fetter & walecka - department of physicsphysics.wustl.edu/wimd/q540-13-16b.pdf · fetter &...
TRANSCRIPT
Correlations
Fetter & Walecka
QMPT 540
Nucleons in nuclear matter• NN interaction requires summation of ladder diagrams• Study influence of SRC on sp propagator
• Formulate in self-consistent form
• employs noninteracting but dressed convolution of sp propagators
⇥km�m�� | �pphh(K, E) |k�m⇥m⇥�⇤= ⇥km�m�� | V |k�m⇥m⇥�⇤ + ⇥km�m�� | ⇥�pphh(K, E) |k�m⇥m⇥�⇤
= ⇥km�m�� | V |k�m⇥m⇥�⇤ +12
�
m�m��
⇥d3q
(2�)3⇥km�m�� | V |qm⇤m⇤�⇤
� Gfpphh(K, q;E) ⇥qm⇤m⇤� | �pphh(K, E) |k�m⇥m⇥�⇤
Gfpphh(K, q;E) =
� ⇤
�F
dE⇥� ⇤
�F
dE⇥⇥Sp(q + K/2;E⇥)Sp(K/2� q;E⇥⇥)E � E⇥ � E⇥⇥ + i�
�� �F
�⇤dE⇥
� �F
�⇤dE⇥⇥Sh(q + K/2;E⇥)Sh(K/2� q;E⇥⇥)
E � E⇥ � E⇥⇥ � i�
QMPT 540
Lehmann representation• Dispersion relation (arrows for location of poles in energy plane)
• Corresponding self-energy
• Energy integral can be performed (note arrows)
⇤km�m�� | ⇥�pphh(K, E) |k⌅m⇥m⇥�⌅
=�1⇥
� ⇧
2⇤F
dE⌅ Im ⇤km�m�� | ⇥�pphh(K, E⌅) |k⌅m⇥m⇥�⌅E � E⌅ + i�
+1⇥
� 2⇤F
�⇧dE⌅ Im ⇤km�m�� | ⇥�pphh(K, E⌅) |k⌅m⇥m⇥�⌅
E � E⌅ � i�
⇥ ⇤km�m�� | ⇥�⇤(K, E) |k⌅m⇥m⇥�⌅+ ⇤km�m�� | ⇥�⇥(K, E) |k⌅m⇥m⇥�⌅
⇤⇥�(k;E) = �i1�
�
m�m��
⇥d3k�
(2⇥)3
⇥dE�
2⇥G(k�;E�)
⇥ ⇤ 12 (k � k�)m�m�� | ⇥�pphh(K, E + E�) | 1
2 (k � k�)m�m��⌅
⇤⇥�(k;E) =1�
�
m�m��
⇥d3k⌅
(2⇥)3
⇥ ⇥F
�⇧dE⌅ ⇤ 1
2 (k � k⌅)m�m�� | ⇥�⇤(E + E⌅) | 12 (k � k⌅)m�m��⌅Sh(k⌅, E⌅)
� 1�
�
m�m��
⇥d3k⌅
(2⇥)3
⇥ ⇧
⇥F
dE⌅ ⇤ 12 (k � k⌅)m�m�� | ⇥�⇥(E + E⌅) | 1
2 (k � k⌅)m�m��⌅Sp(k⌅, E⌅)
⇥ ⇥⇤⇤(k;E) + ⇥⇤⇥(k;E)
QMPT 540
Final steps and implementation• Total self-energy
• includes HF-like term
• Practical calculations first done with mean-field sp propagators in scattering equation
⇥(k;E) = ⇥V (k)� 1⇥
� ⇧
�F
dE⌅ Im ⇥(k;E⌅)E � E⌅ + i�
+1⇥
� �F
�⇧dE⌅ Im ⇥(k;E⌅)
E � E⌅ � i�
= ⇥V (k) + �⇥⇤(k;E) + �⇥⇥(k;E)
�V (k) =⇥
d3k�
(2⇥)31�
�
m�m��
⇥ 12 (k � k�)m�m�� | V | 1
2 (k � k�)m�m��⇤n(k�)
⇤(0)⇥�(k;E) =
1⇥
�
m�m��
⇥d3k⇤
(2⇤)3⇥ 1
2 (k � k⇤)m�m�� | ⇥�(0)⇥ (E + ⌅(k⇤)) | 1
2 (k � k⇤)m�m��⇤ �(kF � k⇤)
� 1⇥
�
m�m��
⇥d3k⇤
(2⇤)3⇥ 1
2 (k � k⇤)m�m�� | ⇥�(0)� (E + ⌅(k⇤)) | 1
2 (k � k⇤)m�m��⇤ �(k⇤ � kF )
QMPT 540
Results for mean-field input• Realistic interactions generate pairing instabilities• Avoid with “gap” is sp spectrum according to
• Hole strength spread so “sp energy” below QP energy --> gap
• Requires full knowledge of self-energy • Self-consistent determination of sp spectrum
• Subsequent determination of self-energy constrained by sp spectrum -> imaginary part exhibits momentum dependent domains
�(k) =�
dE E Sh(k, E)�dE Sh(k, E)
k < kF
�(k) =�
dE E SQ(k, E)�dE SQ(k,E)
= EQ(k) k > kF
