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Outline Intro EFT Dilute Summary Refs Fermion Many-Body Systems I Dick Furnstahl Department of Physics Ohio State University June, 2004 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Outline Overview of Fermion Many-Body Systems Effective Low-Energy Theories EFT for Dilute Fermi Systems Summary I: Fermion Many-body Systems References and Resources Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional Examples of Fermion Many-Body Systems Collections of “fundamental” fermions (electrons, quarks, . . . ) or composites of odd number of fermions (e.g., proton) Isolated atoms or molecules electrons interacting via long-range (screened) Coulomb find charge distribution, binding energy, bond lengths, . . . Bulk solid-state materials metals, insulators, semiconductors, superconductors, . . . Liquid 3 He (superfluid!) Cold fermionic atoms in (optical) traps Atomic nuclei Neutron stars color superconducting quark matter neutron matter Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional Examples of Fermion Many-Body Systems Collections of “fundamental” fermions (electrons, quarks, . . . ) or composites of odd number of fermions (e.g., proton) Isolated atoms or molecules electrons interacting via long-range (screened) Coulomb find charge distribution, binding energy, bond lengths, . . . Bulk solid-state materials metals, insulators, semiconductors, superconductors, . . . Liquid 3 He (superfluid!) Cold fermionic atoms in (optical) traps Atomic nuclei Neutron stars color superconducting quark matter neutron matter Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional 126 Limits of nuclear existence 82 protons roc r-p rp 28 20 50 ss ce ro -p 82 50 8 28 2 20 2 8 =10 A Ab initio few-body calculations 12 A= neutrons A~ s es ory he l T Field a n tio ean nc Fu ent M y t t nsi sis De lfcon Se 60 0Ñω Shell Model Many-body approaches for ordinary nuclei No-Core Shell Model G-matrix Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional How Are Cold Atoms Like Neutron Stars? Regal et al., ultracold fermions Dick Furnstahl Chandra X-Ray Observatory image of pulsar in 3C58 Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional Nuclear and Cold Atom Many-Body Problems 50 40 30 20 10 0 -10 n-n potential (MeV) O2-O2 potential (meV) Lennard-Jones and nucleon-nucleon potentials 500 n-n system 400 O -O system 2 300 2 200 100 0 -100 0 0 1 2 3 n-n distance (fm) 0.4 0.8 O2-O2 distance (nm) 1.2 [figure borrowed from J. Dobaczewski] Are there universal features of such many-body systems? How can we deal with “hard cores” in many-body systems? Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach One Hamiltonian for all problems and energy/length scales Dick Furnstahl For nuclear structure, protons and neutrons with a local potential fit to NN data Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach One Hamiltonian for all problems and energy/length scales Find the “best” potential Dick Furnstahl For nuclear structure, protons and neutrons with a local potential fit to NN data NN potential with χ2 /dof ≈ 1 up to ∼ 300 MeV energy Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Dick Furnstahl For nuclear structure, protons and neutrons with a local potential fit to NN data NN potential with χ2 /dof ≈ 1 up to ∼ 300 MeV energy Let phenomenology dictate whether three-body forces are needed (answer: yes!) Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Avoid divergences Dick Furnstahl For nuclear structure, protons and neutrons with a local potential fit to NN data NN potential with χ2 /dof ≈ 1 up to ∼ 300 MeV energy Let phenomenology dictate whether three-body forces are needed (answer: yes!) Add “form factor” to suppress high-energy intermediate states; don’t consider cutoff dependence Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Systems Traditional (Nuclear) Many-Body Physics: “Old” Approach One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Avoid divergences Choose diagrams by “art” Dick Furnstahl For nuclear structure, protons and neutrons with a local potential fit to NN data NN potential with χ2 /dof ≈ 1 up to ∼ 300 MeV energy Let phenomenology dictate whether three-body forces are needed (answer: yes!) Add “form factor” to suppress high-energy intermediate states; don’t consider cutoff dependence Use physical arguments (often handwaving) to justify the subset of diagrams used Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Resolution and the Pointillists Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Resolution and the Pointillists George Seurat painted using closely spaced small dots (≈ 0.4 mm wide) of pure pigment Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Resolution and the Pointillists George Seurat painted using closely spaced small dots (≈ 0.4 mm wide) of pure pigment Why do the dots blend together? Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Diffraction and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Wavelength and Resolution Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Principles of Effective Low-Energy Theories Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Principles of Effective Low-Energy Theories If system is probed at low energies, fine details not resolved Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Principles of Effective Low-Energy Theories If system is probed at low energies, fine details not resolved use low-energy variables for low-energy processes short-distance structure can be replaced by something simpler without distorting low-energy observables Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering “Simple” Many-Body Problem: Hard Spheres Infinite potential at radius R R Scattering solutions are simple: u0(r) = sin[k(r-R)] 2 Ek = k /M 0 R r >>R What is the energy / particle of the many-body system at a given density? Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Quick Review of Scattering P/2 + k P/2 + k0 P/2 − k 0 sin(kr+δ) 0 P/2 − k r R r →∞ ikr Relative motion in frame with P = 0: ψ(r ) −→ eik·r + f (k, θ) er where k 2 = k 0 2 = MEk and cos θ = k̂ · k̂ 0 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Quick Review of Scattering P/2 + k P/2 + k0 P/2 − k 0 sin(kr+δ) 0 P/2 − k r R r →∞ ikr Relative motion in frame with P = 0: ψ(r ) −→ eik·r + f (k, θ) er where k 2 = k 0 2 = MEk and cos θ = k̂ · k̂ 0 Differential cross section is dσ/dΩ = |f (k, θ)|2 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Quick Review of Scattering P/2 + k P/2 + k0 P/2 − k 0 sin(kr+δ) 0 P/2 − k r R r →∞ ikr Relative motion in frame with P = 0: ψ(r ) −→ eik·r + f (k, θ) er where k 2 = k 0 2 = MEk and cos θ = k̂ · k̂ 0 Differential cross section is dσ/dΩ = |f (k, θ)|2 P Central V =⇒ partial waves: f (k, θ) = l (2l + 1)fl (k)Pl (cos θ) where fl (k ) = eiδl (k) sin δl (k) 1 = k k cot δl (k) − ik and the S-wave phase shift is defined by r →∞ u0 (r ) −→ sin[kr + δ0 (k)] Dick Furnstahl =⇒ δ0 (k ) = −kR for hard sphere Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering At Low Energies: Effective Range Expansion As first shown by Schwinger, k l+1 cot δl (k) has a power series expansion. For l = 0: k cot δ0 = − 1 1 + r0 k 2 − Pr03 k 4 + · · · a0 2 which defines the scattering length a0 and the effective range r0 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering At Low Energies: Effective Range Expansion As first shown by Schwinger, k l+1 cot δl (k) has a power series expansion. For l = 0: k cot δ0 = − 1 1 + r0 k 2 − Pr03 k 4 + · · · a0 2 which defines the scattering length a0 and the effective range r0 While r0 ∼ R, the range of the potential, a0 can be anything if a0 ∼ R, it is called “natural” |a0 | R (unnatural) is particularly interesting =⇒ tomorrow! Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering At Low Energies: Effective Range Expansion As first shown by Schwinger, k l+1 cot δl (k) has a power series expansion. For l = 0: k cot δ0 = − 1 1 + r0 k 2 − Pr03 k 4 + · · · a0 2 which defines the scattering length a0 and the effective range r0 While r0 ∼ R, the range of the potential, a0 can be anything if a0 ∼ R, it is called “natural” |a0 | R (unnatural) is particularly interesting =⇒ tomorrow! The effective range expansion for hard sphere scattering is: k cot(−kR) = − 1 1 + Rk 2 + · · · R 3 =⇒ a0 = R so the low-energy effective theory is natural Dick Furnstahl Fermion Many-Body Systems I r0 = 2R/3 Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion If a0 is natural, then low-energy scattering simplifies further For scattering at momentum k 1/R, we should recover a perturbative expansion in kR for scattering amplitude: f0 (k ) ∝ 1 −→ a0 1 − ia0 k − (a02 − a0 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k) − ik Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion If a0 is natural, then low-energy scattering simplifies further For scattering at momentum k 1/R, we should recover a perturbative expansion in kR for scattering amplitude: f0 (k ) ∝ 1 −→ a0 1 − ia0 k − (a02 − a0 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k) − ik Can we reproduce this simple expansion for the hard-sphere? Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion If a0 is natural, then low-energy scattering simplifies further For scattering at momentum k 1/R, we should recover a perturbative expansion in kR for scattering amplitude: f0 (k ) ∝ 1 −→ a0 1 − ia0 k − (a02 − a0 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k) − ik Can we reproduce this simple expansion for the hard-sphere? Perturbation theory in the hard-sphere potential won’t work: =⇒ 0 hk|V |k0 i ∝ Z 0 dx eik·x V (x) e−ik ·x −→ ∞ R Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion (cont.) Standard solution: Solve the scattering problem nonperturbatively, then expand in kR Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion (cont.) Standard solution: Solve the scattering problem nonperturbatively, then expand in kR For our example, this is easy =⇒ use δ0 (k) = −kR: f0 (k ) ∝ 1 −→ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k ) − ik −→ 1 − ikR − 2k 2 R 2 /3 + O(k 3 R 3 ) Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion (cont.) Standard solution: Solve the scattering problem nonperturbatively, then expand in kR For our example, this is easy =⇒ use δ0 (k) = −kR: f0 (k ) ∝ 1 −→ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k ) − ik −→ 1 − ikR − 2k 2 R 2 /3 + O(k 3 R 3 ) Easy for 2–2 scattering, but not for the many-body problem! Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering In Search of a Perturbative Expansion (cont.) Standard solution: Solve the scattering problem nonperturbatively, then expand in kR For our example, this is easy =⇒ use δ0 (k) = −kR: f0 (k ) ∝ 1 −→ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) k cot δ(k ) − ik −→ 1 − ikR − 2k 2 R 2 /3 + O(k 3 R 3 ) Easy for 2–2 scattering, but not for the many-body problem! EFT approach: k 1/R means we probe at low resolution =⇒ replace potential with a simpler but general interaction Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering EFT for “Natural” Short-Range Interaction A simple, general interaction is a sum of delta functions and derivatives of delta functions. In momentum space, hk|Veft |k0 i = C0 + 1 2 C2 (k2 + k0 ) + C20 k · k0 + · · · 2 Or, Left has most general local (contact) interactions: Left →2i − h ∂ ↔ ∇ C0 † 2 C2 = ψ i + ψ− (ψ ψ) + (ψψ)† (ψ ∇ 2 ψ) + h.c. ∂t 2M 2 16 † + ↔ C20 ↔ † D0 † 3 (ψ ∇ ψ) · (ψ ∇ ψ) − (ψ ψ) + . . . 8 6 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering EFT for “Natural” Short-Range Interaction A simple, general interaction is a sum of delta functions and derivatives of delta functions. In momentum space, hk|Veft |k0 i = C0 + 1 2 C2 (k2 + k0 ) + C20 k · k0 + · · · 2 Or, Left has most general local (contact) interactions: Left →2i − h ∂ ↔ ∇ C0 † 2 C2 = ψ i + ψ− (ψ ψ) + (ψψ)† (ψ ∇ 2 ψ) + h.c. ∂t 2M 2 16 † + ↔ C20 ↔ † D0 † 3 (ψ ∇ ψ) · (ψ ∇ ψ) − (ψ ψ) + . . . 