to nuclear mean field calculations

24 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Problems with Extrapolations Stable nuclei 126 Known nuclei 82 r-process Protons rp-process Terra incognita Neutron stars Neutrons Figure The nuclear landscape, defining the territory of nuclear physics research. On this chart of the nuclides, black squares represent stable nuclei and nuclei with half-lives comparable to or longer than the age of the Earth. These nuclei define the valley of stability. By adding either protons or neutrons, one moves away from the valley of stability, finally reaching the drip lines where nuclear binding forces Many-Body are no longer EFT strong enough to hold these nuclei

25 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Problems with Extrapolations

26 Outline Systems EFT Dilute DFT Future a 0 Atoms RIA DFT Problems with Extrapolations Mass formulas and energy functionals do well where there is data, but elsewhere... two-neutron separation energies S 2n (MeV) Sn data exist Experiment HFB-SLy4 HFB-SkP HFB-D1S SkX RHB-NL3 LEDF Mass Formulae Neutron Number data do not exist Neutron Number Neutron Number exp FRDM CKZ JM MJ T+ Figure 6: Predicted two-neutron separation energies for the even-even Sn isotopes using several microscopic models based on effective nucleon-nucleon interactions and obtained with phenomenological

27 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Why Use EFT For Many-Body Physics? Connections between different processes and to QCD Guide to making systematic calculations with error estimates For RIA physics = reliable, model independent extrapolation

28 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Why Use EFT For Many-Body Physics? Connections between different processes and to QCD Guide to making systematic calculations with error estimates For RIA physics = reliable, model independent extrapolation Analogy between EFT and basic numerical analysis naive error analysis: pick a method and reduce the mesh size (e.g., increase grid points) until the error is acceptable sophisticated error analysis: understand scaling and sources of error (e.g., algorithm vs. round-off errors) = Does it work as well as it should? representation dependence = not all are equally effective! extrapolation: completeness of an expansion basis

29 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis Numerical Derivatives f (x) = [f(x+h)-f(x)]/h + O(h) relative error mesh size h

30 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis relative error Numerical Derivatives f (x) = [f(x+h)-f(x)]/h + O(h) f (x) = [f(x+h/2)-f(x-h/2)]/h + O(h 2 ) mesh size h

31 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis relative error Numerical Derivatives f (x) = [f(x+h)-f(x)]/h + O(h) f (x) = [f(x+h/2)-f(x-h/2)]/h + O(h 2 ) Richardson extrapolation O(h 4 ) mesh size h

32 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis Numerical Integration relative error h n to h n trapezoid rule O(h 2 ) mesh size h

33 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis Numerical Integration relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) mesh size h

34 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Numerical Analysis Numerical Integration relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) Milne s rule O(h 6 ) mesh size h

35 Outline Systems EFT Dilute DFT Future Analogs RG Chiral The Representation Can Make A Difference! E.g., elliptic integral: 1 0 (1 x 2 )(2 x) dx

36 Outline Systems EFT Dilute DFT Future Analogs RG Chiral The Representation Can Make A Difference! E.g., elliptic integral: 1 0 (1 x 2 )(2 x) dx How do the numerical errors behave? relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) Milne s rule O(h 6 ) before Numerical Integration mesh size h

37 Outline Systems EFT Dilute DFT Future Analogs RG Chiral The Representation Can Make A Difference! E.g., elliptic integral: 1 0 (1 x 2 )(2 x) dx How do the numerical errors behave? After transformation: π/2 0 sin 2 y 2 cos y dy relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) Milne s rule O(h 6 ) before Numerical Integration after mesh size h

38 Outline Systems EFT Dilute DFT Future Analogs RG Chiral The Representation Can Make A Difference! E.g., elliptic integral: 1 0 (1 x 2 )(2 x) dx How do the numerical errors behave? After transformation: π/2 0 sin 2 y 2 cos y dy relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) Milne s rule O(h 6 ) before Numerical Integration after mesh size h

39 Outline Systems EFT Dilute DFT Future Analogs RG Chiral The Representation Can Make A Difference! E.g., elliptic integral: 1 0 (1 x 2 )(2 x) dx How do the numerical errors behave? After transformation: π/2 0 sin 2 y 2 cos y dy relative error h n to h n trapezoid rule O(h 2 ) Simpson s rule O(h 4 ) Milne s rule O(h 6 ) before Numerical Integration after mesh size h

40 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Completeness, Fitting, and Extrapolation What if I fit my model in one region, then predict in another? Take our function: (1 x 2 )(2 x) and fit it for 0.3 x 0.6 f(x) exact function a 0 + a 1 x + a 2 x 2 b 0 + b 1 x + b 3 x 3 c 0 + c 1 x + c 3 x 3 + c 4 x x

41 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Completeness, Fitting, and Extrapolation What if I fit my model in one region, then predict in another? Take our function: (1 x 2 )(2 x) and fit it for 0.3 x 0.6 f(x) exact function a 0 + a 1 x + a 2 x 2 b 0 + b 1 x + b 3 x 3 c 0 + c 1 x + c 3 x 3 + c 4 x x

42 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Completeness, Fitting, and Extrapolation What if I fit my model in one region, then predict in another? Take our function: (1 x 2 )(2 x) and fit it for 0.3 x 0.6 Compare complete and incomplete models and weighting relative error a 0 + a 1 x + a 2 x 2 b 0 + b 1 x + b 3 x x

43 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Completeness, Fitting, and Extrapolation What if I fit my model in one region, then predict in another? Take our function: (1 x 2 )(2 x) and fit it for 0.3 x 0.6 Compare complete and incomplete models and weighting relative error a 0 + a 1 x + a 2 x 2 b 0 + b 1 x + b 3 x 3 c 0 + c 1 x + c 3 x 3 + c 4 x x

44 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Completeness, Fitting, and Extrapolation What if I fit my model in one region, then predict in another? Take our function: (1 x 2 )(2 x) and fit it for 0.3 x 0.6 Compare complete and incomplete models and weighting relative error a 0 + a 1 x + a 2 x 2 b 0 + b 1 x + b 3 x 3 c 0 + c 1 x + c 3 x 3 + c 4 x 4 weighted x

45 Outline Systems EFT Dilute DFT Future Analogs RG Chiral NN Potential and Scattering Phase Shifts n-n potential (MeV) n-n system O -O system n-n distance (fm) low 0 energies 0.4 = 0.8 large a O 2-O 2 distance (nm) zero crossing = hard core phase shift (degrees) np 1 S 0 (PWA93) E lab (MeV)

46 V NN (k,k) [fm] Outline Systems EFT Dilute DFT Future Analogs RG Chiral NN Potential and Scattering Phase Shifts Now look at NN potentials in momentum space: s-wave k V k Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ] phase shift (degrees) np 1 S 0 (PWA93) E lab (MeV) Many different potentials with same phase shifts (χ 2 /dof 1)

47 Outline Systems EFT Dilute DFT Future Analogs RG Chiral NN Scattering in the COM Frame k +k k +k T 3 2 T k +k = V B k +k + q Λ B χ 2 /dof 1 bare potential V B Probes intermediate states to q Λ B = 25 fm 1 =. 5 GeV V B V NN (k,k) [fm] Model dependent: q 3 fm k [fm -1 ] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I

48 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Momentum NN Potential Bogner, Kuo, Schwenk k +k k +k T 3 T = V Λ + q Λ 2 V Λ k +k k +k Require dt dλ = 0 = renormalization group equation for V Λ Run from Λ B = 25 fm 1 to Λ = 2 fm 1 E lab. = 350 MeV V NN (k,k) [fm] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ]

49 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Momentum NN Potential Bogner, Kuo, Schwenk k +k k +k T 3 T = V Λ + q Λ 2 V Λ k +k k +k Require dt dλ = 0 = renormalization group equation for V Λ Run from Λ B = 25 fm 1 to Λ = 2 fm 1 E lab. = 350 MeV V NN (k,k) [fm] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ]

50 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Momentum NN Potential Bogner, Kuo, Schwenk k +k k +k T 3 T = V Λ + q Λ 2 V Λ k +k k +k Require dt dλ = 0 = renormalization group equation for V Λ Run from Λ B = 25 fm 1 to Λ = 2 fm 1 E lab. = 350 MeV V NN (k,k) [fm] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ]

51 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Momentum NN Potential Bogner, Kuo, Schwenk k +k k +k T 3 T = V Λ + q Λ 2 V Λ k +k k +k Require dt dλ = 0 = renormalization group equation for V Λ Run from Λ B = 25 fm 1 to Λ = 2 fm 1. E lab = 350 MeV Same long distance physics = collapse! V NN (k,k) [fm] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ]

52 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Energy Observables Unchanged Phase shift δ vs. E Lab [MeV] 0 1 S P S1 P0 5 P D1 1 ε P1 PSA93

53 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Energy Observables Unchanged Phase shift δ vs. E Lab [MeV] 0 1 S P S1 P0 5 P D1 1 ε P1 PSA93 CD Bonn

54 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Energy Observables Unchanged Phase shift δ vs. E Lab [MeV] 0 1 S P S1 P0 5 P D1 1 ε P1 PSA93 CD Bonn V Λ=2 fm -1

55 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Low-Momentum Pot l in the Many-Body Problem Removing hard core = simpler many-body starting point for neutron matter [Schwenk, Friman, Brown] Simple Hartree-Fock (triangles) instead of BHF (circles)

