Topological media: quantum liquids, topological insulators & quantum vacuum
|
|
- Joy McCoy
- 6 years ago
- Views:
Transcription
1 Topological media: quantum liquids, topological insulators & quantum vacuum Landau Institute G. Volovik CC-2010, Chernogolovka, July 26, Introduction: Universe as object of ultralow temperature physics * quantum vacuum as topological medium * effective quantum field theories emerging at low T 2. Fermi surface as topological object *normal 3He, metals, 3. Dirac (Fermi points as topological objects * superfluid 3He-A, semimetals, cuprate superconductors, graphene, vacuum of Standard Model of particle physics in massless phase * topological invariants for gapless 2D and 3D topological matter * QED, QCD and gravity as emergent phenomena * quantum vacuum as cryo-crystal, α-phase of superfluid 3He 4. Fully gapped topological media * superfluid 3He-B, topological insulators, chiral superconductors, vacuum of Standard Model of particle physics in present massive phase * topological invariants for gapped 2D and 3D topological matter * edge states & Majorana fermions ( planar phase of 3He & surface of 3He-B * intrinsic QHE & spin-qhe 5. Conclusion * important role of momentum-space topology
2 Torsion & spinning strings, torsion instanton Fermion zero modes on strings & walls Antigravitating (negative-mass string Gravitational Aharonov-Bohm effect Domain wall terminating on string String terminating on domain wall Monopoles on string & Boojums Witten superconducting string Soft core string, Q-balls Kibble mechanism Dark matter detector Primordial magnetic field Baryogenesis by textures Cosmological & Newton constants dark energy dark matter Effective gravity Bi-metric & conformal gravity Graviton, dilaton Spin connection Rotating vacuum Vacuum dynamics conformal anomaly & strings Inflation Branes matter creation vacuum gravity black holes ergoregion, event horizon Hawking & Unruh effects black hole entropy Vacuum instability Superfluidity of neutron star vortices, glitches shear flow instability neutron stars Z &W strings skyrmions Alice string Pion string cosmology Gravity QCD quark matter Quark condensate Nambu--Jona-Lasinio Vaks--Larkin Color superfluidity Savvidi vacuum cosmic strings 3 He nuclear physics physical vacuum High Energy Physics Plasma Physics Nuclei vs 3He droplet Shell model Pair-correlations Collective modes Quark confinement, QCD cosmology Intrinsic orbital momentum of quark matter Emergence & effective theories Weyl & Majorana fermions Vacuum polarization, screening - antiscreening, running coupling Symmetry breaking (anisotropy of vacuum Parity violation -- chiral fermions Vacuum instability in strong fields, pair production Casimir force, quantum friction Fermionic charge of vacuum Higgs fields & gauge bosons Momentum-space topology Hierarchy problem, Supersymmetry high-t & chiral superconductivity Condensed Matter Phenome nology phase transitions Neutrino oscillations Chiral anomaly & axions Spin & isospin, String theory CPT-violation, GUT low dimensional systems Bose condensates hydrodynamics disorder random anisotropy unity of physics 3 He Grand Unification Gap nodes Low -T scaling mixed state Broken time reversal 1/2-vortex, vortex dynamics Films: FQHE, Statistics & charge of skyrmions & vortices Edge states; spintronics 1D fermions in vortex core Critical fluctuations Mixture of condensates Vector & spinor condensates BEC of quasipartcles, magnon BEC & laser meron, skyrmion, 1/2 vortex General; relativistic; spin superfluidity multi-fluid rotating superfluid Shear flow instability quantum phase transitions & momentum-space topology Larkin- Imry-Ma Relativistic plasma topological insulator Magnetohydrodynamic Photon mass classes of random Turbulence of vortex lines Vortex Coulomb matrices propagating vortex front plasma velocity independent Reynolds number
3 3+1 sources of effective Quantum Field Theories in many-body system & quantum vacuum Lev Landau I think it is safe to say that no one understands Quantum Mechanics Richard Feynman Thermodynamics is the only physical theory of universal content Albert Einstein Symmetry: conservation laws, translational invariance, spontaneously broken symmetry, Grand Unification,... effective theories of quantum liquids: two-fluid hydrodynamics of superfluid 4 He & Fermi liquid theory of liquid 3 He Topology: you can't comb the hair on a ball smooth, anti-grand-unification missing ingredient in Landau theories
4 Landau view on a many body system many body systems are simple at low energy & temperature weakly excited state of liquid can be considered as system of "elementary excitations" Landau, 1941 equally applied to: superfluids, solids, & relativistic quantum vacuum helium liquids ground state + elementary excitations ground state = vacuum quasiparticles = elementary particles Universe vacuum + elementary particles why is low energy physics applicable to our vacuum?
5 characteristic high-energy scale in our vacuum is Planck energy E P =(hc 5 /G 1/ GeV10 32 K high-energy physics is extremely ultra-low energy physics highest energy in accelerators E ew 1 TeV K high-energy physics & cosmology belong to ultra-low temperature physics T of cosmic background radiation T CMBR 1 K E ew E Planck T CMBR E Planck cosmology is extremely ultra-low frequency physics cosmological expansion v(r,t = H(t r Hubble law H E Planck Hubble parameter our Universe is extremely close to equilibrium ground state We should study general properties of equilibrium ground states - quantum vacua
6 Why no freezing at low T? natural masses of elementary particles are of order of characteristic energy scale the Planck energy m E Planck 1019 GeV10 32 K even at highest temperature we can reach T 1 TeV1016 K everything should be completely frozen out e m/t =10 = , another great challenge?
7 main hierarchy puzzle cosmological constant puzzle m quarks, m leptons <<< E Planck 4 Λ <<<< E Planck its emergent physics solution: its emergent physics solution: m quarks = m leptons = 0 Λ = 0 reason: momentum-space topology of quantum vacuum reason: thermodynamics of quantum vacuum
8 Why no freezing at low T? massless particles & gapless excitations are not frozen out who protects massless excitations?