QMPT 540
Self-energy below Fermi energy• Wave vectors 0.1 (solid), 0.51 (dotted), and 2.1 fm-1 (dashed)• kF = 1.36 fm-1
• Im part
• Spectral functions with peaks at• QP spectral function
• with and
EQ(k) =�2k2
2m+ Re�(k;EQ(k))
SQ(k, E) =1�
Z2Q(k) | W (k) |
(E � EQ(k))2 + (ZQ(k)W (k))2
W (k) = Im �(k;EQ(k))ZQ(k) =
⇤1�
��Re �(k;E)
�E
⇥
E=EQ(k)
⌅�1
QMPT 540
Spectral functions• Near kF about 70% of sp strength is contained in QP peak• additional ~13% distributed below the Fermi energy
• remaining strength (~17%) above the Fermi energy• Note “gap”
• Distribution narrows• towards kF
QMPT 540
Spectral functions above the Fermi energy• Wave vectors 0.79 (dotted), 1.74 (solid), and 3.51 fm-1 (dashed)• Common distribution -> SRC
• For 0.79 -> 17%• εF + 100 MeV -> 13%
• above 500 MeV -> 7%• Without tensor force:
• strength only 10.5%• Momentum distribution
• n(0) same for different methods• and interactions (not at kF)
• Solid: self-consistent
QMPT 540
Self-consistent results• Wave vectors 0.0 (solid), 1.36 (dotted), and 2.1 fm-1 (dashed)• Limited set of Gaussians --> self-consistent
• Spectral functions• Main difference:
– common strength
• Slightly less correlated• ZF from 0.72 to 0.75
QMPT 540
SRC and saturation• Energy sum rule
• Contribution from high momenta after energy integral for different densities for Reid potential
EN0
N=
�
2⇤
⇤d3k
(2⇥)3
⇤ �F
�⇥dE
��2k2
2m+ E
⇥Sh(k;E)
QMPT 540
Saturation properties of nuclear matter• Colorful and continuing story• Initiated by Brueckner: proper treatment of SRC in medium ->
ladder diagrams but only include pp propagation
• Brueckner G-matrix but Bethe-Goldstone equation…• Dispersion relation
• Include HF term in “BHF” self-energy
• Below Fermi energy: no imaginary part
⇥km�m�� | G(K, E) |k�m⇥m⇥�⇤ = ⇥km�m�� | V |k�m⇥m⇥�⇤
+12
�
m�m��
⇥d3q
(2⇤)3⇥km�m�� | V |qm⇤m⇤�⇤ ⇥(|q + K/2| � kF ) ⇥(|K/2 � q| � kF )
E � ⌅(q + K/2) � ⌅(K/2 � q) + i�⇥qm⇤m⇤� | G(K, E) |k�m⇥m⇥�⇤
⇤km�m�� | G(K, E) |k⇥m⇥m⇥�⌅ = ⇤km�m�� | V |k⇥m⇥m⇥�⌅ � 1⇥
� ⇤
2⇤F
dE⇥ Im ⇤km�m�� | �G(K, E⇥) |k⇥m⇥m⇥�⌅E � E⇥ + i�
⇥ ⇤km�m�� | V |k⇥m⇥m⇥�⌅+ ⇤km�m�� | �G�(K, E) |k⇥m⇥m⇥�⌅
�BHF (k;E)) =⇥
d3k�
(2⇤)31⇥
�
m�m��
�(kF � k�) ⇥ 12 (k � k�)m�m�� | G(k + k�;E + ⌅(k�) | 1
2 (k � k�) m�m��⇤
QMPT 540
BHF• DE for k < kF yields solutions at
• with strength < 1• Since there is no imaginary part below the Fermi energy, no
momenta above kF can admix -> problem with particle number
• Only sp energy is determined self-consistently• Choice of auxiliary potential
– Standard only for k < kF (0 above)
– Continuous all k