56 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Three-Body Forces are Inevitable! What if we have three nucleons interacting? Successive two-body scatterings with short-lived high-energy intermediate states unresolved = must be absorbed into three-body force Binding Energy (MeV) Triton Binding Energy AV18 CD Bonn Experiment Λ (fm -1 ) [Bogner, Nogga, Schwenk]

57 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Three-Body Forces are Inevitable! What if we have three nucleons interacting? Successive two-body scatterings with short-lived high-energy intermediate states unresolved = must be absorbed into three-body force Binding Energy (MeV) Triton Binding Energy AV18 CD Bonn Experiment How do we organize three-body forces? Λ (fm -1 ) [Bogner, Nogga, Schwenk]

58 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Renormalization and Short-Distance Physics 3 V B = C0 2 q > Λ V B q > Λ intermediate states = replace with contact term: C 0 δ 3 (x x ) L eft = (ψ ψ) 2 + V NN (k,k) [fm] Paris Bonn A Argonne v18 Idaho A CD Bonn Nijmegen94 II Nijmegen94 I k [fm -1 ]

59 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Effective Field Theory Ingredients From Crossing the Border [nucl-th/ ] 1. Use the most general L with low-energy dof s consistent with the global and local symmetries of the underlying theory 2. Declaration of regularization and renormalization scheme 3. Well-defined power counting = small expansion parameters

60 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Effective Field Theory Ingredients: NN From Crossing the Border [nucl-th/ ] 1. Use the most general L with low-energy dof s consistent with the global and local symmetries of the underlying theory L eft = L ππ + L πn + L NN chiral symmetry = systematic long-distance pion physics 2. Declaration of regularization and renormalization scheme 3. Well-defined power counting = small expansion parameters

61 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Effective Field Theory Ingredients: NN From Crossing the Border [nucl-th/ ] 1. Use the most general L with low-energy dof s consistent with the global and local symmetries of the underlying theory L eft = L ππ + L πn + L NN chiral symmetry = systematic long-distance pion physics 2. Declaration of regularization and renormalization scheme momentum cutoff and Weinberg counting use cutoff sensitivity as measure of uncertainties! 3. Well-defined power counting = small expansion parameters

62 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Effective Field Theory Ingredients: NN From Crossing the Border [nucl-th/ ] 1. Use the most general L with low-energy dof s consistent with the global and local symmetries of the underlying theory L eft = L ππ + L πn + L NN chiral symmetry = systematic long-distance pion physics 2. Declaration of regularization and renormalization scheme momentum cutoff and Weinberg counting use cutoff sensitivity as measure of uncertainties! 3. Well-defined power counting = small expansion parameters use the separation of scales = {p, m π} with Λ Λ χ 1 GeV χ Weinberg: power-count V NN and solve S-equation chiral symmetry = V NN = ν=ν min c ν Q ν with ν 0

63 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Chiral Effective Field Theory for Two Nucleons Epelbaum, Meißner, et al. Also Entem, Machleidt L πn + match at low energy Q ν 1π 2π 4N 1S0 3S P0 1D D3 3G

64 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Chiral Effective Field Theory for Two Nucleons Epelbaum, Meißner, et al. Also Entem, Machleidt L πn + match at low energy Q ν 1π 2π 4N Q 0 1S0 3S P0 1D D3 3G

65 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Chiral Effective Field Theory for Two Nucleons Epelbaum, Meißner, et al. Also Entem, Machleidt L πn + match at low energy Q ν 1π 2π 4N Q 0 Q 1 1S0 3S P0 1D D3 3G

66 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Chiral Effective Field Theory for Two Nucleons Epelbaum, Meißner, et al. Also Entem, Machleidt L πn + match at low energy Q ν 1π 2π 4N Q 0 Q 1 Q 2 1S0 3S P0 1D D3 3G

67 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Chiral Effective Field Theory for Two Nucleons Epelbaum, Meißner, et al. Also Entem, Machleidt L πn + match at low energy Q ν 1π 2π 4N Q 0 Q 1 Q 2 Q 3 1S0 3S P0 1D D3 3G

68 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Effective Field Theory G. P. Lepage, How to Renormalize the Schrödinger Equation! "$# % % & Errors in the 1 S 0 phase shifts versus energy through orders Λ 2 and Λ 4. Results from the theory with just pion exchange (V 1π ) are also shown. The cutoff was Λ=330 MeV in each case.

69 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Error Plots in Effective Field Theory G. P. Lepage, How to Renormalize the Schrödinger Equation!#"%$ & & '(' & ) & Errors in the 1 S 0 phase shifts versus energy for different values of the cutoff Λ.

70 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Segue: From EFT Potentials to EFT Many-Body So far: Systematic few-body potentials for input to exact methods for solving many-body Schrödinger equations The effort to develop many-body potentials for nuclei continues No-core shell model calculations are applying these potentials Steady progress expected but limited range in A = N + Z

71 Outline Systems EFT Dilute DFT Future Analogs RG Chiral Segue: From EFT Potentials to EFT Many-Body So far: Systematic few-body potentials for input to exact methods for solving many-body Schrödinger equations The effort to develop many-body potentials for nuclei continues No-core shell model calculations are applying these potentials Steady progress expected but limited range in A = N + Z Turn now to more basic interactions but direct many-body EFT Start with simplest systems; protoype is cold Fermi atoms in a trap Technical advantages from physics simplifications Large scattering length problem Finite systems

72 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Simple Many-Body Problem: Hard Spheres Infinite potential at radius R sin(kr+δ) R 0 R r ~ 1/ k F Scattering length a 0 = R Dilute nr 3 1 = k F a 0 1 What is the energy / particle?

73 Outline Systems EFT Dilute DFT Future Spheres Large a 0 In Search of a Perturbative Expansion For free-space scattering at momentum k 1/R, we should recover a perturbative expansion in kr for scattering amplitude: f 0 (k) 1 k cot δ(k) ik a 0 ia 2 0k (a 3 0 a2 0r 0 /2)k 2 + O(k 3 a 3 0 ) with a 0 = R and r 0 = 2R/3 for hard-core spheres

74 Outline Systems EFT Dilute DFT Future Spheres Large a 0 In Search of a Perturbative Expansion For free-space scattering at momentum k 1/R, we should recover a perturbative expansion in kr for scattering amplitude: f 0 (k) 1 k cot δ(k) ik a 0 ia 2 0k (a 3 0 a2 0r 0 /2)k 2 + O(k 3 a 3 0 ) with a 0 = R and r 0 = 2R/3 for hard-core spheres Perturbation theory in the hard-core potential won t work: = k V k dx e ik x V (x) e ik x 0 R

75 Outline Systems EFT Dilute DFT Future Spheres Large a 0 In Search of a Perturbative Expansion For free-space scattering at momentum k 1/R, we should recover a perturbative expansion in kr for scattering amplitude: f 0 (k) 1 k cot δ(k) ik a 0 ia 2 0k (a 3 0 a2 0r 0 /2)k 2 + O(k 3 a 3 0 ) with a 0 = R and r 0 = 2R/3 for hard-core spheres Perturbation theory in the hard-core potential won t work: = k V k dx e ik x V (x) e ik x 0 R Standard solution: Solve nonperturbatively, then expand

76 Outline Systems EFT Dilute DFT Future Spheres Large a 0 In Search of a Perturbative Expansion For free-space scattering at momentum k 1/R, we should recover a perturbative expansion in kr for scattering amplitude: f 0 (k) 1 k cot δ(k) ik a 0 ia 2 0k (a 3 0 a2 0r 0 /2)k 2 + O(k 3 a 3 0 ) with a 0 = R and r 0 = 2R/3 for hard-core spheres Perturbation theory in the hard-core potential won t work: = k V k dx e ik x V (x) e ik x 0 R Standard solution: Solve nonperturbatively, then expand EFT approach: k 1/R means we probe at low resolution = replace potential with a simpler but general interaction

77 Outline Systems EFT Dilute DFT Future Spheres Large a 0 EFT for Natural Dilute Fermi Gas A simple, general interaction is a sum of delta functions and derivatives of delta functions. In momentum space, k V eft k = C C 2(k 2 + k 2 ) + C 2 k k + Or, L eft has most general local (contact) interactions: L eft = ψ [ i t + 2 2M ] ψ C 0 2 (ψ ψ) 2 + C 2 [ (ψψ) (ψ 2 ψ) + h.c. ] 16 + C 2 8 (ψ ψ) (ψ ψ) D 0 6 (ψ ψ) Dimensional analysis = C 2i 4π M R2i+1, D 2i 4π M R2i+4

78 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Renormalization Consider the leading potential V (0) EFT (x) = C 0δ(x) or k V (0) eft k = = C 0 Choosing C 0 a 0 gets the first term. Now k VG 0 V k : = d 3 q 1 (2π) 3 k 2 q 2! + iɛ = Linear divergence!