9 gapless fermions live near Fermi surface & Fermi point who protects Fermi surface & Fermi point? Topology we live because Fermi point is the hedgehog protected by topology p z p y Life protection p x Fermi point: hedgehog in momentum space hedgehog is stable: one cannot comb the hair on a ball smooth
10 tools Thermodynamics Topology in momentum space responsible for properties of vacuum energy problems of cosmological constant: perfect equilibrium Lorentz invariant vacuum has Λ = 0; perturbed vacuum has nonzero Λ on order of perturbation Λ <<<< E 4 Planck responsible for properties of fermionic and bosonic quantum fields in the background of quantum vacuum Fermi point in momentum space protected by topology is a source of massless Weyl fermions, gauge fields & gravity m quarks, m leptons <<< E Planck
11 Quantum vacuum as topological substance: universality classes physics at low T is determined by gapless excitations universality classes of gapless vacua topology is robust to deformations: nodes in spectrum survive interaction Horava, Kitaev, Ludwig, Schnyder, Ryu, Furusaki,...
12 2. Liquid 3 He & effective theory of vacuum with Fermi surface two major universality classes of gapless fermionic vacua Landau theory of Fermi liquid Standard Model + gravity vacuum with Fermi surface vacuum with Fermi point gravity emerges from Fermi point analog of Fermi surface g µν (p µ - ea µ - eτ.w µ (p ν - ea ν - eτ.w ν = 0
13 Topological stability of Fermi surface Energy spectrum of non-interacting gas of fermionic atoms E(p = E>0 empty levels Fermi surface E=0 p2 2m µ = E<0 p2 occupied levels: Fermi sea 2m p F 2m p=p F is Fermi surface a domain wall in momentum space? 2 Green's function G -1 = iω E(p ω Φ=2π Fermi surface: vortex ring in p-space p y (p z pf phase of Green's function G(ω,p= G e iφ has winding number N = 1 p x no! it is a vortex ring
14 Route to Landau Fermi-liquid is Fermi surface robust to interaction? Sure! Because of topology: winding number N=1 cannot change continuously, interaction cannot destroy singularity then Fermi surface survives in Fermi liquid? ω p y (p z pf p x Landau theory of Fermi liquid is topologically protected & thus is universal all metals have Fermi surface... Not only metals. Some superconductore too! Φ=2π Fermi surface: vortex line in p-space G(ω,p= G e iφ Stability conditions & Fermi surface topologies in a superconductor Gubankova-Schmitt-Wilczek, Phys.Rev. B74 (
15 quantized vortex in r-space Fermi surface in p-space Topology in r-space z homotopy group π 1 how is it in p-space? Topology in p-space ω y p y (p z vortex ring Φ=2π Ψ(r= Ψ e iφ scalar order parameter of superfluid & superconductor classes of mapping S 1 U(1 manifold of broken symmetry vacuum states x winding number N 1 = 1 Fermi surface Φ=2π G(ω,p= G e iφ pf Green's function (propagator p x classes of mapping S 1 GL(n,C space of non-degenerate complex matrices
16 3. Superfluid 3 He-A & Standard Model From Fermi surface to Fermi point z magnetic hedgehog vs right-handed electron y p z p y x p x again no difference? hedgehog in r-space σ(r=r ^ right-handed and left-handed massless quarks and leptons are elementary particles in Standard Model hedgehog in p-space ^ σ(p = p close to Fermi point Landau CP symmetry is emergent H = + c σ.p right-handed electron = hedgehog in p-space with spines = spins
17 E=cp p y (p z p x
18 where are Dirac particles? E=cp Dirac particle - composite object made of left and right particles p y (p z E p x p y (p z E=cp p x p y (p z p x E 2 = c 2 p 2 + m 2 mixing of left and right particles is secondary effect, which occurs at extremely low temperature T ew 1 TeV10 16 K
19
20 Fermi (Dirac points in 3+1 gapless topological matter topologically protected point nodes in: superfluid 3 He-A, triplet cold Fermi gases, semi-metal (Abrikosov-Beneslavskii N 3 = 1 eijk ds k g. ( p i 8π g pj g over 2D surface S in 3D p-space Gap node - Fermi point (anti-hedgehog N 3 = 1 p 1 E p y (p z N 3 =1 p 2 Gap node - Fermi point (hedgehog S 2 p x H = p2 2m µ c(p x ip y c(p x + ip y p2 + µ 2m g 3 (p g 1 (p +i g 2 (p = g 1 (p i g 2 (p g 3 (p
21 emergence of relativistic QFT near Fermi (Dirac point original non-relativistic Hamiltonian p2 c(p x + ip y H = 2m µ p2 c(p x ip y + µ 2m close to nodes, i.e. in low-energy corner relativistic chiral fermions emerge H = N 3 c τ.p E = ± cp chirality is emergent?? g 3 (p g 1 (p +i g 2 (p = g 1 (p i g 2 (p g 3 (p left-handed particles p 1 N 3 = 1 N 3 =1 p 2 right-handed particles top. invariant determines chirality in low-energy corner = τ.g(p E p y (p z p x what else is emergent? relativistic invariance as well
22 bosonic collective modes in two generic fermionic vacua Landau theory of Fermi liquid Standard Model + gravity collective Bose modes: Fermi surface collective Bose modes of fermionic vacuum: propagating oscillation of shape of Fermi surface Fermi point propagating oscillation of position of Fermi point p p - ea form effective dynamic electromagnetic field propagating oscillation of slopes A E 2 = c 2 p 2 g ik p i p k form effective dynamic gravity field Landau, ZhETF 32, 59 (1957 two generic quantum field theories of interacting bosonic & fermionic fields
