Quantum mechanics without particles
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1 Quantum mechanics without particles Institute Lecture, Indian Institute of Technology, Kanpur January 21, 2014 sachdev.physics.harvard.edu HARVARD
2 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
3 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
4 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Interference of water waves
5 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Send electrons through the slits
6 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Send electrons through the slits
7 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Interference of electrons
8 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Which slit does an electron pass through? Interference of electrons
9 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Which slit does an electron pass through? No interference when you watch the electrons Interference of electrons
10 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Which slit does an electron pass through? Each electron passes through both slits! Interference of electrons
11 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment L Let L represent the state with the electron in the left slit
12 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Let L represent the state with the electron in the left slit L R And R represents the state with the electron in the right slit
13 Principles of Quantum Mechanics: 1. Quantum Superposition The double slit experiment Let L represent the state with the electron in the left slit L R And R represents the state with the electron in the right slit Actual state of the electron is L + R
14 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle
15 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle Hydrogen atom:
16 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle Hydrogen atom: Hydrogen molecule: = _ = 1 2 ( )
17 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle _
18 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle _
19 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle _
20 Principles of Quantum Mechanics: 1I. Quantum Entanglement Quantum Entanglement: quantum superposition with more than one particle _ Einstein-Podolsky-Rosen paradox : Non-local correlations between observations arbitrarily far apart
21 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
22 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
23 Sommerfeld-Bloch theory of metals, insulators, and superconductors: many-electron quantum states are adiabatically connected to independent electron states Metals E In Metal k
24 Boltzmann-Landau theory of dynamics of metals: Long-lived quasiparticles (and quasiholes) have weak interactions which can be described by a Boltzmann equation Metals E In Metal k
25 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
26 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
27 Spinning electrons localized on a square lattice H = ij J ij Si S j S=1/2 spins J J/ Examine ground state as a function of
28 Spinning electrons localized on a square lattice H = J ij Si S j ij J J/ = 1 2 At large ground state is a quantum paramagnet with spins locked in valence bond singlets
29 Spinning electrons localized on a square lattice H = J ij Si S j ij J J/ = 1 2 Nearest-neighor spins are entangled with each other. Can be separated into an Einstein-Podolsky-Rosen (EPR) pair.
30 Spinning electrons localized on a square lattice H = ij J ij Si S j J J/ For 1, the ground state has antiferromagnetic ( Néel ) order, and the spins align in a checkerboard pattern
31 = 1 2 c
32 = 1 2 c Pressure in TlCuCl3 A. Oosawa, K. Kakurai, T. Osakabe, M. Nakamura, M. Takeda, and H. Tanaka, Journal of the Physical Society of Japan, 73, 1446 (2004).
33 TlCuCl 3 An insulator whose spin susceptibility vanishes exponentially as the temperature T tends to zero.
34 TlCuCl 3 Quantum paramagnet at ambient pressure
35 TlCuCl 3 Neel order under pressure A. Oosawa, K. Kakurai, T. Osakabe, M. Nakamura, M. Takeda, and H. Tanaka, Journal of the Physical Society of Japan, 73, 1446 (2004).