79 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Renormalization Consider the leading potential V (0) EFT (x) = C 0δ(x) or k V (0) eft k = = C 0 Choosing C 0 a 0 gets the first term. Now k VG 0 V k : = Λc d 3 q 1 (2π) 3 k 2 q 2 + iɛ Λ c 2π 2 ik 4π + O(k 2 /Λ c ) = If cutoff at Λ c, then can absorb into V (0), but all powers of k 2

80 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Renormalization Consider the leading potential V (0) EFT (x) = C 0δ(x) or k V (0) eft k = = C 0 Choosing C 0 a 0 gets the first term. Now k VG 0 V k : = d D q 1 D 3 (2π) 3 k 2 q 2 ik + iɛ 4π Dimensional regularization with minimal subtraction = only one power of k!

81 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Dim. reg. + minimal subtraction = simple power counting: P/2 + k P/2 + k = + P/2 k P/2 k it (k, cos θ) ic 0 M 4π (C0)2 k O(k 3 ) ( M )2 +i (C 0) 3 k 2 ic 2k 2 ic 4π 2k 2 cos θ Matching: C 0 = 4π M a 0 = 4π M R, C 2 = 4π M a 2 0 r 0 2 = 4π M R3 3,

82 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Dim. reg. + minimal subtraction = simple power counting: P/2 + k P/2 + k = + P/2 k P/2 k it (k, cos θ) ic 0 M 4π (C0)2 k O(k 3 ) ( M )2 +i (C 0) 3 k 2 ic 2k 2 ic 4π 2k 2 cos θ Matching: C 0 = 4π M a 0 = 4π M R, C 2 = 4π M a 2 0 r 0 2 = 4π M R3 3, Recovers effective range expansion order-by-order with perturbative diagrammatic expansion one power of k per diagram estimate truncation error from dimensional analysis

83 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Now Sum Over Fermions in the Fermi Sea Leading order V (0) EFT (x) = C 0δ(x) = a 0 k 6 F

84 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Now Sum Over Fermions in the Fermi Sea Leading order V (0) EFT (x) = C 0δ(x) = a 0 k 6 F At the next order, we get a linear divergence again: = k F d 3 q 1 (2π) 3 k 2 q 2

85 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Now Sum Over Fermions in the Fermi Sea Leading order V (0) EFT (x) = C 0δ(x) = a 0 k 6 F At the next order, we get a linear divergence again: = k F d 3 q 1 (2π) 3 k 2 q 2 Same renormalization fixes it! Particles holes k F 1 k 2 q 2 = 0 1 k 2 q 2 kf 0 1 D 3 k 2 q 2 kf 0 1 k 2 q 2 a2 0k 7 F

86 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams E V = n k F 2 [ 3 2M 5 ]

87 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams O ( kf 6 ) E : V = n k F 2 2M [ (ν 1) 5 3π (k Fa 0 ) ]

88 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams O ( k 6 F) : O ( k 7 F) : + E V = n k F 2 [ (ν 1) 2M 5 3π (k Fa 0 ) 4 + (ν 1) 35π 2 (11 2 ln 2)(k Fa 0 ) 2 ]

89 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams O ( k 6 F) : O ( k 7 F) : + E V = n k F 2 [ (ν 1) 2M 5 3π (k Fa 0 ) 4 + (ν 1) 35π 2 (11 2 ln 2)(k Fa 0 ) 2 O ( k 8 F) : + ]

90 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams O ( k 6 F) : O ( k 7 F) : + O ( k 8 F) : + E V = n k F 2 [ (ν 1) 2M 5 3π (k Fa 0 ) 4 + (ν 1) 35π 2 (11 2 ln 2)(k Fa 0 ) 2 + (ν 1) ( (ν 3) ) (k F a 0 ) ]

91 Outline Systems EFT Dilute DFT Future Spheres Large a 0 T = 0 Energy Density from Hugenholtz Diagrams O ( kf) 6 : O ( kf) 7 : + O ( kf) 8 : E V = n k F 2 [ (ν 1) 2M 5 3π (k Fa 0 ) 4 + (ν 1) 35π 2 (11 2 ln 2)(k Fa 0 ) 2 + (ν 1) ( (ν 3) ) (k F a 0 ) 3 + (ν 1) 1 10π (k Fr 0 )(k F a 0 ) 2 + (ν + 1) 1 5π (k Fa p ) 3 + ]

92 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Looks Like a Power Series in k F! Is it?

93 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Looks Like a Power Series in k F! Is it? New logarithmic divergences in 3 3 scattering + (C 0 ) 4 ln(k F /Λ c )

94 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Looks Like a Power Series in k F! Is it? New logarithmic divergences in 3 3 scattering + (C 0 ) 4 ln(k F /Λ c ) Changes in Λ c must be absorbed by 3-body coupling D 0 (Λ c ) = D 0 (Λ c ) (C 0 ) 4 ln(a 0 Λ c ) + const. [Braaten & Nieto] [ ] d = 0 = same coefficient! dλ c

95 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Looks Like a Power Series in k F! Is it? New logarithmic divergences in 3 3 scattering + (C 0 ) 4 ln(k F /Λ c ) Changes in Λ c must be absorbed by 3-body coupling D 0 (Λ c ) = D 0 (Λ c ) (C 0 ) 4 ln(a 0 Λ c ) + const. [Braaten & Nieto] [ ] d = 0 = same coefficient! dλ c What does this imply for the energy density? O ( k 9 F ln(k F ) ) : + + (ν 2)(ν 1) (k F a 0 ) 4 ln(k F a 0 )

96 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Large Scattering Length Problem Attractive with a 0 If R 1/k F a 0, then expect scale invariance R Energy and gap are pure numbers times E FG = 3 5 kf 2 2M ~ 1/ k F a 0

97 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Large Scattering Length Problem Attractive with a 0 If R 1/k F a 0, then expect scale invariance R Energy and gap are pure numbers times E FG = 3 5 kf 2 2M EFT power counting says: sum everything with leading vertices Easy in free space = geometric sum of bubbles Many more diagrams in the medium ~ 1/ a 0 k F

98 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Calculations Summing All Leading Diagrams Green s Function Monte Carlo (GMFC) [J. Carlson et al.] Solve many-body S-eqn with variational wf improved by GFMC GFMC applied to real nuclei up to A = 12 with energies to 1% Large a 0 : Convenient potential tuned to a 0

99 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Calculations Summing All Leading Diagrams Green s Function Monte Carlo (GMFC) [J. Carlson et al.] Solve many-body S-eqn with variational wf improved by GFMC GFMC applied to real nuclei up to A = 12 with energies to 1% Large a 0 : Convenient potential tuned to a 0 Lattice calculation for two spins = no fermion sign problem! Path integral evaluated on discretized space-time lattice QCD lattice calculations = best nonperturbative results Large a 0 : Proposed by J.-W. Chen and D. Kaplan In progress by QCD lattice gauge theorist [M. Wingate]

100 Outline Systems EFT Dilute DFT Future Spheres Large a 0 GFMC Results [J. Carlson et al.] Extrapolate to large numbers of fermions 20 Pairing gap ( ) = 0.9 E FG E/E FG 10 odd N E = 0.44 N E FG even N N Energy per particle: E/N = 0.44(1)E FG

101 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Trapped Atoms Low densities and temperatures = only a 0 enters Use Feshbach resonances to tune scattering length a 0 ± Universal behavior? Superfluidity? BCS-BEC crossover?

102 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Is There An Additional Expansion?

103 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Is There An Additional Expansion? No parameters with dimensions. What about geometry?

104 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Is There An Additional Expansion? No parameters with dimensions. What about geometry? J. Steele: Organize according to space-time dimension P/2 q k F 1 P/2 q k F 1 2 D/2

105 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Is There An Additional Expansion? No parameters with dimensions. What about geometry? J. Steele: Organize according to space-time dimension P/2 q k F 1 P/2 q k F 1 2 D/2 Leading 1/D analytic expansion yields: ( E A = E FG k ) Fa 0 /9 a + O(1/D) 0 4 π 2k F a 0 9 E FG [cf. 0.44(1) E FG ]

106 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Is There An Additional Expansion? No parameters with dimensions. What about geometry? J. Steele: Organize according to space-time dimension P/2 q k F 1 P/2 q k F 1 2 D/2 Leading 1/D analytic expansion yields: ( E A = E FG k ) Fa 0 /9 a + O(1/D) 0 4 π 2k F a 0 9 E FG [cf. 0.44(1) E FG ] Subleading??? Pairing gap???

107 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Only an EFT Sampler: Many Omitted Topics Bose many-body systems (BEC s and all that) Three-body physics with large scattering lengths Halo nuclei, pairing, relativistic systems,...

108 Outline Systems EFT Dilute DFT Future Spheres Large a 0 Only an EFT Sampler: Many Omitted Topics Bose many-body systems (BEC s and all that) Three-body physics with large scattering lengths Halo nuclei, pairing, relativistic systems,... Turn now to Density Functional Theory (DFT)

109 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Density Functional Theory Hohenberg-Kohn: There exists an energy functional E v [n]... E v [n] = F HK [n] + d 3 x v(x)n(x) E v [n] minimized for ground state n(x) F HK is universal (same for any external v) = H 2 to DNA!