23 relativistic quantum fields and gravity emerging near Fermi point Atiyah-Bott-Shapiro construction: linear expansion of Hamiltonian near the nodes in terms of Dirac Γ-matrices E = v F (p p F linear expansion near Fermi surface emergent relativity H = e k i Γ i 0.(p k p k linear expansion near Fermi point p z p y g µν (p µ - ea µ - eτ.w µ (p ν - ea ν - eτ.w ν = 0 hedgehog in p-space p x effective metric: emergent gravity effective electromagnetic field all ingredients of Standard Model : chiral fermions & gauge fields emerge in low-energy corner together with spin, Dirac Γ matrices, gravity & physical laws: Lorentz & gauge invariance, equivalence principle, etc effective SU(2 gauge field effective isotopic spin effective electric charge e = + 1 or 1 gravity & gauge fields are collective modes of vacua with Fermi point
24 quantum vacuum as cryo-crystal 4D graphene Michael Creutz JHEP 04 ( Fermi (Dirac points with Fermi (Dirac points with N 3 = +1 N 3 = 1
25 4. From Fermi point to intrinsic QHE & topological insulators N 3 = 1 eijk ds k g. ( p i 8π g pj g over 2D surface S in 3D momentum space 3+1vacuum with Fermi point dimensional reduction p y Fully gapped 2+1 system p x N 3 = 1 dp x dp y g. ( p x 4π g py g over the whole 2D momentum space or over 2D Brillouin zone
26 topological insulators & superconductors in 2+1 p-wave 2D superconductor, 3 He-A film, HgTe insulator quantum well H = p2 2m µ c(p x ip y c(p x + ip y p2 + µ 2m p 2 = p x 2 +py 2 How to extract useful information on energy states from Hamiltonian without solving equation Hψ = Eψ
27 Topological invariant in momentum space H = p2 2m µ c(p x ip y c(p x + ip y p2 + µ 2m g 3 (p g 1 (p +i g 2 (p H = g 1 (p i g 2 (p g 3 (p = τ.g(p p 2 = p x 2 +py 2 N 3 = 1 d 2 p g. ( p x 4π g py g fully gapped 2D state at µ = 0 GV, JETP 67, 1804 (1988 Skyrmion (coreless vortex in momentum space at µ > 0 p y p x unit vector g (p x,p y g^ sweeps unit sphere N 3 (µ > 0 = 1
28 H = quantum phase transition: from topological to non-topologicval insulator/superconductor Topological invariant in momentum space N 3 = p2 2m µ c(p x ip y c(p x + ip y p2 + µ 2m 1 d 2 p g. ( p x 4π g py g g 3 (p g 1 (p +i g 2 (p = g 1 (p i g 2 (p g 3 (p trivial insulator N 3 = 0 N 3 N 3 = 1 topological insulator = τ.g(p µ intermediate state at µ = 0 must be gapless µ = 0 quantum phase transition N 3 = 0 is origin of fermion zero modes at the interface between states with different N 3
29 p-space invariant in terms of Green's function & topological QPT N 3 = 1 24π 2 e µνλ tr d 2 p dω G µ G -1 G ν G -1 G λ G -1 quantum phase transitions in thin 3 He-A film N 3 = 4 N 3 = 6 GV & Yakovenko J. Phys. CM 1, 5263 (1989 N 3 = 2 transition between plateaus must occur via gapless state! N 3 = 0 QPT from trivial to topological state gap gap a 1 a 2 a 3 gap plateau-plateau QPT between topological states a film thickness
30 example: QPT between gapless & gapped matter T (temperature topological semi-metal q c topological quantum phase transitions transitions between ground states (vacua of the same symmetry, but different topology in momentum space no change of symmetry along the path q - parameter of system quantum phase transition at q=q c different asymptotes when T => T n q e /T 0 c T topological insulator other topological QPT: Lifshitz transition, transtion between topological and nontopological superfluids, plateau transitions, confinement-deconfinement transition,... T T QPT interrupted by thermodynamic transitions no symmetry change along the path line of 1-st order transition broken symmetry q 2-nd order transition q q line of 1-st order transition line of 2-nd order transition
31 Zero energy states on surface of topological insulators & superfluids p y Fully gapped 2+1 system p x N 3 = 1 dp x dp y g. ( p x 4π g py g Fully gapped 3+1 system Majorana fermions on the surface and in the vortex cores
32 interface between two 2+1 topological insulators or gapped superfluids y N 3 = N interface N 3 = N + x gapped state gapless interface gapped state * domain wall in 2D chiral superconductors: H = p2 2m c(p x i p y tanh x µ c(p x + i p y tanh x p2 + µ 2m p x - component p x ip y N 3 = 1 0 p x +ip y N 3 = +1 x p y - component
33 Edge states at interface between two 2+1 topological insulators or gapped superfluids y N 3 = N interface N 3 = N + gapped state gapped state empty E(p y 0 left moving edge states occupied p y GV JETP Lett. 55, 368 (1992 Index theorem: number of fermion zero modes at interface: ν = N + N
34 Edge states and currents empty E(p y 2D non-topological insulator or vacuum left moving edge states current y 2D topological insulator N 3 = 0 N 3 = 0 N 3 = 1 current y right moving edge states 2D non-topological insulator or vacuum x E(p y empty 0 p y 0 p y occupied occupied current J y = J left +J right = 0
35 Edge states and Quantum Hall effect 2D non-topological insulator or vacuum 2D topological insulator 2D non-topological insulator or vacuum apply voltage V N 3 = 0 V/2 current E(p y V/2 E(p y +V/2 y N 3 = 1 V/2 current y N 3 = 0 x V/2 0 p y left moving edge states right moving edge states V/2 0 p y current J y = J left +J right = σ xy E y σ xy = e 2 N 3 4π
36 Intrinsic spin-current quantum Hall effect & momentum-space invariant spin current J x z = 1 4π (γn ss dh z /dy + N se E y spin-spin QHE spin-charge QHE 2D singlet superconductor: spin/spin σ xy = N ss 4π s-wave: N ss = 0 p x + ip y : N ss = 2 d xx-yy + id xy : N ss = 4 film of planar phase of superfluid 3 He spin/charge σ xy = N se 4π GV & Yakovenko J. Phys. CM 1, 5263 (1989
37 planar phase film of 3He & 2D topological insulator p2 c(p x + i p y σ z H = 2m µ p2 c(p x i p y σ z + µ 2m N 3 = 1 eµνλ tr [ d 2 p dω G µ G -1 G ν G -1 G λ G -1 ] = 0 24π 2 N se = 1 eµνλ tr [ d 2 p dω σ z G µ G -1 G ν G -1 G λ G -1 ] 24π 2 N 3 = N N = 0 N + 3 = +1 N 3 = 1 + N N se = + 3 = N 3 2 spin quantum Hall effect spin current J x z = 1 Nse E y 4π spin-charge QHE spin/charge σ xy = N se 4π N se = 2 GV & Yakovenko J. Phys. CM 1, 5263 (1989