• Only one calculation of G-matrix for standard choice• Iterations for continuous choice
�BHF (k) =�2k2
2m+ �BHF (k; �BHF (k))
Us(k) = �BHF (k; �BHF (k))
Uc(k) = �BHF (k; �BHF (k))
QMPT 540
BHF• Propagator• Energy
• Rewrite using on-shell self-energy
• First term: kinetic energy free Fermi gas• Compare
• so BHF obtained by replacing V by G
GBHF (k;E) =⇥(k � kF )
E � ⇤BHF (k) + i�+
⇥(kF � k)E � ⇤BHF (k)� i�
EA0
A=
⇥
2⌅
⇤d3k
(2⇤)3
��2k2
2m+ ⇧BHF
⇥�(k � kF )
EA0
A=
4⇤
⇥d3k
(2⇥)3�2k2
2m+
12⇤
⇥d3k
(2⇥)3
⇥d3k�
(2⇥)3�
m�m��
�(kF � k)�(kF � k�)
⇥ 12 (k � k�) m�m�� | G(k + k�; ⌅BHF (k) + ⌅BHF (k�)) | 1
2 (k � k�) m�m��⇤
EHF =12
⇤
p
�(pF � p)�
p2
2m+ ⇥HF (p)
⇥
= TFG +12
⇤
pp�
�(pF � p)�(pF � p�) ⇥pp�| V |pp�⇤
QMPT 540
BHF• Binding energy usually
within 10 MeV from empirical volume term in the mass formula even for very strong repulsive cores
• Repulsion always completely cancelled by higher-order terms
• Minimum in density never coincides with empirical value when binding OK -> Coester band
Location of minimum determined by deuteron D-state probability
QMPT 540
Historical perspective• First attempt using scattering in the medium Brueckner 1954
• Formal development (linked cluster expansion) Goldstone 1956
• Reorganized perturbation expansion (60s) Bethe & students involving ordering in the number of hole lines BBG-expansion
• Variational Theory vs. Lowest Order BBG (70s) Clark (also crisis paper) Pandharipande
• Variational results & next hole-line terms (80s) Day, Wiringa
• New insights from experiment & theory NIKHEF Amsterdam about what nucleons are up to in the nucleus (90s)
• 3-hole line terms with continuous choice (90s) Baldo et al.
• Ongoing...
QMPT 540
Some remarks• Variational results gave more binding than G-matrix calculations• Interest in convergence of Brueckner approach
• Bethe et al.: hole-line expansion• G-matrix: sums all energy terms with 2 independent hole lines
(noninteracting ...)
• Dominant for low-density• Phase space arguments suggests to group all terms with 3
independent hole lines as the next contribution
• Requires technique from 3-body problem first solved by Faddeev -> Bethe-Faddeev summation
• Including these terms generates minima indicated by✴in figure
• Better but not yet good enough
QMPT 540
More• Variational results and 3-hole-line results more or less in
agreement• Baldo et al. also calculated 3-hole-line terms with continuous
choice for auxiliary potential and found that results do not depend on choice of auxiliary potential, furthermore 2-hole-line with continuous choice is already sufficient!