110 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham DFT V HO = V KS Interacting density with v HO Non-interacting density with v KS

111 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham DFT V HO = V KS Interacting density with v HO Orbitals {φ i (x)} in local potential v KS ([n], x) Non-interacting density with v KS [ 2 /2m + v KS (x)]φ i = ɛ i φ i = n(x) = N φ i (x) 2 i=1 find Kohn-Sham potential v KS (x) from δe v [n]/δn(x) Solve self-consistently

112 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Density Functional Theory Dominant application: inhomogeneous electron gas Interacting point electrons in static potential of atomic nuclei Ab initio calculations of atoms, molecules, crystals, surfaces number of retrieved records per year Hartree Fock Density Functional Theory year

113 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Density Functional Theory Dominant application: inhomogeneous electron gas Interacting point electrons in static potential of atomic nuclei Ab initio calculations of atoms, molecules, crystals, surfaces % deviation from experiment Atomization Energies of Hydrocarbon Molecules Hartree-Fock DFT Local Spin Density Approximation DFT Generalized Gradient Approximation H 2 C 2 C 2 H 2 CH 4 C 2 H 4 C 2 H 6 C 6 H 6 molecule

114 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Quotes From the DFT Literature

115 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Quotes From the DFT Literature A Chemist s Guide to DFT (Koch & Holthausen, 2000) To many, the success of DFT appeared somewhat miraculous, and maybe even unjust and unjustified. Unjust in view of the easy achievement of accuracy that was so hard to come by in the wave function based methods. And unjustified it appeared to those who doubted the soundness of the theoretical foundations.

116 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Quotes From the DFT Literature A Chemist s Guide to DFT (Koch & Holthausen, 2000) To many, the success of DFT appeared somewhat miraculous, and maybe even unjust and unjustified. Unjust in view of the easy achievement of accuracy that was so hard to come by in the wave function based methods. And unjustified it appeared to those who doubted the soundness of the theoretical foundations. Density Functional Theory (AJP, Argaman & Makov, 2000) It is important to stress that all practical applications of DFT rest on essentially uncontrolled approximations, such as the LDA...

117 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Quotes From the DFT Literature A Chemist s Guide to DFT (Koch & Holthausen, 2000) To many, the success of DFT appeared somewhat miraculous, and maybe even unjust and unjustified. Unjust in view of the easy achievement of accuracy that was so hard to come by in the wave function based methods. And unjustified it appeared to those who doubted the soundness of the theoretical foundations. Density Functional Theory (AJP, Argaman & Makov, 2000) It is important to stress that all practical applications of DFT rest on essentially uncontrolled approximations, such as the LDA... Meta-Generalized Gradient Approximation (Perdew et al., 1999) Some say that there is no systematic way to construct density functional approximations. But there are more or less systematic ways, and the approach taken... here is one of the former.

118 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Thermodynamic Interpretation of DFT Consider a system of spins S i on a lattice with interaction g The partition function has the information about the energy, magnetization of the system: Z = Tr e βg P {i,j} S i S j

119 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Thermodynamic Interpretation of DFT Consider a system of spins S i on a lattice with interaction g The partition function has the information about the energy, magnetization of the system: Z = Tr e βg P {i,j} S i S j The magnetization M is M = S i i = 1 Z Tr [ ( i S i ) e βg P {i,j} S i S j ]

120 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Add A Magnetic Probe Source H The source probes configurations near the ground state Z[H] = e βf [H] = Tr e β(g P {i,j} S i S j +H P i S i )

121 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Add A Magnetic Probe Source H The source probes configurations near the ground state Z[H] = e βf [H] = Tr e β(g P {i,j} S i S j +H P i S i ) Variations of the source yield the magnetization M = S i i H F [H] = H

122 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Add A Magnetic Probe Source H The source probes configurations near the ground state Z[H] = e βf [H] = Tr e β(g P {i,j} S i S j +H P i S i ) Variations of the source yield the magnetization M = S i i H F [H] = H F[H] is the Helmholtz free energy. Set H = 0 (or equal to a real external source) at the end

123 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Legendre Transformation to Effective Action Find H[M] by inverting M = S i = F[H] H H i

124 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Legendre Transformation to Effective Action Find H[M] by inverting M = S i = F[H] H H i Legendre transform to the Gibbs free energy Γ[M] = F [H] + H M

125 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Legendre Transformation to Effective Action Find H[M] by inverting M = S i = F[H] H H i Legendre transform to the Gibbs free energy Γ[M] = F [H] + H M The ground-state magnetization M gs follows by minimizing Γ[M]: H = Γ[M] Γ[M] M M = 0 Mgs

126 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results DFT as Analogous Legendre Transformation In analogy to the spin system, add source J(x) coupled to density operator n(x) ψ (x)ψ(x) to the partition function: Z[J] = e W [J] Tr e β(b H+J bn) D[ψ ]D[ψ] e R [L+J ψ ψ]

127 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results DFT as Analogous Legendre Transformation In analogy to the spin system, add source J(x) coupled to density operator n(x) ψ (x)ψ(x) to the partition function: Z[J] = e W [J] Tr e β(b H+J bn) D[ψ ]D[ψ] e R [L+J ψ ψ] The density n(x) in the presence of J(x) is n(x) n(x) J = δw [J] δj(x)

128 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results DFT as Analogous Legendre Transformation In analogy to the spin system, add source J(x) coupled to density operator n(x) ψ (x)ψ(x) to the partition function: Z[J] = e W [J] Tr e β(b H+J bn) D[ψ ]D[ψ] e R [L+J ψ ψ] The density n(x) in the presence of J(x) is n(x) n(x) J = δw [J] δj(x) Invert to find J[n] and Legendre transform from J to n: Γ[n] = W [J] + J n with J(x) = δγ[n] δγ[n] δn(x) δn(x) = 0 ngs(x) = For static n(x), Γ[n] the DFT energy functional F HK!

129 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results What can EFT do for DFT? Effective action as a path integral = construct W [J] order-by-order in EFT expansion For dilute system, same diagrams as before

130 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results What can EFT do for DFT? Effective action as a path integral = construct W [J] order-by-order in EFT expansion For dilute system, same diagrams as before Inversion method: order-by-order inversion from W [J] to Γ[n] E.g., J(x) = J 0 (x) + J LO (x) + J NLO (x) +... Two conditions on J 0 : n(x) = δw 0[J 0 ] J 0 (x) and J 0 (x) n=ngs = δγ interacting[n] δn(x) n=ngs

131 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results What can EFT do for DFT? Effective action as a path integral = construct W [J] order-by-order in EFT expansion For dilute system, same diagrams as before Inversion method: order-by-order inversion from W [J] to Γ[n] E.g., J(x) = J 0 (x) + J LO (x) + J NLO (x) +... Two conditions on J 0 : n(x) = δw 0[J 0 ] J 0 (x) and J 0 (x) n=ngs = δγ interacting[n] δn(x) Interpretation: J 0 is the external potential that yields for a noninteracting system the exact density This is the Kohn-Sham potential! Two conditions on J 0 = Self-consistency n=ngs

132 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) J 0 (x) = [

133 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) LO : J 0 (x) = [ (ν 1) ν 4πa 0 M ρ(x)

134 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) LO : NLO : + J 0 (x) = [ (ν 1) ν 4πa 0 M ρ(x) c 1 a 2 0 2M [ρ(x)]4/3

135 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) LO : NLO : + J 0 (x) = [ (ν 1) ν 4πa 0 M ρ(x) c 1 a 2 0 2M [ρ(x)]4/3 NNLO : +

136 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) LO : NLO : + J 0 (x) = [ (ν 1) ν 4πa 0 M ρ(x) c 1 a 2 0 2M [ρ(x)]4/3 NNLO : + c 2 a 3 0 [ρ(x)]5/3 + +

137 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Kohn-Sham J 0 According to the EFT Expansion Simplifying with the local density approximation (LDA) LO : NLO : + J 0 (x) = [ (ν 1) ν 4πa 0 M ρ(x) c 1 a 2 0 2M [ρ(x)]4/3 NNLO : c 2 a0 3 [ρ(x)]5/3 c 3 a0 2 r 0 [ρ(x)] 5/3 ] c 4 ap[ρ(x)] 3 5/3 +

138 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure:

139 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi)

140 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi) 2. Evaluate local single-particle potential v KS (r) v(r) J 0 (r)

141 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi) 2. Evaluate local single-particle potential v KS (r) v(r) J 0 (r) 3. Solve for lowest N states (including degeneracies): {ψ α, ɛ α } [ 2 2M + v KS(r) ] ψ α (x) = ɛ α ψ α (x)

142 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi) 2. Evaluate local single-particle potential v KS (r) v(r) J 0 (r) 3. Solve for lowest N states (including degeneracies): {ψ α, ɛ α } [ 2 2M + v KS(r) ] ψ α (x) = ɛ α ψ α (x) 4. Compute a new density n(r) = N α=1 ψ α(x) 2 other observables are functionals of {ψ α, ɛ α }

143 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi) 2. Evaluate local single-particle potential v KS (r) v(r) J 0 (r) 3. Solve for lowest N states (including degeneracies): {ψ α, ɛ α } [ 2 2M + v KS(r) ] ψ α (x) = ɛ α ψ α (x) 4. Compute a new density n(r) = N α=1 ψ α(x) 2 other observables are functionals of {ψ α, ɛ α } 5. Repeat until changes are small ( self-consistent )

144 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Dilute Fermi Gas in a Harmonic Trap Iteration procedure: 1. Guess an initial density profile n(r) (e.g., Thomas-Fermi) 2. Evaluate local single-particle potential v KS (r) v(r) J 0 (r) 3. Solve for lowest N states (including degeneracies): {ψ α, ɛ α } [ 2 2M + v KS(r) ] ψ α (x) = ɛ α ψ α (x) 4. Compute a new density n(r) = N α=1 ψ α(x) 2 other observables are functionals of {ψ α, ɛ α } 5. Repeat until changes are small ( self-consistent ) Looks like a simple Hartree calculation!