38 Intrinsic spin-current quantum Hall effect & edge state spin current J x z = 1 (γn 4π ss dh z /dy + N se E y spin-charge QHE y y N se = 0 V/2 spin current N se = 2 spin current V/2 N se = 0 x E(p y V/2 E(p y +V/2 right moving spin up left moving spin up V/2 p y spin/charge σ xy = N se 4π V/2 p y right moving spin down electric current is zero spin current is nonzero left moving spin down
39 3D topological superfluids / insulators / semiconductors / vacua gapless topologically nontrivial vacua fully gapped topologically nontrivial vacua 3He-A, Standard Model above electroweak transition, semimetals, 4D graphene (cryocrystalline vacuum 3He-B, Standard Model below electroweak transition, topological insulators, triplet & singlet chiral superconductor,... Bi 2 Te 3
40 Present vacuum as semiconductor or insulator 3 conduction bands of d-quarks electric charge q=-1/3 E (p 3 conduction bands of u-quarks, q=+2/3 conduction electron band, q=-1 neutrino band, q=0 neutrino band, q=0 p valence electron band, q=-1 3 valence u-quark bands q=+2/3 3 valence d-quark bands q=-1/3 Quantum vacuum: Dirac sea electric charge of quantum vacuum Q= Σ q a = N [ (-1/3 + 3 (+2/3 ] = 0 a dielectric and magnetic properties of vacuum (running coupling constants
41 fully gapped 3+1 topological matter superfluid 3 He-B, topological insulator Bi 2 Te 3, present vacuum of Standard Model * Standard Model vacuum as topological insulator Topological invariant protected by symmetry N Κ = 1 24π 2 e µνλ tr dv Κ G µ G -1 G ν G -1 G λ G -1 over 3D momentum space G is Green's function at ω=0, Κ is symmetry operator GΚ =+/ ΚG Standard Model vacuum: Κ=γ 5 Gγ 5 = γ 5 G N Κ = 8n g 8 massive Dirac particles in one generation
42 topological superfluid 3 He-B ( Η = p2 c B σ.p 2m* µ p2 c B σ.p 2m* + µ ( ( ( p2 2m* µ = τ 3 +c B σ.p τ 1 Hτ 2 = τ 2 H K = τ 2 1/m* non-topological superfluid topological 3 He-B N Κ = 0 N Κ = +2 0 N Κ = 1 N Κ = +1 µ Dirac vacuum 1/m* = 0 Dirac N Κ = 2 topological superfluid N Κ = 0 Dirac non-topological superfluid Η = ( Μ c B σ.p c B σ.p + Μ GV JETP Lett. 90, 587 (2009
43 Boundary of 3D gapped topological superfluid vacuum x,y 3 He-B Η = ( p2 c B σ.p 2m* µ+u(z p2 c B σ.p 2m* + µ U(z ( N Κ = 0 N Κ = +2 Majorana fermions on wall 0 µ U(z N Κ = +2 z Majorana particle = Majorana anti-particle 1/2 of fermion: b = b + spectrum of Majorana zero modes H zm = c ^ B z. σ x p = c B (σ x p y σ y p x N Κ = 0 0 z helical fermions
44 fermion zero modes on Dirac wall Dirac wall Dirac vacuum Dirac vacuum Η = ( Μ(z cσ.p cσ.p + Μ(z ( N Κ = 1 Μ < 0 N Κ = +1 Μ > 0 Volkov-Pankratov, 2D massless fermions in inverted contacts JETP Lett. 42, 178 (1985 chiral fermions N Κ = 1 Μ 0 N Κ = +1 z 0 Dirac point at the wall z Dirac point nodal line in Bi 2 Te 3 Dirac point is below FS: nodal line on surface of topological insulator Bi 2 Te 3
45 Majorana fermions: edge states on the boundary of 3D gapped topological matter * boundary of topological superfluid 3 He-B vacuum N Κ = 0 x,y 3 He-B N Κ = +2 Η = ( Majorana fermions on wall p2 cσ.p 2m* µ+u(z p2 cσ.p 2m* + µ U(z µ U(z N Κ = +2 ( 0 z N Κ = 0 0 spectrum of fermion zero modes * Dirac domain wall H zm = c (σ x p y σ y p x chiral fermion N Κ = 1 Μ 0 N Κ = +1 z Η = ( Μ(z cσ.p helical fermions cσ.p + Μ(z ( Volkov-Pankratov, 2D massless fermions in inverted contacts JETP Lett. 42, 178 (1985
46 Majorana fermions Η = p2 on interface in topological superfluid 3 He-B 2m* µ σ x c x p x +σ y c y p y +σ z c z p z p2 (σ x c x p x +σ y c y p y +σ z c z p z 2m* + µ ( N Κ = 2 c x N Κ = +2 0 c y N Κ = 2 N Κ = +2 N Κ = +2 N Κ = 2 domain wall phase diagram one of 3 "speeds of light" changes sign across wall Majorana fermions c z N Κ = +2 spectrum of fermion zero modes N Κ = 2 0 z H zm = c (σ x p y σ y p x
47 Conclusion Momentum-space topology determines: universality classes of quantum vacua effective field theories in these quantum vacua topological quantum phase transitions (Lifshitz, plateau, etc. quantization of Hall and spin-hall conductivity topological Chern-Simons & Wess-Zumino terms quantum statistics of topological objects spectrum of edge states & fermion zero modes on walls & quantum vortices chiral anomaly & vortex dynamics, etc.
Topological semimetals: from Standard Model to flat band
a^ Topological semimetals: from Standard Model to flat band G. Volovik Aalto University Landau Institute a^ 1. Gapless & gapped topological media 2. Fermi surface as topological object Frascati, 7 Settembre,
More informationWorkshop and Conference on Geometrical Aspects of Quantum States in Condensed Matter. 1-5 July 2013
2469-1 Workshop and Conference on Geometrical Aspects of Quantum States in Condensed Matter 1-5 July 2013 Momentum space topology in Standard Model and in condensed matter Grigory Volovik Aalto University
More informationThe Universe in a helium droplet: from semi-metals & topological insulators to particle physics & cosmology G. Volovik Zelenogorsk, July 12, 2010
The Universe in a helium droplet: from semi-metals & topological insulators to particle physics & cosmology G. Volovik Zelenogorsk, July 12, 2010 1. Introduction: helium liquids & Universe * effective
More informationContents. 1.1 Prerequisites and textbooks Physical phenomena and theoretical tools The path integrals... 9
Preface v Chapter 1 Introduction 1 1.1 Prerequisites and textbooks......................... 1 1.2 Physical phenomena and theoretical tools................. 5 1.3 The path integrals..............................