36 = 1 2 c
37 Quasiparticles in the paramagnetic phase c Spin S =1 triplon
38 Quasiparticles in the paramagnetic phase c Spin S =1 triplon
39 Quasiparticles in the paramagnetic phase c Spin S =1 triplon
40 Quasiparticles in the Néel phase Spin waves c
41 Quasiparticles in the Néel phase Spin waves c
42 Quasiparticles in the Néel phase Spin waves c
43 Excitations of TlCuCl 3 with varying pressure Energy [mev] Pressure [kbar] Christian Ruegg, Bruce Normand, Masashige Matsumoto, Albert Furrer, Desmond McMorrow, Karl Kramer, Hans Ulrich Gudel, Severian Gvasaliya, Hannu Mutka, and Martin Boehm, Phys. Rev. Lett. 100, (2008)
44 Excitations of TlCuCl 3 with varying pressure Energy [mev] Triplon quasiparticles of the quantum paramagnet Pressure [kbar] Christian Ruegg, Bruce Normand, Masashige Matsumoto, Albert Furrer, Desmond McMorrow, Karl Kramer, Hans Ulrich Gudel, Severian Gvasaliya, Hannu Mutka, and Martin Boehm, Phys. Rev. Lett. 100, (2008)
45 Excitations of TlCuCl 3 with varying pressure Energy [mev] Spin waves above the Néel state Pressure [kbar] Christian Ruegg, Bruce Normand, Masashige Matsumoto, Albert Furrer, Desmond McMorrow, Karl Kramer, Hans Ulrich Gudel, Severian Gvasaliya, Hannu Mutka, and Martin Boehm, Phys. Rev. Lett. 100, (2008)
46 Excitations of TlCuCl 3 with varying pressure Energy [mev] Quasiparticle analog of the Higgs boson at the theoretically predicted energy! Pressure [kbar] S. Sachdev, arxiv: Christian Ruegg, Bruce Normand, Masashige Matsumoto, Albert Furrer, Desmond McMorrow, Karl Kramer, Hans Ulrich Gudel, Severian Gvasaliya, Hannu Mutka, and Martin Boehm, Phys. Rev. Lett. 100, (2008)
47 = 1 2 c
48 = 1 2 c Quantum critical point with non-local entanglement in spin wavefunction A. W. Sandvik and D. J. Scalapino, Phys. Rev. Lett. 72, 2777 (1994).
49 Long-range entanglement No quasiparticles - no simple description of excitations. The low energy excitations are described by a theory which has the same structure as Einstein s theory of special relativity, but with the spin-wave velocity playing the role of the velocity of light. The theory of the critical point has an even larger symmetry corresponding to conformal transformations of spacetime: we refer to such a theory as a CFT3 Characteristics of quantum critical point
50 Long-range entanglement No quasiparticles - no simple description of excitations. The low energy excitations are described by a theory which has the same structure as Einstein s theory of special relativity, but with the spin-wave velocity playing the role of the velocity of light. The theory of the critical point has an even larger symmetry corresponding to conformal transformations of spacetime: we refer to such a theory as a CFT3 Characteristics of quantum critical point
51 Long-range entanglement No quasiparticles - no simple description of excitations. The low energy excitations are described by a theory which has the same structure as Einstein s theory of special relativity, but with the spin-wave velocity playing the role of the velocity of light. The theory of the critical point has an even larger symmetry corresponding to conformal transformations of spacetime: we refer to such a theory as a CFT3 Characteristics of quantum critical point
52 Long-range entanglement No quasiparticles - no simple description of excitations. The low energy excitations are described by a theory which has the same structure as Einstein s theory of special relativity, but with the spin-wave velocity playing the role of the velocity of light. The theory of the critical point has an even larger symmetry corresponding to conformal transformations of spacetime: we refer to such a theory as a CFT3 Characteristics of quantum critical point
53 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
54 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
55 String theory Allows unification of the standard model of particle physics with gravity. Low-lying string modes correspond to gauge fields, gravitons, quarks...
56 A D-brane is a d-dimensional surface on which strings can end. The low-energy theory on a D-brane has no gravity, similar to theories of entangled electrons of interest to us. In d = 2, we obtain strongly-interacting CFT3s. These are dual to string theory on anti-de Sitter space: AdS4.
57 A D-brane is a d-dimensional surface on which strings can end. The low-energy theory on a D-brane has no gravity, similar to theories of entangled electrons of interest to us. In d = 2, we obtain strongly-interacting CFT3s. These are dual to string theory on anti-de Sitter space: AdS4.
58 A D-brane is a d-dimensional surface on which strings can end. The low-energy theory on a D-brane has no gravity, similar to theories of entangled electrons of interest to us. In d = 2, we obtain strongly-interacting CFT3s. These are dual to string theory on anti-de Sitter space: AdS4.