145 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Check Out An Example 4 Dilute Fermi Gas in Harmonic Trap N F =7, A=240, ν=2, a 0 = C 0 = 0 (noninteracting) 3 ρ(r/b) 2 E/A <k F a s > r/b

146 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Check Out An Example 4 3 Dilute Fermi Gas in Harmonic Trap N F =7, A=240, ν=2, a 0 = C 0 = 0 (noninteracting) Kohn-Sham LO ρ(r/b) 2 E/A <k F a s > r/b

147 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Check Out An Example 4 Dilute Fermi Gas in Harmonic Trap N F =7, A=240, ν=2, a 0 = C 0 = 0 (noninteracting) Kohn-Sham LO Kohn-Sham NLO (LDA) ρ(r/b) 2 1 E/A <k F a s > r/b

148 Outline Systems EFT Dilute DFT Future Intro Thermo DFT/EFT Results Check Out An Example 4 Dilute Fermi Gas in Harmonic Trap N F =7, A=240, ν=2, a 0 = C 0 = 0 (noninteracting) Kohn-Sham LO Kohn-Sham NLO (LDA) Kohn-Sham NNLO (LDA) ρ(r/b) 2 1 E/A <k F a s > r/b

Bayesian Fitting in Effective Field Theory

Bayesian Fitting in Effective Field Theory Bayesian Fitting in Effective Field Theory Department of Physics Ohio State University February, 26 Collaborators: D. Phillips (Ohio U.), U. van Kolck (Arizona), R.G.E. Timmermans (Groningen, Nijmegen)

More information

Fermion Many-Body Systems II

Fermion Many-Body Systems II Outline Atoms Stars Answer RG Department of Physics Ohio State University June, 2004 Outline Outline Atoms Stars Answer RG Universality (Un)like Overview of Cold Atoms Overview of Neutron Stars Answer:

More information

Effective Field Theory for Density Functional Theory II

Effective Field Theory for Density Functional Theory II Effective Field Theory for Density Functional Theory II Department of Physics Ohio State University February, 2006 I. Overview of EFT, RG, DFT for fermion many-body systems II. EFT/DFT for dilute Fermi

More information

Covariant Density Functional Theory

Covariant Density Functional Theory Outline DFT Action Dilute Renormalization Summary Covariant Density Functional Theory Department of Physics Ohio State University September, 2004 Outline DFT Action Dilute Renormalization Summary Covariant

More information

Density Functional Theory and Effective Field Theory

Density Functional Theory and Effective Field Theory Outline Skyrme DFT Sources Pairing Future Density Functional Theory and Effective Field Theory Department of Physics Ohio State University September, 2004 Outline Skyrme DFT Sources Pairing Future Density

More information

Effective Field Theory for Density Functional Theory I

Effective Field Theory for Density Functional Theory I Effective Field Theory for Density Functional Theory I Department of Physics Ohio State University February, 26 I. Overview of EFT, RG, DFT for fermion many-body systems II. EFT/DFT for dilute Fermi systems

More information

Nuclear Forces / DFT for Nuclei III

Nuclear Forces / DFT for Nuclei III Nuclear Forces / DFT for Nuclei III Department of Physics Ohio State University August, 2008 I. Overview of EFT/RG. II. Chiral effective field theory. III. RG for nuclear forces. EFT for many-body systems.

More information

Effective Field Theory and. the Nuclear Many-Body Problem

Effective Field Theory and. the Nuclear Many-Body Problem Effective Field Theory and the Nuclear Many-Body Problem Thomas Schaefer North Carolina State University 1 Schematic Phase Diagram of Dense Matter T nuclear matter µ e neutron matter? quark matter µ 2

More information

Effective Field Theory and. the Nuclear Many-Body Problem

Effective Field Theory and. the Nuclear Many-Body Problem Effective Field Theory and the Nuclear Many-Body Problem Thomas Schaefer North Carolina State University 1 Nuclear Effective Field Theory Low Energy Nucleons: Nucleons are point particles Interactions

More information

Renormalization group methods in nuclear few- and many-body problems

Renormalization group methods in nuclear few- and many-body problems Renormalization group methods in nuclear few- and many-body problems Lecture 2 S.K. Bogner (NSCL/MSU) 2011 National Nuclear Physics Summer School University of North Carolina at Chapel Hill Lecture 2 outline

More information

From Density Functional Theory to Generalized Skyrme

From Density Functional Theory to Generalized Skyrme Outline Action Sources Pairing Summary From Density Functional Theory to Generalized Skyrme Department of Physics Ohio State University December, 2004 Outline Action Sources Pairing Summary From Density

More information

Atomic Nuclei at Low Resolution

Atomic Nuclei at Low Resolution Atomic Department of Physics Ohio State University November, 29 Collaborators: E. Anderson, S. Bogner, S. Glazek, E. Jurgenson, R. Perry, S. Ramanan, A. Schwenk + UNEDF collaboration Overview DOFs EFT

More information

Nuclear structure I: Introduction and nuclear interactions

Nuclear structure I: Introduction and nuclear interactions Nuclear structure I: Introduction and nuclear interactions Stefano Gandolfi Los Alamos National Laboratory (LANL) National Nuclear Physics Summer School Massachusetts Institute of Technology (MIT) July

More information

Renormalization Group Methods for the Nuclear Many-Body Problem

Renormalization Group Methods for the Nuclear Many-Body Problem Renormalization Group Methods for the Nuclear Many-Body Problem A. Schwenk a,b.friman b and G.E. Brown c a Department of Physics, The Ohio State University, Columbus, OH 41 b Gesellschaft für Schwerionenforschung,

More information

Renormalization group methods in nuclear few- and many-body problems

Renormalization group methods in nuclear few- and many-body problems Renormalization group methods in nuclear few- and many-body problems Lecture 1 S.K. Bogner (NSCL/MSU) 2011 National Nuclear Physics Summer School University of North Carolina at Chapel Hill Useful readings

More information

Lattice Simulations with Chiral Nuclear Forces

Lattice Simulations with Chiral Nuclear Forces Lattice Simulations with Chiral Nuclear Forces Hermann Krebs FZ Jülich & Universität Bonn July 23, 2008, XQCD 2008, NCSU In collaboration with B. Borasoy, E. Epelbaum, D. Lee, U. Meißner Outline EFT and

More information

Modern Theory of Nuclear Forces

Modern Theory of Nuclear Forces Evgeny Epelbaum, FZ Jülich & University Bonn Lacanau, 29.09.2009 Modern Theory of Nuclear Forces Lecture 1: Lecture 2: Lecture 3: Introduction & first look into ChPT EFTs for two nucleons Nuclear forces

More information

RG & EFT for nuclear forces

RG & EFT for nuclear forces RG & EFT for nuclear forces Andreas Nogga, Forschungszentrum Jülich ECT* school, Feb/March 2006 Low momentum interactions: Using the RG to simplify the nuclear force for many-body calculations. Application

More information

Renormalization group methods in nuclear few- and many-body problems

Renormalization group methods in nuclear few- and many-body problems Renormalization group methods in nuclear few- and many-body problems Lecture 1 S.K. Bogner (NSCL/MSU) 2011 National Nuclear Physics Summer School University of North Carolina at Chapel Hill Useful readings

More information

Simplifying the Nuclear Many-Body Problem with Low-Momentum Interactions

Simplifying the Nuclear Many-Body Problem with Low-Momentum Interactions Simplifying the Nuclear Many-Body Problem with Low-Momentum Interactions Scott Bogner September 2005 Collaborators: Dick Furnstahl, Achim Schwenk, and Andreas Nogga The Conventional Nuclear Many-Body Problem

More information

At the end of Section 4, a summary of basic principles for low-energy effective theories was given, which we recap here.

At the end of Section 4, a summary of basic principles for low-energy effective theories was given, which we recap here. Nuclear Forces 2 (last revised: September 30, 2014) 6 1 6. Nuclear Forces 2 a. Recap: Principles of low-energy effective theories Figure 1: Left: high-resolution, with wavelength of probe short compared

More information

PoS(Confinement8)147. Universality in QCD and Halo Nuclei

PoS(Confinement8)147. Universality in QCD and Halo Nuclei Helmholtz-Institut für Strahlen- und Kernphysik (Theorie) and Bethe Center for Theoretical Physics, University of Bonn, Germany E-mail: hammer@itkp.uni-bonn.de Effective Field Theory (EFT) provides a powerful

More information

Coupled-cluster theory for medium-mass nuclei

Coupled-cluster theory for medium-mass nuclei Coupled-cluster theory for medium-mass nuclei Thomas Papenbrock and G. Hagen (ORNL) D. J. Dean (ORNL) M. Hjorth-Jensen (Oslo) A. Nogga (Juelich) A. Schwenk (TRIUMF) P. Piecuch (MSU) M. Wloch (MSU) Seattle,

More information

Ultracold atoms and neutron-rich matter in nuclei and astrophysics

Ultracold atoms and neutron-rich matter in nuclei and astrophysics Ultracold atoms and neutron-rich matter in nuclei and astrophysics Achim Schwenk NORDITA program Pushing the boundaries with cold atoms Stockholm, Jan. 23, 2013 Outline Advances in nuclear forces 3N forces

More information

Towards a model-independent low momentum nucleon-nucleon interaction

Towards a model-independent low momentum nucleon-nucleon interaction Towards a model-independent low momentum nucleon-nucleon interaction S.K. Bogner a, T.T.S. Kuo a 2, A. Schwenk a 3, D.R. Entem b and R. Machleidt b arxiv:nucl-th/84v3 22 Oct 23 Abstract a Department of

More information

The theory of nuclear forces: Is the never-ending ending story coming to an end? R. Machleidt University of Idaho

The theory of nuclear forces: Is the never-ending ending story coming to an end? R. Machleidt University of Idaho The theory of nuclear forces: Is the never-ending ending story coming to an end? University of Idaho What s left to say? Put the recent progress into a wider perspective. Fill in some missing details.