More informationSpeculations on extensions of symmetry and interctions to GUT energies Lecture 16
Speculations on extensions of symmetry and interctions to GUT energies Lecture 16 1 Introduction The use of symmetry, as has previously shown, provides insight to extensions of present physics into physics
More informationField Theory Description of Topological States of Matter. Andrea Cappelli INFN, Florence (w. E. Randellini, J. Sisti)
Field Theory Description of Topological States of Matter Andrea Cappelli INFN, Florence (w. E. Randellini, J. Sisti) Topological States of Matter System with bulk gap but non-trivial at energies below
More informationEffective Field Theories of Topological Insulators
Effective Field Theories of Topological Insulators Eduardo Fradkin University of Illinois at Urbana-Champaign Workshop on Field Theoretic Computer Simulations for Particle Physics and Condensed Matter
More informationQuantum Field Theory. Kerson Huang. Second, Revised, and Enlarged Edition WILEY- VCH. From Operators to Path Integrals
Kerson Huang Quantum Field Theory From Operators to Path Integrals Second, Revised, and Enlarged Edition WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA I vh Contents Preface XIII 1 Introducing Quantum Fields
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Superfluid Helium-3: From very low Temperatures to the Big Bang Dieter Vollhardt Yukawa Institute, Kyoto; November 27, 2007 Contents: The quantum liquids 3 He and 4 He Superfluid phases of 3 He Broken
More informationParticles and Strings Probing the Structure of Matter and Space-Time
Particles and Strings Probing the Structure of Matter and Space-Time University Hamburg DPG-Jahrestagung, Berlin, March 2005 2 Physics in the 20 th century Quantum Theory (QT) Planck, Bohr, Heisenberg,...
More informationMany-Body Problems and Quantum Field Theory
Philippe A. Martin Francois Rothen Many-Body Problems and Quantum Field Theory An Introduction Translated by Steven Goldfarb, Andrew Jordan and Samuel Leach Second Edition With 102 Figures, 7 Tables and
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Superfluid Helium-3: From very low Temperatures to the Big Bang Universität Frankfurt; May 30, 2007 Dieter Vollhardt Contents: The quantum liquids 3 He and 4 He Superfluid phases of 3 He Broken symmetries
More informationThe Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach)
The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach) IPM school and workshop on recent developments in Particle Physics (IPP11) 2011, Tehran, Iran Sedigheh Deldar, University
More informationTopological Insulators
Topological Insulators Aira Furusai (Condensed Matter Theory Lab.) = topological insulators (3d and 2d) Outline Introduction: band theory Example of topological insulators: integer quantum Hall effect
More informationQuantum Field Theory. and the Standard Model. !H Cambridge UNIVERSITY PRESS MATTHEW D. SCHWARTZ. Harvard University
Quantum Field Theory and the Standard Model MATTHEW D. Harvard University SCHWARTZ!H Cambridge UNIVERSITY PRESS t Contents v Preface page xv Part I Field theory 1 1 Microscopic theory of radiation 3 1.1
More informationPRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in
LONDON BEIJING HONG TSINGHUA Report and Review in Physics Vol2 PRINCIPLES OF PHYSICS From Quantum Field Theory to Classical Mechanics Ni Jun Tsinghua University, China NEW JERSEY \Hp SINGAPORE World Scientific
More informationContents. Preface to the First Edition Preface to the Second Edition
Contents Preface to the First Edition Preface to the Second Edition Notes xiii xv xvii 1 Basic Concepts 1 1.1 History 1 1.1.1 The Origins of Nuclear Physics 1 1.1.2 The Emergence of Particle Physics: the
More informationThe Big Picture. Thomas Schaefer. North Carolina State University
The Big Picture Thomas Schaefer North Carolina State University 1 Big Questions What is QCD? What is a Phase of QCD? What is a Plasma? What is a (perfect) Liquid? What is a wqgp/sqgp? 2 What is QCD (Quantum
More informationTopological Insulators in 3D and Bosonization
Topological Insulators in 3D and Bosonization Andrea Cappelli, INFN Florence (w. E. Randellini, J. Sisti) Outline Topological states of matter: bulk and edge Fermions and bosons on the (1+1)-dimensional
More informationSpontaneous symmetry breaking in particle physics: a case of cross fertilization. Giovanni Jona-Lasinio
Spontaneous symmetry breaking in particle physics: a case of cross fertilization Giovanni Jona-Lasinio QUARK MATTER ITALIA, 22-24 aprile 2009 1 / 38 Spontaneous (dynamical) symmetry breaking Figure: Elastic
More informationThe Superfluid-Insulator transition
The Superfluid-Insulator transition Boson Hubbard model M.P. A. Fisher, P.B. Weichmann, G. Grinstein, and D.S. Fisher, Phys. Rev. B 40, 546 (1989). Superfluid-insulator transition Ultracold 87 Rb atoms
More informationThe cosmological constant puzzle
The cosmological constant puzzle Steven Bass Cosmological constant puzzle: Accelerating Universe: believed to be driven by energy of nothing (vacuum) Vacuum energy density (cosmological constant or dark
More informationBlack-hole & white-hole horizons for capillary-gravity waves in superfluids
Black-hole & white-hole horizons for capillary-gravity waves in superfluids G. Volovik Helsinki University of Technology & Landau Institute Cosmology COSLAB Particle Particle physics Condensed matter Warwick
More informationChern-Simons Theory and Its Applications. The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee
Chern-Simons Theory and Its Applications The 10 th Summer Institute for Theoretical Physics Ki-Myeong Lee Maxwell Theory Maxwell Theory: Gauge Transformation and Invariance Gauss Law Charge Degrees of
More informationCondensed Matter Physics and the Nature of Spacetime
Condensed Matter Physics and the Nature of Spacetime Jonathan Bain Polytechnic University Prospects for modeling spacetime as a phenomenon that emerges in the low-energy limit of a quantum liquid. 1. EFTs
More informationThe Standard Model of Electroweak Physics. Christopher T. Hill Head of Theoretical Physics Fermilab
The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab Lecture I: Incarnations of Symmetry Noether s Theorem is as important to us now as the Pythagorean Theorem
More informationVacuum Energy and the cosmological constant puzzle
Vacuum Energy and the cosmological constant puzzle Cosmological constant puzzle: Steven Bass Accelerating Universe: believed to be driven by energy of nothing (vacuum) Positive vacuum energy = negative