59 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
60 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
61 = 1 2 c Quantum critical point with non-local entanglement in spin wavefunction
62 Quantum critical Classical spin waves Dilute triplon gas Neel order
63 S. Sachdev and J. Ye, Phys. Rev. Lett. 69, 2411 (1992). A. V. Chubukov, S. Sachdev, and J. Ye, Phys. Rev. B 49, (1994). Quantum critical Classical spin waves Thermally excited spin waves Dilute triplon gas Thermally excited triplon particles Neel order
64 S. Sachdev and J. Ye, Phys. Rev. Lett. 69, 2411 (1992). A. V. Chubukov, S. Sachdev, and J. Ye, Phys. Rev. B 49, (1994). Classical spin waves Thermally excited spin waves Quantum critical Needed: Accurate theory of quantum critical dynamics without quasiparticles Dilute triplon gas Thermally excited triplon particles Neel order
65 String theory at non-zero temperatures A 2+1 dimensional system at its quantum critical point
66 String theory at non-zero temperatures A 2+1 dimensional system at its quantum critical point A horizon, similar to the surface of a black hole!
67 Black Holes Objects so massive that light is gravitationally bound to them.
68 Black Holes Objects so massive that light is gravitationally bound to them. In Einstein s theory, the region inside the black hole horizon is disconnected from the rest of the universe. Horizon radius R = 2GM c 2
69 Black Holes + Quantum theory Around 1974, Bekenstein and Hawking showed that the application of the quantum theory across a black hole horizon led to many astonishing conclusions
70 Quantum Entanglement across a black hole horizon _
71 Quantum Entanglement across a black hole horizon _
72 Quantum Entanglement across a black hole horizon _ Black hole horizon
73 Quantum Entanglement across a black hole horizon _ Black hole horizon
74 Quantum Entanglement across a black hole horizon There is a non-local quantum entanglement between the inside and outside of a black hole Black hole horizon
75 Quantum Entanglement across a black hole horizon There is a non-local quantum entanglement between the inside and outside of a black hole Black hole horizon
76 Quantum Entanglement across a black hole horizon There is a non-local quantum entanglement between the inside and outside of a black hole This entanglement leads to a black hole temperature (the Hawking temperature) and a black hole entropy (the Bekenstein entropy)
77 String theory at non-zero temperatures A 2+1 dimensional system at its quantum critical point A horizon, whose temperature and entropy equal those of the quantum critical point
78 String theory at non-zero temperatures A 2+1 dimensional system at its quantum critical point A horizon, whose temperature and entropy equal those of the quantum critical point Friction of quantum criticality = waves falling into black brane
79 String theory at non-zero temperatures A 2+1 dimensional system at its quantum critical point A horizon, whose temperature and entropy equal those of the quantum critical point An (extended) Einstein-Maxwell provides successful description of dynamics of quantum critical points at non-zero temperatures (where no other methods apply)
80 Black hole predictions for quantum critical dynamics 0.50 (!)/(e 2 /h) shwlêsq wê2pt Predictions of holographic theory, after analytic continuation to real frequencies W. Witczak-Krempa, E. Sorensen, and S. Sachdev, arxiv: See also K. Chen, L. Liu, Y. Deng, L. Pollet, and N. Prokof ev, arxiv:
81 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
82 Outline 1. Key ideas from quantum mechanics 2. Many-particle systems: the concept of a quasiparticle 3. Quantum phases of a magnetic insulator Quantum critical point without quasiparticles 4. Connections to string theory 5. Non-zero temperatures and black holes 6. The high temperature superconductors
83 YBa 2 Cu 3 O 6+x
84 Nd-Fe-B magnets, YBaCuO superconductor Julian Hetel and Nandini Trivedi, Ohio State University
85 Nd-Fe-B magnets, YBaCuO superconductor Julian Hetel and Nandini Trivedi, Ohio State University
86 Nd-Fe-B magnets, YBaCuO superconductor Julian Hetel and Nandini Trivedi, Ohio State University
87 Nd-Fe-B magnets, YBaCuO superconductor Julian Hetel and Nandini Trivedi, Ohio State University
88 Iron pnictides: a new class of high temperature superconductors Ishida, Nakai, and Hosono arxiv: v1