More information

Quantum Monte Carlo calculations of medium mass nuclei

Quantum Monte Carlo calculations of medium mass nuclei Quantum Monte Carlo calculations of medium mass nuclei Diego Lonardoni FRIB Theory Fellow In collaboration with: J. Carlson, LANL S. Gandolfi, LANL X. Wang, Huzhou University, China A. Lovato, ANL & UniTN

More information

Applications of Renormalization Group Methods in Nuclear Physics 2

Applications of Renormalization Group Methods in Nuclear Physics 2 Applications of Renormalization Group Methods in Nuclear Physics 2 Dick Furnstahl Department of Physics Ohio State University HUGS 2014 Outline: Lecture 2 Lecture 2: SRG in practice Recap from lecture

More information

Renormalization and power counting of chiral nuclear forces. 龙炳蔚 (Bingwei Long) in collaboration with Chieh-Jen Jerry Yang (U.

Renormalization and power counting of chiral nuclear forces. 龙炳蔚 (Bingwei Long) in collaboration with Chieh-Jen Jerry Yang (U. Renormalization and power counting of chiral nuclear forces 龙炳蔚 (Bingwei Long) in collaboration with Chieh-Jen Jerry Yang (U. Arizona) What are we really doing? Correcting Weinberg's scheme about NN contact

More information

Nuclear structure Anatoli Afanasjev Mississippi State University

Nuclear structure Anatoli Afanasjev Mississippi State University Nuclear structure Anatoli Afanasjev Mississippi State University 1. Nuclear theory selection of starting point 2. What can be done exactly (ab-initio calculations) and why we cannot do that systematically?

More information

Three-nucleon forces and neutron-rich nuclei

Three-nucleon forces and neutron-rich nuclei Three-nucleon forces and neutron-rich nuclei Achim Schwenk Facets of Strong Interaction Physics Hirschegg 40 + Bengt 60, Jan. 18, 2012 Happy Birthday Bengt! Outline Understanding three-nucleon forces Three-body

More information

RG & EFT for nuclear forces

RG & EFT for nuclear forces RG & EFT for nuclear forces Andreas Nogga, Forschungszentrum Jülich ECT* school, Feb/March 2006 Low momentum interactions: Using the RG to simplify the nuclear force for many-body calculations. Application

More information

Evgeny Epelbaum. Forschungszentrum Jülich & Universität Bonn

Evgeny Epelbaum. Forschungszentrum Jülich & Universität Bonn Evgeny Epelbaum KHuK Jahrestagung, GSI, 25.10.2007 Evgeny Epelbaum Forschungszentrum Jülich & Universität Bonn Outline Motivation & Introduction Few nucleons in chiral EFT: where do we stand Work in progress:

More information

Nuclear structure III: Nuclear and neutron matter. National Nuclear Physics Summer School Massachusetts Institute of Technology (MIT) July 18-29, 2016

Nuclear structure III: Nuclear and neutron matter. National Nuclear Physics Summer School Massachusetts Institute of Technology (MIT) July 18-29, 2016 Nuclear structure III: Nuclear and neutron matter Stefano Gandolfi Los Alamos National Laboratory (LANL) National Nuclear Physics Summer School Massachusetts Institute of Technology (MIT) July 18-29, 2016

More information

The NN system: why and how we iterate

The NN system: why and how we iterate The NN system: why and how we iterate Daniel Phillips Ohio University Research supported by the US department of energy Plan Why we iterate I: contact interactions Why we iterate II: pion exchange How

More information

Microscopically Based Energy Functionals. S.K. Bogner (NSCL/MSU)

Microscopically Based Energy Functionals. S.K. Bogner (NSCL/MSU) Microscopically Based Energy Functionals S.K. Bogner (NSCL/MSU) Dream Scenario: From QCD to Nuclei 2 SciDAC 2 Project Building a Universal Nuclear Energy Density Functional See http://undef.org for details

More information

Modern Theory of Nuclear Forces

Modern Theory of Nuclear Forces Evgeny Epelbaum, FZ Jülich & University Bonn Lacanau, 28.09.2009 Modern Theory of Nuclear Forces Lecture 1: Lecture 2: Introduction & first look into ChPT EFTs for two nucleons Chiral Perturbation Theory

More information

INTRODUCTION TO EFFECTIVE FIELD THEORIES OF QCD

INTRODUCTION TO EFFECTIVE FIELD THEORIES OF QCD INTRODUCTION TO EFFECTIVE FIELD THEORIES OF QCD U. van Kolck Institut de Physique Nucléaire d Orsay and University of Arizona Supported in part by CNRS, Université Paris Sud, and US DOE Outline Effective

More information

Alex Gezerlis. New Ideas in Constraining Nuclear Forces ECT*, Trento, Italy June 5, 2018

Alex Gezerlis. New Ideas in Constraining Nuclear Forces ECT*, Trento, Italy June 5, 2018 Quantum Monte Carlo interactions with From microscopic to effective Chiral Effective Field Theory Interactions using Quantum Monte Carlo Alex Gezerlis New Ideas in Constraining Nuclear Forces ECT*, Trento,

More information

Quantum Monte Carlo calculations with chiral Effective Field Theory Interactions

Quantum Monte Carlo calculations with chiral Effective Field Theory Interactions Quantum Monte Carlo calculations with chiral Effective Field Theory Interactions Alexandros Gezerlis East Lansing, MI 3rd International Symposium on Nuclear Symmetry Energy July 25, 2013 Motivation for

More information

Nuclear Physics from Lattice Effective Field Theory

Nuclear Physics from Lattice Effective Field Theory Nuclear Physics from Lattice Effective Field Theory Dean Lee (NCSU/Bonn) work done in collaboration with Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Ulf-G. Meißner (Bonn/Jülich) Buḡra Borasoy (now

More information

Neutron-rich matter and neutrino-matter interactions based on chiral effective field theory

Neutron-rich matter and neutrino-matter interactions based on chiral effective field theory Neutron-rich matter and neutrino-matter interactions based on chiral effective field theory Achim Schwenk Astrophysical Transients: Multi-Messenger Probes of Nuclear Physics INT, July 29, 2011 Outline

More information

Coupled-cluster theory for nuclei

Coupled-cluster theory for nuclei Coupled-cluster theory for nuclei Thomas Papenbrock and G. Hagen D. J. Dean M. Hjorth-Jensen B. Velamur Asokan INT workshop Weakly-bound systems in atomic and nuclear physics Seattle, March 8-12, 2010

More information

POWER COUNTING WHAT? WHERE?

POWER COUNTING WHAT? WHERE? POWER COUNTING WHAT? WHERE? U. van Kolck Institut de Physique Nucléaire d Orsay and University of Arizona Supported by CNRS and US DOE 1 Outline Meeting the elephant What? Where? Walking out of McDonald

More information

Dense Matter for Dummies (Non-Experts)

Dense Matter for Dummies (Non-Experts) for Dummies (Non-Experts) Department of Physics Ohio State University July, 26 Pictures have been freely borrowed from online sources; I apologize in advance for any omitted citations. Also, inclusion

More information

Neutron matter from chiral effective field theory interactions

Neutron matter from chiral effective field theory interactions Neutron matter from chiral effective field theory interactions Ingo Tews, In collaboration with K. Hebeler, T. Krüger, A. Schwenk, JINA Neutron Stars, May 26, 2016, Athens, OH Chiral effective field theory

More information

Few-nucleon contributions to π-nucleus scattering

Few-nucleon contributions to π-nucleus scattering Mitglied der Helmholtz-Gemeinschaft Few-nucleon contributions to π-nucleus scattering Andreas Nogga, Forschungszentrum Jülich INT Program on Simulations and Symmetries: Cold Atoms, QCD, and Few-hadron

More information

Effective Field Theory for Density Functional Theory III

Effective Field Theory for Density Functional Theory III Effective Field Theory for Density Functional Theory III Department of Physics Ohio State University September, 25 I. Overview of EFT, RG, DFT for fermion many-body systems II. EFT/DFT for dilute Fermi

More information

Local chiral NN potentials and the structure of light nuclei

Local chiral NN potentials and the structure of light nuclei Local chiral NN potentials and the structure of light nuclei Maria Piarulli @ELBA XIV WORKSHOP June 7-July 1 16, Marciana Marina, Isola d Elba PHYSICAL REVIEW C 91, 43(15) Minimally nonlocal nucleon-nucleon