• Conclusion: convergence OK for a given realistic two-body interaction for the energy per particle
• Very recently: Monte Carlo calculations may modify this assessment
• Also: for other observables no such statements can be made• Still nuclear matter saturation problem!
QMPT 540
Possible solutions• Include three-body interactions: inevitable on account of isobar
– Simplest diagram: space of nucleons -> 3-body force
– Inclusion in nuclear matter still requires phenomenology to get saturation right
– Also needed for few-body nuclei; there is some incompatibility
• Include aspects of relativity– Dirac-BHF approach: ad hoc adaptation of BHF to nucleon spinors
– Physical effect: coupling to scalar-isoscalar meson reduced with density
– Antiparticles? Dirac sea? Three-body correlations?
– Spin-orbit splitting in nuclei OK
– Nucleons less correlated with higher density? (compare liquid 3He)
QMPT 540
Personal perspective• Based on results from (e,e’p) reactions as discussed here
– nucleons are dressed (substantially) and this should be included in the description of nuclear matter (depletion, high-momentum components in the ground state, propagation w.r.t. correlated ground state <--> BHF?)
– SRC dominate actual value of saturation density• from 208Pb charge density: 0.16 nucleons/fm3
• determined from s-shell proton occupancy at small radius• occupancy determined mostly by SRC (see next chapter)
– Result for SCGF of ladders• Ghent discrete approach• St. Louis gaussians (Libby Roth)
• ccBHF --> SCGF closer to box• do not include LRC!!
Inclusion of Δ-isobars as 3N- and 4N-force
NPA389,492(82)
Prog.Part.Nucl.Phys.12,529(83)
2N,3N, and 4N from
B. D. Day, PRC24,1203(81)
Pion collectivity: nuclei vs. nuclear matter
Vπ (q) = −fπ2
mπ2
q2
mπ2 + q2
• Pion collectivity leads to pion condensation at higher density in nuclear matter (including Δ-isobars) => Migdal ...
• No such collectivity observed in nuclei ⇒ LAMPF / Osaka data
• Momentum conservation in nuclear matter dramatically favors amplification of π-exhange interaction at fixed q
• Nuclei: interaction is sampled over all momenta Phys. Lett. B146, 1(1984)
Needs further study!
⇒ Exclude collective pionic contributions to nuclear matter binding energy
Nuclear Saturation without π-collectivity • Variational calculations treat LRC (on average) and SRC
simultaneously (Parquet equivalence) so difficult to separate LRC and SRC
• Remove 3-body ring diagram from Catania hole-line expansion calculation ⇒ about the correct saturation density
• Hole-line expansion doesn’t treat Pauli principle very well• Present results improve treatment of Pauli principle by self-
consistency of spectral functions => more reasonable saturation density and binding energy acceptable
• Neutron matter: pionic contributions must be included (Δ)
Two Nuclear Matter Problems
• With π-collectivity and only nucleons
• Variational + CBF and three hole-line results presumed OK
• NOT OK if Δ-isobars are included
• Relevant for neutron matter
• Without π-collectivity • Treat only SRC• But at a sophisticated level by
using self-consistency• Confirmation from Gent results ⇒ PRL 90, 152501 (2003)
• 3N-forces difficult ⇒ π ...
• Relativity?
The usual one The relevant one
Comments
• Saturation depends on NNσ-coupling in medium but underlying correlated two-pion exchange behaves differently in medium
• m* ⇒ 0 with increasing
ρopposite in liquid 3He appears unphysical
• Dirac sea under control?• sp strength overestimated
too many nucleons for k<kF
• Microscopic models yield only attraction in matter and more so with increasing ρ
• Microscopic background of phenomenological repulsion in 3N-force (if it exists)?
• 4N-, etc. forces yield increasing attraction with ρ
• Needed in light nuclei!• Mediated by π-exchange
Relativity Three-body forces