More informationSuperfluidity and Symmetry Breaking. An Unfinished Symphony
Superfluidity and Symmetry Breaking An Unfinished Symphony The Classics The simplest model for superfluidity involves a complex scalar field that supports a phase (U(1)) symmetry in its fundamental equations,
More informationFYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction
FYS 3510 Subatomic physics with applications in astrophysics Nuclear and Particle Physics: An Introduction Nuclear and Particle Physics: An Introduction, 2nd Edition Professor Brian Martin ISBN: 978-0-470-74275-4
More informationWhere are we heading? Nathan Seiberg IAS 2016
Where are we heading? Nathan Seiberg IAS 2016 Two half-talks A brief, broad brush status report of particle physics and what the future could be like The role of symmetries in physics and how it is changing
More informationIntroduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1
Introduction to Particle Physics HST July 2016 Luis Alvarez Gaume 1 Basics Particle Physics describes the basic constituents of matter and their interactions It has a deep interplay with cosmology Modern
More informationThe Phases of QCD. Thomas Schaefer. North Carolina State University
The Phases of QCD Thomas Schaefer North Carolina State University 1 Plan of the lectures 1. QCD and States of Matter 2. The High Temperature Phase: Theory 3. Exploring QCD at High Temperature: Experiment
More informationThe mass of the Higgs boson
The mass of the Higgs boson LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12 a prediction Higgs boson found standard model Higgs boson T.Plehn, M.Rauch Spontaneous symmetry breaking confirmed
More informationSuperinsulator: a new topological state of matter
Superinsulator: a new topological state of matter M. Cristina Diamantini Nips laboratory, INFN and Department of Physics and Geology University of Perugia Coll: Igor Lukyanchuk, University of Picardie
More informationAstronomy 182: Origin and Evolution of the Universe
Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 12 Nov. 18, 2015 Today Big Bang Nucleosynthesis and Neutrinos Particle Physics & the Early Universe Standard Model of Particle
More informationlattice that you cannot do with graphene! or... Antonio H. Castro Neto
Theoretical Aspects What you can do with cold atomsof on agraphene honeycomb lattice that you cannot do with graphene! or... Antonio H. Castro Neto 2 Outline 1. Graphene for beginners 2. Fermion-Fermion
More informationStrongly correlated Cooper pair insulators and superfluids
Strongly correlated Cooper pair insulators and superfluids Predrag Nikolić George Mason University Acknowledgments Collaborators Subir Sachdev Eun-Gook Moon Anton Burkov Arun Paramekanti Affiliations and
More informationEffects of spin-orbit coupling on the BKT transition and the vortexantivortex structure in 2D Fermi Gases
Effects of spin-orbit coupling on the BKT transition and the vortexantivortex structure in D Fermi Gases Carlos A. R. Sa de Melo Georgia Institute of Technology QMath13 Mathematical Results in Quantum
More informationSuperfluid Helium-3: From very low Temperatures to the Big Bang
Center for Electronic Correlations and Magnetism University of Augsburg Superfluid Helium-3: From very low Temperatures to the Big Bang Dieter Vollhardt Dvořák Lecture Institute of Physics, Academy of
More informationThe Scale-Symmetric Theory as the Origin of the Standard Model
Copyright 2017 by Sylwester Kornowski All rights reserved The Scale-Symmetric Theory as the Origin of the Standard Model Sylwester Kornowski Abstract: Here we showed that the Scale-Symmetric Theory (SST)
More informationSupersymmetry and how it helps us understand our world
Supersymmetry and how it helps us understand our world Spitalfields Day Gauge Theory, String Theory and Unification, 8 October 2007 Theoretical Physics Institute, University of Minnesota What is supersymmetry?
More informationUnsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY
Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY 1 I am going to go through some of the major unsolved problems in theoretical physics. I mean the existing theories seem
More informationA Superfluid Universe
A Superfluid Universe Lecture 2 Quantum field theory & superfluidity Kerson Huang MIT & IAS, NTU Lecture 2. Quantum fields The dynamical vacuum Vacuumscalar field Superfluidity Ginsburg Landau theory BEC
More informationClassification of Symmetry Protected Topological Phases in Interacting Systems
Classification of Symmetry Protected Topological Phases in Interacting Systems Zhengcheng Gu (PI) Collaborators: Prof. Xiao-Gang ang Wen (PI/ PI/MIT) Prof. M. Levin (U. of Chicago) Dr. Xie Chen(UC Berkeley)
More informationGauge/Gravity Duality: An introduction. Johanna Erdmenger. Max Planck Institut für Physik, München
.. Gauge/Gravity Duality: An introduction Johanna Erdmenger Max Planck Institut für Physik, München 1 Outline I. Foundations 1. String theory 2. Dualities between quantum field theories and gravity theories
More informationHolography of compressible quantum states
Holography of compressible quantum states New England String Meeting, Brown University, November 18, 2011 sachdev.physics.harvard.edu HARVARD Liza Huijse Max Metlitski Brian Swingle Compressible quantum
More informationKatsushi Arisaka University of California, Los Angeles Department of Physics and Astronomy
11/14/12 Katsushi Arisaka 1 Katsushi Arisaka University of California, Los Angeles Department of Physics and Astronomy arisaka@physics.ucla.edu Seven Phases of Cosmic Evolution 11/14/12 Katsushi Arisaka
More informationLecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM
Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles
More informationPhysics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare
Physics Beyond the Standard Model Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Increasingly General Theories Grand Unified Theories of electroweak and strong interactions Supersymmetry
More informationMay 7, Physics Beyond the Standard Model. Francesco Fucito. Introduction. Standard. Model- Boson Sector. Standard. Model- Fermion Sector
- Boson - May 7, 2017 - Boson - The standard model of particle physics is the state of the art in quantum field theory All the knowledge we have developed so far in this field enters in its definition:
More informationTopological Electromagnetic and Thermal Responses of Time-Reversal Invariant Superconductors and Chiral-Symmetric band insulators