More information

Light hypernuclei based on chiral and phenomenological interactions

Light hypernuclei based on chiral and phenomenological interactions Mitglied der Helmholtz-Gemeinschaft Light hypernuclei based on chiral and phenomenological interactions Andreas Nogga, Forschungszentrum Jülich International Conference on Hypernuclear and Strange Particle

More information

The oxygen anomaly F O

The oxygen anomaly F O The oxygen anomaly O F The oxygen anomaly - not reproduced without 3N forces O F without 3N forces, NN interactions too attractive many-body theory based on two-nucleon forces: drip-line incorrect at 28

More information

Renormalization group methods in nuclear few- and many-body problems

Renormalization group methods in nuclear few- and many-body problems Renormalization group methods in nuclear few- and many-body problems Lecture 3 S.K. Bogner (NSCL/MSU) 2011 National Nuclear Physics Summer School University of North Carolina at Chapel Hill Lecture 2 outline

More information

Small bits of cold, dense matter

Small bits of cold, dense matter Small bits of cold, dense matter Alessandro Roggero (LANL) with: S.Gandolfi & J.Carlson (LANL), J.Lynn (TUD) and S.Reddy (INT) ArXiv:1712.10236 Nuclear ab initio Theories and Neutrino Physics INT - Seattle

More information

Pairing in Nuclear and Neutron Matter Screening effects

Pairing in Nuclear and Neutron Matter Screening effects Pairing Degrees of Freedom in Nuclei and Nuclear Medium Seattle, Nov. 14-17, 2005 Outline: Pairing in Nuclear and Neutron Matter Screening effects U. Lombardo pairing due to the nuclear (realistic) interaction

More information

Quantum Monte Carlo calculations of neutron and nuclear matter

Quantum Monte Carlo calculations of neutron and nuclear matter Quantum Monte Carlo calculations of neutron and nuclear matter Stefano Gandolfi Los Alamos National Laboratory (LANL) Advances and perspectives in computational nuclear physics, Hilton Waikoloa Village,

More information

The Nuclear Many-Body Problem

The Nuclear Many-Body Problem The Nuclear Many-Body Problem relativistic heavy ions vacuum electron scattering quarks gluons radioactive beams heavy few nuclei body quark-gluon soup QCD nucleon QCD few body systems many body systems

More information

The nucleon-nucleon system in chiral effective theory

The nucleon-nucleon system in chiral effective theory The nucleon-nucleon system in chiral effective theory Daniel Phillips Ohio University Research supported by the US Department of Energy Plan χet for nuclear forces: the proposal Leading order for S waves

More information

Nuclear few- and many-body systems in a discrete variable representation basis

Nuclear few- and many-body systems in a discrete variable representation basis Nuclear few- and many-body systems in a discrete variable representation basis Jeremy W. Holt* Department of Physics University of Washington *with A. Bulgac, M. M. Forbes L. Coraggio, N. Itaco, R. Machleidt,

More information

Quantum Monte Carlo with

Quantum Monte Carlo with Quantum Monte Carlo with QuantumField Monte Carlo Interactions with Chiral Effective Theory Chiral Effective Field Theory Interactions From matter to nuclei Alexandros Gezerlis ECT*-EMMI Workshop Neutron-Rich

More information

Neutron Matter: EOS, Spin and Density Response

Neutron Matter: EOS, Spin and Density Response Neutron Matter: EOS, Spin and Density Response LANL : A. Gezerlis, M. Dupuis, S. Reddy, J. Carlson ANL: S. Pieper, R.B. Wiringa How can microscopic theories constrain mean-field theories and properties

More information

Three-Body Bound State Calculations by Using Three-Dimensional Low Momentum Interaction V low k

Three-Body Bound State Calculations by Using Three-Dimensional Low Momentum Interaction V low k Preprint number: 6.668 Three-Body Bound State Calculations by Using Three-Dimensional Low Momentum Interaction V low k arxiv:6.668v [nucl-th Feb M. R. Hadizadeh, Institute of Nuclear and Particle Physics,

More information

Ab Initio Nuclear Structure Theory

Ab Initio Nuclear Structure Theory Ab Initio Nuclear Structure Theory Lecture 1: Hamiltonian Robert Roth Overview Lecture 1: Hamiltonian Prelude Many-Body Quantum Mechanics Nuclear Hamiltonian Matrix Elements Lecture 2: Correlations Two-Body

More information

Few Body Methods in Nuclear Physics - Lecture I

Few Body Methods in Nuclear Physics - Lecture I Few Body Methods in Nuclear Physics - Lecture I Nir Barnea The Hebrew University, Jerusalem, Israel Sept. 2010 Course Outline 1 Introduction - Few-Body Nuclear Physics 2 Gaussian Expansion - The Stochastic

More information

Constraints on neutron stars from nuclear forces

Constraints on neutron stars from nuclear forces Constraints on neutron stars from nuclear forces Achim Schwenk Workshop on the formation and evolution of neutron stars Bonn, Feb. 27, 2012 Main points Advances in nuclear forces and nuclear matter theory

More information

Part III: The Nuclear Many-Body Problem

Part III: The Nuclear Many-Body Problem Part III: The Nuclear Many-Body Problem To understand the properties of complex nuclei from first principles Microscopic Valence- Space Interactions Model spaces Many-body perturbation theory (MBPT) Calculating

More information

Some new developments in relativistic point-coupling models

Some new developments in relativistic point-coupling models Some new developments in relativistic point-coupling models T. J. Buervenich 1, D. G. Madland 1, J. A. Maruhn 2, and P.-G. Reinhard 3 1 Los Alamos National Laboratory 2 University of Frankfurt 3 University

More information

NN-Correlations in the spin symmetry energy of neutron matter

NN-Correlations in the spin symmetry energy of neutron matter NN-Correlations in the spin symmetry energy of neutron matter Symmetry energy of nuclear matter Spin symmetry energy of neutron matter. Kinetic and potential energy contributions. A. Rios, I. Vidaña, A.

More information

THE THREE NUCLEON SYSTEM AT LEADING ORDER OF CHIRAL EFFECTIVE THEORY

THE THREE NUCLEON SYSTEM AT LEADING ORDER OF CHIRAL EFFECTIVE THEORY THE THREE NUCLEON SYSTEM AT LEADING ORDER OF CHIRAL EFFECTIVE THEORY Young-Ho Song(RISP, Institute for Basic Science) Collaboration with R. Lazauskas( IPHC, IN2P3-CNRS) U. van Kolck (Orsay, IPN & Arizona

More information

TRIUMF. Three-body forces in nucleonic matter. Weakly-Bound Systems in Atomic and Nuclear Physics. Kai Hebeler (TRIUMF) INT, Seattle, March 11, 2010

TRIUMF. Three-body forces in nucleonic matter. Weakly-Bound Systems in Atomic and Nuclear Physics. Kai Hebeler (TRIUMF) INT, Seattle, March 11, 2010 Three-body forces in nucleonic matter Kai Hebeler (TRIUMF) INT, Seattle, March 11, 21 TRIUMF A. Schwenk, T. Duguet, T. Lesinski, S. Bogner, R. Furnstahl Weakly-Bound Systems in Atomic and Nuclear Physics

More information

Quantum Monte Carlo calculations of two neutrons in finite volume

Quantum Monte Carlo calculations of two neutrons in finite volume Quantum Monte Carlo calculations of two neutrons in finite volume Philipp Klos with J. E. Lynn, I. Tews, S. Gandolfi, A. Gezerlis, H.-W. Hammer, M. Hoferichter, and A. Schwenk Nuclear Physics from Lattice

More information

Effective Field Theory for Cold Atoms I

Effective Field Theory for Cold Atoms I Effective Field Theory for Cold Atoms I H.-W. Hammer Institut für Kernphysik, TU Darmstadt and Extreme Matter Institute EMMI School on Effective Field Theory across Length Scales, ICTP-SAIFR, Sao Paulo,

More information

Recent results in lattice EFT for nuclei

Recent results in lattice EFT for nuclei Recent results in lattice EFT for nuclei Dean Lee (NC State) Nuclear Lattice EFT Collaboration Centro de Ciencias de Benasque Pedro Pascua Bound states and resonances in EFT and Lattice QCD calculations

More information

E. Fermi: Notes on Thermodynamics and Statistics (1953))

E. Fermi: Notes on Thermodynamics and Statistics (1953)) E. Fermi: Notes on Thermodynamics and Statistics (1953)) Neutron stars below the surface Surface is liquid. Expect primarily 56 Fe with some 4 He T» 10 7 K ' 1 KeV >> T melting ( 56 Fe) Ionization: r Thomas-Fermi

More information

Relativistic point-coupling models for finite nuclei

Relativistic point-coupling models for finite nuclei Relativistic point-coupling models for finite nuclei T. J. Buervenich 1, D. G. Madland 1, J. A. Maruhn 2, and P.-G. Reinhard 3 1 Los Alamos National Laboratory 2 University of Frankfurt 3 University of

More information

Chiral effective field theory on the lattice: Ab initio calculations of nuclei

Chiral effective field theory on the lattice: Ab initio calculations of nuclei Chiral effective field theory on the lattice: Ab initio calculations of nuclei Nuclear Lattice EFT Collaboration Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Timo Lähde (Jülich) Dean Lee (NC State)