89 Resistivity 0 + AT BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " 2.0 AF SDW 1.0 Superconductivity 0 S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010)
90 Resistivity 0 + AT BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " Neel (AF) and nematic order 2.0 AF SDW 1.0 Superconductivity 0 S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010)
91 Resistivity 0 + AT BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " Neel (AF) and nematic order 2.0 AF SDW 1.0 Superconductivity 0 S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010)
92 Resistivity 0 + AT BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " 2.0 AF SDW 1.0 Superconductivity 0 Superconductor Bose condensate of pairs of electrons S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010)
93 Resistivity 0 + AT BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " 2.0 AF SDW 1.0 Superconductivity 0 Ordinary metal S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010) (Fermi liquid)
94 Resistivity 0 + AT Strange Metal no quasiparticles, Landau-Boltzmann theory does not apply BaFe 2 (As 1-x P x ) 2 T 0 T SD T c α " 2.0 AF SDW 1.0 Superconductivity 0 S. Kasahara, T. Shibauchi, K. Hashimoto, K. Ikada, S. Tonegawa, R. Okazaki, H. Shishido, H. Ikeda, H. Takeya, K. Hirata, T. Terashima, and Y. Matsuda, Physical Review B 81, (2010)
95 Quantum criticality of Ising-nematic ordering in a metal y Occupied states x Empty states A metal with a Fermi surface with full square lattice symmetry
96 Quantum criticality of Ising-nematic ordering in a metal y x Neel (AF) and nematic order Spontaneous elongation along x direction
97 Quantum criticality of Ising-nematic ordering in a metal y x Neel (AF) and nematic order Spontaneous elongation along y direction
98 Quantum criticality of Ising-nematic ordering in a metal or =0 =0 r r c Zero temperature phase diagram as a function of some parameter r
99 Quantum criticality of Ising-nematic ordering in a metal T Strange TI-n Metal or Fermi liquid r c Fermi liquid r Phase diagram as a function of T and r
100 Quantum criticality of Ising-nematic ordering in a metal T Strange TI-n Metal or Strongly-coupled non-fermi liquid metal with no quasiparticles Fermi liquid r c Fermi liquid r Phase diagram as a function of T and r
101 Strongly-coupled quantum critical points lead to a novel regime of quantum dynamics without quasiparticles. The simplest examples are CFT3s realized in experiments on ultracold bosons and in model antiferromagnets. Methods of string theory, and black hole dynamics, provide a quantitative understanding of quantum Monte studies of quantum critical points in condensed matter. Exciting recent progress on the description of metallic states without quasiparticles, via quantum field theory and holography
102 Strongly-coupled quantum critical points lead to a novel regime of quantum dynamics without quasiparticles. The simplest examples are CFT3s realized in experiments on ultracold bosons and in model antiferromagnets. Methods of string theory, and black hole dynamics, provide a quantitative understanding of quantum Monte studies of quantum critical points in condensed matter. Exciting recent progress on the description of metallic states without quasiparticles, via quantum field theory and holography
103 Strongly-coupled quantum critical points lead to a novel regime of quantum dynamics without quasiparticles. The simplest examples are CFT3s realized in experiments on ultracold bosons and in model antiferromagnets. Methods of string theory, and black hole dynamics, provide a quantitative understanding of quantum Monte studies of quantum critical points in condensed matter. Exciting recent progress on the description of metallic states without quasiparticles, via quantum field theory and holography
104 Strongly-coupled quantum critical points lead to a novel regime of quantum dynamics without quasiparticles. The simplest examples are CFT3s realized in experiments on ultracold bosons and in model antiferromagnets. Methods of string theory, and black hole dynamics, provide a quantitative understanding of quantum Monte studies of quantum critical points in condensed matter. Exciting recent progress on the description of metallic states without quasiparticles, via quantum field theory and holography
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