Topological Electromagnetic and Thermal Responses of Time-Reversal Invariant Superconductors and Chiral-Symmetric band insulators Satoshi Fujimoto Dept. Phys., Kyoto University Collaborator: Ken Shiozaki
More informationAharonov-Bohm Effect and Unification of Elementary Particles. Yutaka Hosotani, Osaka University Warsaw, May 2006
Aharonov-Bohm Effect and Unification of Elementary Particles Yutaka Hosotani, Osaka University Warsaw, May 26 - Part 1 - Aharonov-Bohm effect Aharonov-Bohm Effect! B)! Fµν = (E, vs empty or vacuum!= Fµν
More informationQUANTUM FIELD THEORY. A Modern Introduction MICHIO KAKU. Department of Physics City College of the City University of New York
QUANTUM FIELD THEORY A Modern Introduction MICHIO KAKU Department of Physics City College of the City University of New York New York Oxford OXFORD UNIVERSITY PRESS 1993 Contents Quantum Fields and Renormalization
More informationTime Reversal Invariant Ζ 2 Topological Insulator
Time Reversal Invariant Ζ Topological Insulator D Bloch Hamiltonians subject to the T constraint 1 ( ) ΘH Θ = H( ) with Θ = 1 are classified by a Ζ topological invariant (ν =,1) Understand via Bul-Boundary
More informationHIGH DENSITY NUCLEAR CONDENSATES. Paulo Bedaque, U. of Maryland (Aleksey Cherman & Michael Buchoff, Evan Berkowitz & Srimoyee Sen)
HIGH DENSITY NUCLEAR CONDENSATES Paulo Bedaque, U. of Maryland (Aleksey Cherman & Michael Buchoff, Evan Berkowitz & Srimoyee Sen) What am I talking about? (Gabadadze 10, Ashcroft 89) deuterium/helium at
More informationThe Phases of QCD. Thomas Schaefer. North Carolina State University
The Phases of QCD Thomas Schaefer North Carolina State University 1 Motivation Different phases of QCD occur in the universe Neutron Stars, Big Bang Exploring the phase diagram is important to understanding
More informationPart III The Standard Model
Part III The Standard Model Theorems Based on lectures by C. E. Thomas Notes taken by Dexter Chua Lent 2017 These notes are not endorsed by the lecturers, and I have modified them (often significantly)
More informationStephen Blaha, Ph.D. M PubHsMtw
Quantum Big Bang Cosmology: Complex Space-time General Relativity, Quantum Coordinates,"Dodecahedral Universe, Inflation, and New Spin 0, 1 / 2,1 & 2 Tachyons & Imagyons Stephen Blaha, Ph.D. M PubHsMtw
More informationAnomaly. Kenichi KONISHI University of Pisa. College de France, 14 February 2006
Anomaly Kenichi KONISHI University of Pisa College de France, 14 February 2006 Abstract Symmetry and quantization U A (1) anomaly and π 0 decay Origin of anomalies Chiral and nonabelian anomaly Anomally
More informationDuality and Holography
Duality and Holography? Joseph Polchinski UC Davis, 5/16/11 Which of these interactions doesn t belong? a) Electromagnetism b) Weak nuclear c) Strong nuclear d) a) Electromagnetism b) Weak nuclear c) Strong
More informationSome open questions in physics
K.A. Meissner, Unsolved problems p. 1/25 Some open questions in physics Krzysztof A. Meissner Instytut Fizyki Teoretycznej UW Instytut Problemów Ja drowych Kraków, 23.10.2009 K.A. Meissner, Unsolved problems
More informationA Review of Solitons in Gauge Theories. David Tong
A Review of Solitons in Gauge Theories David Tong Introduction to Solitons Solitons are particle-like excitations in field theories Their existence often follows from general considerations of topology
More informationA first trip to the world of particle physics
A first trip to the world of particle physics Itinerary Massimo Passera Padova - 13/03/2013 1 Massimo Passera Padova - 13/03/2013 2 The 4 fundamental interactions! Electromagnetic! Weak! Strong! Gravitational
More informationFundamental Particles
Fundamental Particles Standard Model of Particle Physics There are three different kinds of particles. Leptons - there are charged leptons (e -, μ -, τ - ) and uncharged leptons (νe, νμ, ντ) and their
More informationTopological Defects inside a Topological Band Insulator
Topological Defects inside a Topological Band Insulator Ashvin Vishwanath UC Berkeley Refs: Ran, Zhang A.V., Nature Physics 5, 289 (2009). Hosur, Ryu, AV arxiv: 0908.2691 Part 1: Outline A toy model of
More informationSymmetries Then and Now
Symmetries Then and Now Nathan Seiberg, IAS 40 th Anniversary conference Laboratoire de Physique Théorique Global symmetries are useful If unbroken Multiplets Selection rules If broken Goldstone bosons
More informationNovember 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model
Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one
More informationField Theory Description of Topological States of Matter
Field Theory Description of Topological States of Matter Andrea Cappelli, INFN Florence (w. E. Randellini, J. Sisti) Outline Topological states of matter Quantum Hall effect: bulk and edge Effective field
More informationWhat ideas/theories are physicists exploring today?
Where are we Headed? What questions are driving developments in fundamental physics? What ideas/theories are physicists exploring today? Quantum Gravity, Stephen Hawking & Black Hole Thermodynamics A Few
More informationVacuum Energy and. Cosmological constant puzzle:
Vacuum Energy and the cosmological constant puzzle Steven Bass Cosmological constant puzzle: (arxiv:1503.05483 [hep-ph], MPLA in press) Accelerating Universe: believed to be driven by energy of nothing
More informationThe God particle at last? Astronomy Ireland, Oct 8 th, 2012
The God particle at last? Astronomy Ireland, Oct 8 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV I The Higgs boson
More informationCritical lines and points. in the. QCD phase diagram
Critical lines and points in the QCD phase diagram Understanding the phase diagram Phase diagram for m s > m u,d quark-gluon plasma deconfinement quark matter : superfluid B spontaneously broken nuclear
More informationThe God particle at last? Science Week, Nov 15 th, 2012
The God particle at last? Science Week, Nov 15 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV Why is the Higgs particle
More informationPhysics 4213/5213 Lecture 1
August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible
More informationBeyond Standard Models Higgsless Models. Zahra Sheikhbahaee
Beyond Standard Models Higgsless Models Zahra Sheikhbahaee Standard Model There are three basic forces in the Universe: 1. Electroweak force, including electromagnetic force, 2. Strong nuclear force, 3.
More information2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC)
2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC) hep-th/0606045 Success of 2T-physics for particles on worldlines. Field theory version of 2T-physics. Standard Model in 4+2 dimensions.