More information

arxiv:nucl-th/ v1 5 Jan 2007

arxiv:nucl-th/ v1 5 Jan 2007 Are low-energy nuclear observables sensitive to high-energy phase shifts? S.K. Bogner 1, R.J. Furnstahl 1, R.J. Perry 1, A. Schwenk 2 arxiv:nucl-th/711v1 5 Jan 27 1 Department of Physics, The Ohio State

More information

New Frontiers in Nuclear Structure Theory

New Frontiers in Nuclear Structure Theory New Frontiers in Nuclear Structure Theory From Realistic Interactions to the Nuclear Chart Robert Roth Institut für Kernphysik Technical University Darmstadt Overview Motivation Nucleon-Nucleon Interactions

More information

Nucleon-nucleon interaction in covariant chiral effective field theory

Nucleon-nucleon interaction in covariant chiral effective field theory Guilin, China The Seventh Asia-Pacific Conference on Few-Body Problems in Physics Nucleon-nucleon interaction in covariant chiral effective field theory Xiu-Lei Ren School of Physics, Peking University

More information

Nuclear Structure and Reactions using Lattice Effective Field Theory

Nuclear Structure and Reactions using Lattice Effective Field Theory Nuclear Structure and Reactions using Lattice Effective Field Theory Dean Lee North Carolina State University Nuclear Lattice EFT Collaboration Frontiers of Nuclear Physics Kavli Institute for Theoretical

More information

Nuclear structure from chiral-perturbation-theory two- plus three-nucleon interactions

Nuclear structure from chiral-perturbation-theory two- plus three-nucleon interactions Nuclear structure from chiral-perturbation-theory two- plus three-nucleon interactions Petr Navratil Lawrence Livermore National Laboratory* Collaborators: W. E. Ormand (LLNL), J. P. Vary (ISU), E. Caurier

More information

Effective Field Theory and Finite-Density Systems

Effective Field Theory and Finite-Density Systems ANNUAL REVIEWS Further Click here for quick links to Annual Reviews content online, including: Other articles in this volume Top cited articles Top downloaded articles Our comprehensive search Effective

More information

Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 1

Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 1 2358-19 Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation 6-17 August 2012 Introduction to Nuclear Physics - 1 P. Van Isacker GANIL, Grand Accelerateur National d'ions Lourds

More information

arxiv: v1 [nucl-th] 31 Oct 2013

arxiv: v1 [nucl-th] 31 Oct 2013 Renormalization Group Invariance in the Subtractive Renormalization Approach to the NN Interactions S. Szpigel and V. S. Timóteo arxiv:1311.61v1 [nucl-th] 31 Oct 13 Faculdade de Computação e Informática,

More information

Effective Field Theory for Nuclear Physics! Akshay Vaghani! Mississippi State University!

Effective Field Theory for Nuclear Physics! Akshay Vaghani! Mississippi State University! Effective Field Theory for Nuclear Physics! Akshay Vaghani! Mississippi State University! Overview! Introduction! Basic ideas of EFT! Basic Examples of EFT! Algorithm of EFT! Review NN scattering! NN scattering

More information

arxiv:nucl-th/ v1 12 Feb 2007

arxiv:nucl-th/ v1 12 Feb 2007 EFT for DFT R.J. Furnstahl arxiv:nucl-th/74v Feb 7 Department of Physics, Ohio State University, Columbus, OH 43 furnstahl.@osu.edu These lectures give an overview of the ongoing application of effective

More information

Few- Systems. Selected Topics in Correlated Hyperspherical Harmonics. Body. A. Kievsky

Few- Systems. Selected Topics in Correlated Hyperspherical Harmonics. Body. A. Kievsky Few-Body Systems 0, 11 16 (2003) Few- Body Systems c by Springer-Verlag 2003 Printed in Austria Selected Topics in Correlated Hyperspherical Harmonics A. Kievsky INFN and Physics Department, Universita

More information

NUCLEAR FORCES. Historical perspective

NUCLEAR FORCES. Historical perspective NUCLEAR FORCES Figure 1: The atomic nucleus made up from protons (yellow) and neutrons (blue) and held together by nuclear forces. Nuclear forces (also known as nuclear interactions or strong forces) are

More information

Physics 795 Nuclear Theory at OSU

Physics 795 Nuclear Theory at OSU Physics 795 Nuclear Theory at OSU Department of Physics Ohio State University October, 2006 Nuclear Theory Group Bunny Clark Ulrich Heinz Sabine Jeschonnek Yuri Kovchegov Robert Perry Current Students/Postdocs

More information

Nuclear physics: a laboratory for many-particle quantum mechanics or From model to theory in nuclear structure physics

Nuclear physics: a laboratory for many-particle quantum mechanics or From model to theory in nuclear structure physics Nuclear physics: a laboratory for many-particle quantum mechanics or From model to theory in nuclear structure physics G.F. Bertsch University of Washington Stockholm University and the Royal Institute

More information

Quantum Theory of Many-Particle Systems, Phys. 540

Quantum Theory of Many-Particle Systems, Phys. 540 Quantum Theory of Many-Particle Systems, Phys. 540 Questions about organization Second quantization Questions about last class? Comments? Similar strategy N-particles Consider Two-body operators in Fock

More information

Similarity renormalization group for nucleon-nucleon interactions

Similarity renormalization group for nucleon-nucleon interactions PHYSICAL REVIEW C 75, 0600(R) (2007) Similarity renormalization group for nucleon-nucleon interactions S. K. Bogner, * R. J. Furnstahl, and R. J. Perry Department of Physics, The Ohio State University,

More information

Mean-field concept. (Ref: Isotope Science Facility at Michigan State University, MSUCL-1345, p. 41, Nov. 2006) 1/5/16 Volker Oberacker, Vanderbilt 1

Mean-field concept. (Ref: Isotope Science Facility at Michigan State University, MSUCL-1345, p. 41, Nov. 2006) 1/5/16 Volker Oberacker, Vanderbilt 1 Mean-field concept (Ref: Isotope Science Facility at Michigan State University, MSUCL-1345, p. 41, Nov. 2006) 1/5/16 Volker Oberacker, Vanderbilt 1 Static Hartree-Fock (HF) theory Fundamental puzzle: The

More information

Toward a unified description of equilibrium and dynamics of neutron star matter

Toward a unified description of equilibrium and dynamics of neutron star matter Toward a unified description of equilibrium and dynamics of neutron star matter Omar Benhar INFN and Department of Physics Sapienza Università di Roma I-00185 Roma, Italy Based on work done in collaboration

More information

Three-nucleon potentials in nuclear matter. Alessandro Lovato

Three-nucleon potentials in nuclear matter. Alessandro Lovato Three-nucleon potentials in nuclear matter Alessandro Lovato PRC 83, 054003 (2011) arxiv:1109.5489 Outline Ab initio many body method Nuclear Hamiltonian: 2- and 3- body potentials Density dependent potential

More information

Shell evolution and pairing in calcium isotopes with two- and three-body forces

Shell evolution and pairing in calcium isotopes with two- and three-body forces Shell evolution and pairing in calcium isotopes with two- and three-body forces Javier Menéndez Institut für Kernphysik, TU Darmstadt ExtreMe Matter Institute (EMMI) with Jason D. Holt, Achim Schwenk and

More information

FROM QCD TO NUCLEI: ASPECTS OF NUCLEAR THEORY IN FRANCE

FROM QCD TO NUCLEI: ASPECTS OF NUCLEAR THEORY IN FRANCE FROM QCD TO NUCLEI: ASPECTS OF NUCLEAR THEORY IN FRANCE Ubirajara van Kolck Institut de Physique Nucléaire 1 Outline Hadronic theory in France Nuclear forces from QCD Low-energy nuclear theory in France

More information

Three-nucleon forces and shell structure of neutron-rich Ca isotopes

Three-nucleon forces and shell structure of neutron-rich Ca isotopes Three-nucleon forces and shell structure of neutron-rich Ca isotopes Javier Menéndez Institut für Kernphysik (TU Darmstadt) and ExtreMe Matter Institute (EMMI) NUSTAR Week 3, Helsinki, 9 October 13 Outline

More information

Pionless EFT for Few-Body Systems

Pionless EFT for Few-Body Systems Pionless EFT for Few-Body Systems Betzalel Bazak Physique Theorique Institut de Physique Nucleaire d Orsay Nuclear Physics from Lattice QCD Insitute for Nuclear Theory April 7, 2016 Seattle Betzalel Bazak

More information

Ab initio lattice EFT from light to medium mass nuclei Nuclear Lattice EFT Collaboration

Ab initio lattice EFT from light to medium mass nuclei Nuclear Lattice EFT Collaboration Ab initio lattice EFT from light to medium mass nuclei Nuclear Lattice EFT Collaboration Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Timo Lähde (Jülich) Dean Lee (NC State) Thomas Luu (Jülich/Bonn)

More information

Intersections of nuclear physics and cold atom physics

Intersections of nuclear physics and cold atom physics Intersections of nuclear physics and cold atom physics Thomas Schaefer North Carolina State University Unitarity limit Consider simple square well potential a < 0 a =, ǫ B = 0 a > 0, ǫ B > 0 Unitarity

More information