Spectral Continuity in Dense QCD Phys.Rev.D.78:011501,2008 - - PowerPoint PPT Presentation

spectral continuity in dense qcd
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Spectral Continuity in Dense QCD Phys.Rev.D.78:011501,2008 - - PowerPoint PPT Presentation

Spectral Continuity in Dense QCD Phys.Rev.D.78:011501,2008 Quark-Hadron continuity (in-medium) QCD sum rules Key words Different roles of vacuum condensates arXiv:0802.4143[ hep-ph ] M. T. (Saga) N. Yamamoto (Tokyo) T. Hatsuda (Tokyo) (


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SLIDE 1 Spectral Continuity in Dense QCD (有限密度QCDにおけるスペクトル連続性)
  • T. Hatsuda (Tokyo)
  • N. Yamamoto (Tokyo)
  • M. T. (Saga)
arXiv:0802.4143[hep-ph] Phys.Rev.D.78:011501,2008 Key words “Spectral Continuity” of hadrons (in-medium) QCD sum rules Different roles of vacuum condensates Quark-Hadron continuity μ mV ∝ q q 1/3 ∝ qq µ 2 ∝Δ µc
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SLIDE 2 Plan of this talk 1. Introduction and motivations
  • 2. In-medium QCD Sum Rules (QSR)
  • 3. Flavor-octet vector mesons in QSR
  • 4. Flavor-singlet vector meson in QSR
  • 5. “Spectral Continuity” of vector mesons
  • 6. Sum-mary and Per-spect-ives
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SLIDE 3
  • 1. Introduction and motivations
Exploring the QCD phase diagram is challenging ・Big-Bang Cosmology, Heavy Ion Collisions (Little-Bang) ・Compact Stars (Neutron Stars, Quark Stars) ・Strongly-coupled Quantum Field Theory (QCD) Big-Bang Cosmology Compact Stars QCD coupling const. Heavy Ion Collisions QCD Phase Diagram Observation QCD Cosmology Astrophysics Nuclear Particle Physics Condensed Matter Physics Many-body problem Critical phenomena new state
  • f matter
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SLIDE 4 QCD phase transition and the phase diagram [ Collins-Perry (1975) ] QCD @ high temperature(T ) / density(ρ) ・asymptotic freedom ・screening of color force V(r) ~ αs(T,µ) r e −mscr “weakly interacting gas of quarks/gluons” ∴QCD vacuum undergoes a phase change at some values of T and ρ! Model calculations and numerical simulations ↓ Strongly indicate the existence of such a transition from hadron to quark-gluon phase Tc ~ (150 − 200)MeV ~ 10 12K ρc ~ several × ρnm ~ 1012kg⋅ cm−3 ρ T Quark-gluon plasma (QGP) Hadron Color superconductor (CSC) Tc ρc “Conjectured phase diagram” (roughly speaking)
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SLIDE 5 Hatsuda-Yamamoto-Baym-M.T., Phys. Rev. Lett. 97 (2006) 122001 Possible New Critical Point in Dense QCD @μ≠0 ・Interplay b/w chiral & diquark condensates ・Presence of the U(1) axial anomaly New critical point & Crossover from hadron-to-CSC !! Ginzburg-Landau (GL) model Cartoon phase diagram in 2-light +1-medium flavors : critical point : crossover
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SLIDE 6 Appearance of a new critical point Ginzburg-Landau free energy in massless 3 flavor quark matter Ω3F = a 2σ 2 − c 3 + b 4 σ 4       + α 2 d 2 + β 4 d 4       − γd σ : chiral condensate d : diquark condensate a,b,c,α,β,γ : GL parameters ・Mass term for d ・external field for σ anomaly-driven ‘tHooft interaction (equivalent to Ising Ferro-magnet) Possible phases
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SLIDE 7 Comments 1. All the lines and the points characterizing the whole phase boundaries can be determined analytically.
  • 2. A similar critical point at low temperature has been derived by
Kitazawa et al. [PTP108(2002)929], using the 2-flavor NJL model with scalar and vector type 4-fermion interactions. However since the axial anomaly does not produce a triple boson coupling in 2-flavors, the origin of their critical point will be different with that discussed here.
  • 3. We performed the similar analysis in 2 flavor case and
this case is found in an anisotropic anti-ferromagnet in reality such as GdAlO3 (e.g., see Chaikin-Lubensky’s textbook) Interplay between chiral and diquark condensates Intriguing!!
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SLIDE 8 Excitation spectra Hatsuda-Yamamoto-Baym-M.T., Phys. Rev. D76 (2007) 074001 Generalized Gell-Mann-Oaks-Renner (GOR) relation Low energy excitations ~ Nambu-Goldstone (NG) bosons associated with chiral symmetry breaking (in both hadronic and CSC phases !) ・An example of ”spectral continuity ” of hadrons ・A concrete realization of “quark-hadron continuity ” (Schafer-Wilczek) ..
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SLIDE 9 Pion Pion mass splitting mass splitting unstable Taken from Gordon’s talk in QM08
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SLIDE 10 Quark-Hadron (QH) continuity
  • T. Schafer and F. Wilczek, Phys. Rev. Lett. 82 (1999) 3956