8 6 Dimensional analysis =⇒ C2i ∼ 4π R 2i+1 , M Dick Furnstahl D2i ∼ 4π R 2i+4 M Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Feynman Rules for EFT Vertices − 2i → h ∂ ↔ ∇ C0 † 2 C2 Left = ψ † i + ψ− (ψ ψ) + (ψψ)† (ψ ∇ 2 ψ) + h.c. ∂t 2M 2 16 + ↔ C20 ↔ † D0 † 3 (ψ ∇ ψ) · (ψ ∇ ψ) − (ψ ψ) + . . . 8 6 P/2 + k0 P/2 + k = P/2 − k 0 P/2 − k0 −ihk |VEFT |ki + − iC0 = + −iC2 + k2 + k 0 2 2 + −iC20 k · k0 ··· −iD0 Dick Furnstahl Fermion Many-Body Systems I ··· Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Renormalization Reproduce f0 (k ) in perturbation theory (Born series): f0 (k) ∝ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) (0) Consider the leading potential VEFT (x) = C0 δ(x) or (0) hk|Veft |k0 i =⇒ =⇒ C0 Choosing C0 ∝ a0 gets the first term. Now hk|VG0 V |k0 i: Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Renormalization Reproduce f0 (k ) in perturbation theory (Born series): f0 (k) ∝ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) (0) Consider the leading potential VEFT (x) = C0 δ(x) or (0) hk|Veft |k0 i =⇒ =⇒ C0 Choosing C0 ∝ a0 gets the first term. Now hk|VG0 V |k0 i: Z =⇒ d 3q 1 −→ ∞! 3 2 (2π) k − q 2 + i =⇒ Linear divergence! Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Renormalization Reproduce f0 (k ) in perturbation theory (Born series): f0 (k) ∝ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) (0) Consider the leading potential VEFT (x) = C0 δ(x) or (0) hk|Veft |k0 i =⇒ =⇒ C0 Choosing C0 ∝ a0 gets the first term. Now hk|VG0 V |k0 i: Z =⇒ Λc d 3q 1 Λc ik −→ − + O(k 2 /Λc ) (2π)3 k 2 − q 2 + i 2π 2 4π =⇒ If cutoff at Λc , then can absorb into C0 , but all powers of k 2 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Renormalization Reproduce f0 (k ) in perturbation theory (Born series): f0 (k) ∝ a0 − ia02 k − (a03 − a02 r0 /2)k 2 + O(k 3 a03 ) (0) Consider the leading potential VEFT (x) = C0 δ(x) or (0) hk|Veft |k0 i =⇒ =⇒ C0 Choosing C0 ∝ a0 gets the first term. Now hk|VG0 V |k0 i: Z =⇒ dDq 1 ik D→3 −→ − 3 2 2 (2π) k − q + i 4π Dimensional regularization with minimal subtraction =⇒ only one power of k ! Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Dim. reg. + minimal subtraction =⇒ simple power counting: P/2 + k P/2 + k0 P/2 − k 0 = P/2 − k iT (k, cos θ) + − iC0 − + + +i M 4π !2 (C0 )3 k 2 + − iC2 k 2 Matching: C0 = 4π a0 = 4π R , M M Dick Furnstahl M (C0 )2 k 4π + O(k 3 ) − iC20 k 2 cos θ 3 a2 r C2 = 4π 0 0 = 4π R , M 3 M 2 Fermion Many-Body Systems I ··· Outline Intro EFT Dilute Summary Refs Resolution Low-Energy Scattering Dim. reg. + minimal subtraction =⇒ simple power counting: P/2 + k P/2 + k0 P/2 − k 0 = P/2 − k iT (k, cos θ) + − iC0 − + + +i M 4π !2 (C0 )3 k 2 M (C0 )2 k 4π + − iC2 k 2 + O(k 3 ) − iC20 k 2 cos θ 3 a2 r Matching: C0 = 4π a0 = 4π R , C2 = 4π 0 0 = 4π R , · · · M 3 M M M 2 Recovers expansion order-by-order with perturbative diagrams one power of k per diagram, natural coefficients estimate truncation error from dimensional analysis Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres “Simple” Many-Body Problem: Hard Spheres R Infinite potential at radius R sin(kr+δ) 0 r R ~ 1/ k Scattering length a0 = R Dilute nR 3 1 =⇒ kF a0 1 What is the energy / particle? Dick Furnstahl Fermion Many-Body Systems I F Outline Intro EFT Dilute Summary Refs Spheres Noninteracting Fermi Sea at T = 0 Put system in a large box (V = L3 ) with periodic bc’s spin-isospin degeneracy ν (e.g., for nuclei, ν = 4) fill momentum states up to Fermi momentum kF N=ν kF X k Dick Furnstahl 1, E =ν kF X ~2 k 2 k 2M Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Noninteracting Fermi Sea at T = 0 Put system in a large box (V = L3 ) with periodic bc’s spin-isospin degeneracy ν (e.g., for nuclei, ν = 4) fill momentum