More informationPOST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY
POST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY LOUIS YANG ( 楊智軒 ) UNIVERSITY OF CALIFORNIA, LOS ANGELES (UCLA) DEC 27, 2016 NATIONAL TSING HUA UNIVERSITY OUTLINE Big
More informationQGP, Hydrodynamics and the AdS/CFT correspondence
QGP, Hydrodynamics and the AdS/CFT correspondence Adrián Soto Stony Brook University October 25th 2010 Adrián Soto (Stony Brook University) QGP, Hydrodynamics and AdS/CFT October 25th 2010 1 / 18 Outline
More informationPhysics (PHYS) Courses. Physics (PHYS) 1
Physics (PHYS) 1 Physics (PHYS) Courses PHYS 5001. Introduction to Quantum Computing. 3 Credit Hours. This course will give an elementary introduction to some basics of quantum information and quantum
More informationOrigin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?
Origin of the Universe - 2 ASTR 2120 Sarazin What does it all mean? Fundamental Questions in Cosmology 1. Why did the Big Bang occur? 2. Why is the Universe old? 3. Why is the Universe made of matter?
More informationIs the composite fermion a Dirac particle?
Is the composite fermion a Dirac particle? Dam T. Son GGI conference Gauge/gravity duality 2015 Ref.: 1502.03446 Plan Plan Fractional quantum Hall effect Plan Fractional quantum Hall effect Composite fermion
More informationIntroduction to Elementary Particles
David Criffiths Introduction to Elementary Particles Second, Revised Edition WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA Preface to the First Edition IX Preface to the Second Edition XI Formulas and Constants
More informationEvaluating the Phase Diagram at finite Isospin and Baryon Chemical Potentials in NJL model
Evaluating the Phase Diagram at finite Isospin and Baryon Chemical Potentials in NJL model Chengfu Mu, Peking University Collaborated with Lianyi He, J.W.Goethe University Prof. Yu-xin Liu, Peking University
More informationStrings, gauge theory and gravity. Storrs, Feb. 07
Strings, gauge theory and gravity Storrs, Feb. 07 Outline Motivation - why study quantum gravity? Intro to strings Gravity / gauge theory duality Gravity => gauge: Wilson lines, confinement Gauge => gravity:
More informationThe Superfluid Phase s of Helium 3
The Superfluid Phase s of Helium 3 DIETER VOLLHARD T Rheinisch-Westfälische Technische Hochschule Aachen, Federal Republic of German y PETER WÖLFL E Universität Karlsruhe Federal Republic of Germany PREFACE
More informationNearly Perfect Fluidity: From Cold Atoms to Hot Quarks. Thomas Schaefer, North Carolina State University
Nearly Perfect Fluidity: From Cold Atoms to Hot Quarks Thomas Schaefer, North Carolina State University RHIC serves the perfect fluid Experiments at RHIC are consistent with the idea that a thermalized
More informationOn the Higgs mechanism in the theory of
On the Higgs mechanism in the theory of superconductivity* ty Dietrich Einzel Walther-Meißner-Institut für Tieftemperaturforschung Bayerische Akademie der Wissenschaften D-85748 Garching Outline Phenomenological
More informationIntroduction to Cosmology
Introduction to Cosmology Subir Sarkar CERN Summer training Programme, 22-28 July 2008 Seeing the edge of the Universe: From speculation to science Constructing the Universe: The history of the Universe:
More information3 Dimensional String Theory
3 Dimensional String Theory New ideas for interactions and particles Abstract...1 Asymmetry in the interference occurrences of oscillators...1 Spontaneously broken symmetry in the Planck distribution law...3
More informationAn Introduction to the Standard Model of Particle Physics
An Introduction to the Standard Model of Particle Physics W. N. COTTINGHAM and D. A. GREENWOOD Ж CAMBRIDGE UNIVERSITY PRESS Contents Preface. page xiii Notation xv 1 The particle physicist's view of Nature
More informationGauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger. Julius-Maximilians-Universität Würzburg
Gauge/Gravity Duality: Applications to Condensed Matter Physics. Johanna Erdmenger Julius-Maximilians-Universität Würzburg 1 New Gauge/Gravity Duality group at Würzburg University Permanent members 2 Gauge/Gravity
More informationContents. Appendix A Strong limit and weak limit 35. Appendix B Glauber coherent states 37. Appendix C Generalized coherent states 41
Contents Preface 1. The structure of the space of the physical states 1 1.1 Introduction......................... 1 1.2 The space of the states of physical particles........ 2 1.3 The Weyl Heisenberg algebra
More informationarxiv: v3 [hep-th] 7 Feb 2018
Symmetry and Emergence arxiv:1710.01791v3 [hep-th] 7 Feb 2018 Edward Witten School of Natural Sciences, Institute for Advanced Study Einstein Drive, Princeton, NJ 08540 USA Abstract I discuss gauge and
More informationBeyond the Standard Model
Beyond the Standard Model The Standard Model Problems with the Standard Model New Physics Supersymmetry Extended Electroweak Symmetry Grand Unification References: 2008 TASI lectures: arxiv:0901.0241 [hep-ph]
More informationOverview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.
Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider
More informationTopological Properties of Quantum States of Condensed Matter: some recent surprises.
Topological Properties of Quantum States of Condensed Matter: some recent surprises. F. D. M. Haldane Princeton University and Instituut Lorentz 1. Berry phases, zero-field Hall effect, and one-way light
More informationPart 1. March 5, 2014 Quantum Hadron Physics Laboratory, RIKEN, Wako, Japan 2
MAR 5, 2014 Part 1 March 5, 2014 Quantum Hadron Physics Laboratory, RIKEN, Wako, Japan 2 ! Examples of relativistic matter Electrons, protons, quarks inside compact stars (white dwarfs, neutron, hybrid
More informationQuark matter and the high-density frontier. Mark Alford Washington University in St. Louis
Quark matter and the high-density frontier Mark Alford Washington University in St. Louis Outline I Quarks at high density Confined, quark-gluon plasma, color superconducting II Color superconducting phases
More informationg abφ b = g ab However, this is not true for a local, or space-time dependant, transformations + g ab
Yang-Mills theory Modern particle theories, such as the Standard model, are quantum Yang- Mills theories. In a quantum field theory, space-time fields with relativistic field equations are quantized and,
More informationThe Gauge/Gravity correspondence: linking General Relativity and Quantum Field theory
The Gauge/Gravity correspondence: linking General Relativity and Quantum Field theory Alfonso V. Ramallo Univ. Santiago IFIC, Valencia, April 11, 2014 Main result: a duality relating QFT and gravity Quantum
More information