states up to Fermi momentum kF N=ν kF X 1, E =ν k Note: R F (k) dk ≈ P i k F (ki )∆ki = Dick Furnstahl kF X ~2 k 2 P i 2M F (ki ) 2π L ∆ni = Fermion Many-Body Systems I 2π L P i F (ki ) Outline Intro EFT Dilute Summary Refs Spheres Noninteracting Fermi Sea at T = 0 Put system in a large box (V = L3 ) with periodic bc’s spin-isospin degeneracy ν (e.g., for nuclei, ν = 4) fill momentum states up to Fermi momentum kF N=ν kF X k 1, E =ν kF X ~2 k 2 k 2M R P P Note: F (k) dk ≈ i F (ki )∆ki = i F (ki ) 2π L ∆ni = In 1-D: L N=ν 2π Z +kF dk = −kF N νkF νkF L =⇒ n = = ; π L π 2π L P i F (ki ) E 1 ~2 kF2 = n L 3 2M In 3-D: V N=ν (2π)3 Z kF d 3k = νkF3 N νkF3 V =⇒ n = = ; 6π 2 V 6π 2 Dick Furnstahl Fermion Many-Body Systems I E 3 ~2 kF2 = n V 5 2M Outline Intro EFT Dilute Summary Refs Spheres Noninteracting Fermi Sea at T = 0 Put system in a large box (V = L3 ) with periodic bc’s spin-isospin degeneracy ν (e.g., for nuclei, ν = 4) fill momentum states up to Fermi momentum kF N=ν kF X k 1, E =ν kF X ~2 k 2 k 2M R P P Note: F (k) dk ≈ i F (ki )∆ki = i F (ki ) 2π L ∆ni = In 1-D: L N=ν 2π Z +kF dk = −kF N νkF νkF L =⇒ n = = ; π L π 2π L P i F (ki ) E 1 ~2 kF2 = n L 3 2M In 3-D: V N=ν (2π)3 Z kF d 3k = νkF3 N νkF3 V =⇒ n = = ; 6π 2 V 6π 2 E 3 ~2 kF2 = n V 5 2M Volume/particle V /N = 1/n ∼ 1/kF3 , so spacing ∼ 1/kF Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Sum Over Fermions in the Fermi Sea (0) Leading order VEFT (x) = C0 δ(x) ELO =⇒ !2 kF X C0 = ν(ν − 1) 1 ∝ a0 kF6 2 k Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Sum Over Fermions in the Fermi Sea (0) Leading order VEFT (x) = C0 δ(x) ELO =⇒ !2 kF X C0 = ν(ν − 1) 1 ∝ a0 kF6 2 k At the next order, we get a linear divergence again: Z =⇒ ∞ ENLO ∝ kF Dick Furnstahl C02 d 3q (2π)3 k 2 − q 2 Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Sum Over Fermions in the Fermi Sea (0) Leading order VEFT (x) = C0 δ(x) ELO =⇒ !2 kF X C0 = ν(ν − 1) 1 ∝ a0 kF6 2 k At the next order, we get a linear divergence again: Z ∞ ENLO ∝ =⇒ kF C02 d 3q (2π)3 k 2 − q 2 Same renormalization fixes it! Particles −→ holes Z ∞ kF 1 = k 2 − q2 Z 0 ∞ 1 − k 2 − q2 Z Dick Furnstahl 0 kF 1 D→3 −→ − k 2 − q2 Z 0 kF 1 ∝ a02 kF7 k 2 − q2 Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Feynman Rules for Hugenholtz Diagrams Ground-state energy density E is sum of Hugenholtz diagrams same vertices as free space (same renormalization!) Feynman rules: 1. Each line is assigned conserved ke ≡ (k0 , ~k) and θ(k − kF ) θ(kF − k) e iG0 (k )αβ = iδαβ + . k0 − ω~k + i k0 − ω~k − i β δ α γ −→ (δαγ δβδ + δαδ δβγ ) (spin-independent) 2. 3. After spinRsummations, δαα → −g in every closed fermion loop. + 4. Integrate d 4 k/(2π)4 with eik0 0 for tadpoles Qlmax 5. Symmetry factor i/(S l=2 (l!)k ) counts vertex permutations and equivalent l–tuples of lines Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Power Counting Power counting rules 1. for every propagator: M/k2F 2. for every loop integration: k5F /M 2i+3n−5 3. for every n–body vertex with 2i derivatives: k2i F /MΛ Diagram with V2in n–body vertices of each type scales as (kF )β : β =5+ ∞ X ∞ X (3n + 2i − 5)V2in . n=2 i=0 e.g., =⇒ V02 = 2 =⇒ β = 5 + (3 · 2 + 2 · 0 − 5) · 2 = 7 =⇒ O(k7F ) Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams E kF2 3 = n V 2M 5 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams O kF6 : E kF2 3 2 = n + (ν − 1) (kF a0 ) V 2M 5 3π Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams E kF2 3 2 = n + (ν − 1) (kF a0 ) V 2M 5 3π O kF6 : O kF7 : + + (ν − 1) 4 (11 − 2 ln 2)(kF a0 )2 35π 2 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams E kF2 3 2 = n + (ν − 1) (kF a0 ) V 2M 5 3π O kF6 : O kF7 : O kF8 : + + (ν − 1) 4 (11 − 2 ln 2)(kF a0 )2 35π 2 + Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams E kF2 3 2 = n + (ν − 1) (kF a0 ) V 2M 5 3π O kF6 : + O kF7 : + (ν − 1) + (ν − 1) 0.076 + 0.057(ν − 3) (kF a0 )3 + O kF8 : + 4 (11 − 2 ln 2)(kF a0 )2 35π 2 + Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres T = 0 Energy Density from Hugenholtz Diagrams E kF2 3 2 = n + (ν − 1) (kF a0 ) V 2M 5 3π O kF6 : + O kF7 : + (ν − 1) + (ν − 1) 0.076 + 0.057(ν − 3) (kF a0 )3 + O kF8 : 4 (11 − 2 ln 2)(kF a0 )2 35π 2 1 (kF r0 )(kF a0 )2 10π 1 3 + (ν + 1) (kF ap ) + · · · 5π + (ν − 1) + + + Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Looks Like a Power Series in kF ! Is it? Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Looks Like a Power Series in kF ! Is it? New logarithmic divergences in 3–3 scattering + Dick Furnstahl ∝ (C0 )4 ln(k /Λc ) Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Looks Like a Power Series in kF ! Is it? New logarithmic divergences in 3–3 scattering ∝ (C0 )4 ln(k /Λc ) + Changes in Λc must be absorbed by 3-body coupling D0 (Λc ) =⇒ D0 (Λc ) ∝ (C0 )4 ln(a0 Λc ) + const. [Braaten & Nieto] d dΛc = 0 =⇒ same coefficient! Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Spheres Looks Like a Power Series in kF ! Is it? New logarithmic divergences in 3–3 scattering ∝ (C0 )4 ln(k /Λc ) + Changes in Λc must be absorbed by 3-body coupling D0 (Λc ) =⇒ D0 (Λc ) ∝ (C0 )4 ln(a0 Λc ) + const. [Braaten & Nieto] d dΛc = 0 =⇒ same coefficient! What does this imply for the energy density? O kF9 ln(kF ) : + + Dick Furnstahl ··· ∝ (ν − 2)(ν − 1) (kF a0 )4 ln(kF a0 ) Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Effective Field Theory Ingredients See “Crossing the Border” [nucl-th/0008064] 1. Use the most general L with low-energy dof’s consistent with global and local symmetries of underlying theory ∂ Left = ψ † i ∂t + ∇2 2M ψ− C0 † 2 2 (ψ ψ) Dick Furnstahl − D0 † 3 6 (ψ ψ) + ... Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Effective Field Theory Ingredients See “Crossing the Border” [nucl-th/0008064] 1. Use the most general L with low-energy dof’s consistent with global and local symmetries of underlying theory ∂ Left = ψ † i ∂t + ∇2 2M ψ− C0 † 2 2 (ψ ψ) − D0 † 3 6 (ψ ψ) + ... 2. Declaration of regularization and renormalization scheme natural a0 =⇒ dimensional regularization and minimal subtraction Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Effective Field Theory Ingredients See “Crossing the Border” [nucl-th/0008064] 1. Use the most general L with low-energy dof’s consistent with global and local symmetries of underlying theory ∂ Left = ψ † i ∂t + ∇2 2M ψ− C0 † 2 2 (ψ ψ) − D0 † 3 6 (ψ ψ) + ... 2. Declaration of regularization and renormalization scheme natural a0 =⇒ dimensional regularization and minimal subtraction 3. Well-defined power counting =⇒ small expansion parameters use the separation of scales =⇒ kF with Λ ∼ 1/R =⇒ kF a0 , etc. Λ O kF6 : E =ρ O kF7 : + kF2 3 2 4 2 + (kF a0 ) + (11 − 2 ln 2)(k a ) + · · · F 0 2M 5 3π 35π 2 Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” One Hamiltonian for all problems and energy/length scales Dick Furnstahl Infinite # of low-energy potentials; different resolutions =⇒ different dof’s and Hamiltonians Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” One Hamiltonian for all problems and energy/length scales Find the “best” potential Dick Furnstahl Infinite # of low-energy potentials; different resolutions =⇒ different dof’s and Hamiltonians There is no best potential =⇒ use a convenient one! Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Dick Furnstahl Infinite # of low-energy potentials; different resolutions =⇒ different dof’s and Hamiltonians There is no best potential =⇒ use a convenient one! Many-body data needed and many-body forces inevitable Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Avoid divergences Dick Furnstahl Infinite # of low-energy potentials; different resolutions =⇒ different dof’s and Hamiltonians There is no best potential =⇒ use a convenient one! Many-body data needed and many-body forces inevitable Exploit divergences Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs (Nuclear) Many-Body Physics: “Old” vs. “New” One Hamiltonian for all problems and energy/length scales Find the “best” potential Two-body data may be sufficient; many-body forces as last resort Avoid divergences Choose diagrams by “art” Dick Furnstahl Infinite # of low-energy potentials; different resolutions =⇒ different dof’s and Hamiltonians There is no best potential =⇒ use a convenient one! Many-body data needed and many-body forces inevitable Exploit divergences Power counting determines diagrams and truncation error Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Web Resources These lectures, including additional notes on each slide, are available at http://www.physics.ohio-state.edu/˜ntg/NPSS/ Class notes for a two-quarter course on “Nuclear Many-Body Physics” given by Dick Furnstahl and Achim Schwenk are available at http://www.physics.ohio-state.edu/˜ntg/880/ (username: physics, password: 880.05) Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs References for Many-Body Physics A.L. Fetter and J.D. Walecka, “Quantum Theory of Many-Particle Systems.” Classic text, but pre-path integrals. Now available in an inexpensive (about $20) Dover reprint. Get it! J.W. Negele and H. Orland, “Quantum Many-Particle Systems.” Detailed and careful use of path integrals. Full of good physics but most of the examples are in the problems, so it can be difficult to learn from. N. Nagaosa, “Quantum Field Theory in Condensed Matter Physics.” Recent text, covers path integral methods and symmetry breaking. A.M. Tsvelik, “Quantum Field Theory in Condensed Matter Physics.” Good on one-dimensional systems. M. Stone, “The Physics of Quantum Fields.” A combined introduction to quantum field theory as applied to particle physics problems and to nonrelativistic many-body problems. Some very nice explanations. R.D. Mattuck, “A Guide to Feynman Diagrams in the Many-Body Problems.” This is a nice, intuitive guide to the meaning and use of Feynman diagrams. N. Goldenfeld, “Lectures on Phase Transitions and the Renormalization Group.” The discussion of scaling, dimensional analysis, and phase transitions is wonderful. G.D. Mahan, “Many-Particle Physics.” Standard, encyclopedic reference for condensed matter applications. P. Ring and P. Schuck, “The Nuclear Many-Body Problem.” Somewhat out of date, but still a good, encyclopedic guide to the nuclear many-body problem. Doesn’t discuss Green’s function methods much and no path integrals. K. Huang, “Statistical Mechanics.” Excellent choice for general treatment of statistical mechanics, with good sections on many-body physics. Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs References for Many-Body Effective Field Theory Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Fermi to Dyson in 1953 [recalled in Nature 427 (2004) 297] Concerning a proposed pseudoscalar meson theory: “There are two ways of doing calculations in theoretical physics”, he said. “One way, and this is the way I prefer, is to have a clear physical picture of the process that you are calculating. The other way is to have a precise and self-consistent mathematical formalism. You have neither.” Dick Furnstahl Fermion Many-Body Systems I Outline Intro EFT Dilute Summary Refs Fermi to Dyson in 1953 [recalled in Nature 427 (2004) 297] I was slightly stunned, but ventured to ask him why he did not consider the pseudoscalar meson theory to be a self-consistent mathematical formalism. He replied, “Quantum electrodynamics is a good theory because the forces are weak, and when the formalism is ambiguous we have a clear physical picture to guide us. With the pseudoscalar meson theory there is no physical picture, and the forces are so strong that nothing converges. To reach your calculated results, you had to introduce arbitrary cut-off procedures that are not based either on solid physics or on solid mathematics.” Dick Furnstahl Fermion Many-Body Systems I