excitations low μ(hadron) high μ (CFL) NG bosons π(&H ) π’&H Vector mesons Fermions Baryons (gapped) quarks ρ,ω,φ,K* (massive) gluons However… Investigating some general aspects of hadron spectrum in medium QCD sum rules (QSR) vector mesons (8+1) gluons (8) baryons (8) quarks (9) .. Shifman-Vainshtein-Zakharov, Nucl.Phys.B147 (1979) 385. mismatch? 3 = f N
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SLIDE 11
  • 2. QCD sum rule (QSR)
Current correlators Dispersion relations ΠL AB(ω) = lim r k →0 i r k 2 d 4xe ikx RJ0 A(x)J0 B(0) ΠL(ω) = ρ(u) u2 − (ω + iε)2 du2 Operator product expansion (OPE): ΠL(Q2 → ∞) ~ Cn n (Q2) On Q2n pole continuum ρ(u) u “phenomenology” “spectral function”
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SLIDE 12 QSR (cont’d)
  • 1. In medium, not only the Lorentz scalar but also the tensor
  • perators in OPE contribute to the correlation functions.
(Hatsuda-Lee ‘92, Hatsuda-Koike-Lee ‘93) 2. The spectral function is just phenomenologically given in terms of so called “resonance parameters”. A = q τ Aγµq with q = (u,d,s) τ A tr τ Aτ B [ ] = 2δ AB (A = 0,L,8) In the following, we focus on flavor octet and singlet vector mesons in 3 flavor quark matter at zero temperature and finite density with m = 0. Comments q ρ(u) : U(3) generators with
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SLIDE 13 Warm-up --non-interacting quark matter@μ≠0 -- ΠL ( free)(Q) = − 1 2 logQ 2 + 16 9 q+i∂0q Q 4 + 64 9 q+i∂0 3q Q 6 Spectral function in free quark matter ρ ( free)(u) = Fδ(u 2) + Aθ(u 2 − S0) S0 = (2µ) 2 A =1/(2π 2) F = AS0 scattering of quarks on the Fermi surface with external current, i.e., the Laundau damping term (pole part) decay of the external current into qq-pair with Pauli blocking effect (continuum part) F A S0 u 2 ρ ( free)(u) “pole + continuum” “resonance parameters” Lorentz non-scalar operators
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SLIDE 14 Comment Corrections of the form and to this case can be taken into account in perturbation theory and are compensated by the perturbative corrections to the resonance parameters and the shape of the spectral function. αslnQ 2 αs(µ/Q) n How the genuine nonpertubative effects such as the condensates affect properties of hadrons from QSR? ? F A S0 u 2 ρ ( free)(u) “pole + continuum”
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SLIDE 15 ΠL (8,1) = ΠL ( free) + δΠL (8,1), δΠL (8) = − παs Q 6 1 4 (q γµγ5τ aλ a'q) 2 + 8 27 (q γµλ a'q) 2       δΠL (1) = − παs Q6 2(q γµγ5τ 0λa'q)2 + 8 27 (q γµλa'q)2       In-medium OPE (vector mesons) (1)(x) ≡ q (x)τ 0γµq(x) (8)(x) ≡ q (x)τ aγµq(x), λ a : color SU(3) generators τ a : flavor SU(3) generators (a =1 ~ 8) ΠL (8) ≡ 1 8 ΠL AA A=1 8 , ΠL (1) ≡ ΠL 00
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SLIDE 16 Comments
  • 1. There are several operators neglected up to
whose explicit forms are given in Hatsuda-Lee ‘92, Hatsuda-Koike-Lee ‘93.
  • 2. Among others, the gluon condensate
if it exists, affects the octet and singlet mesons in the same way.
  • 3. The non-scalar operators like the quark-gluon mixed
  • perators and the twist-4 quark operators do not
produce the chiral and diquark condensates and lead only to perturbative corrections to O(1/Q 6), αs π TrFµν 2 , ΠL ( free). 『twist(τ) ≡ cano. dim.(d )-spin』 Ο6,4 = q {Dµ,* Gνλ}γ λγ 5q 2 4 , 4 µν π α TrF s = Ο e.g.) Οd,τ
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SLIDE 17 Pairing patterns and factorization Let us consider here chiral condensate and diquark condensate which are in the most attractive channels (MAC ): q q qq q i αq j α = diag(σ,σ,σ) 1 4 εijkεαβγ q j βCγ5Λ+qk γ = diag(ϕ,ϕ,ϕ) i, j,k : α,β,γ : flavor color Λ+ : positive energy projection op. After rewriting 4 quark ops. in chiral basis and making the Fierz rearrangement together with the factorization ansatz: , we obtain O = P l ⋅ P l l ≅ P l l 2 Πσ = − 448πα s 81Q 6 σ 2 Πϕ (8) = − 5 22 Πϕ (1) = − 320πα s 27Q6 ϕ 2 δΠL (8,1) ≅ Πσ + Πϕ (8,1), where
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SLIDE 18 Comments
  • 1. The qualitative conclusion in the present work
do not depend on the factorization ansatz.
  • 2. Since the chiral condensate is flavor-diagonal ,
it does not distinguish between octet and singlet.
  • 3. While, the diquark condensate has color-flavor
structure so that it can smell flavors differently. This is why the flavor-octet and -singlet vector mesons, which are almost degene
  • rate at low density, tend to split at high
density due to the appearance of diquark condensates.
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SLIDE 19 F − AS0 = 0 2FmV 2 − AS0 2 = − (2µ) 4 2 3FmV 4 − AS0 3 = − (2µ)6 2 + O (8)
  • 3. Flavor-octet vector mesons in QSR
Spectral function ρ (8)(u) = Fδ(u 2 − mV 2 ) + Aθ(u 2 − S0) Plugging this into the dispersion relation, carrying out the asymptotic expansion in terms of , and comparing the result with the OPE expression: 1/Q 2 O (8) = − 448παs 27 σ 2 + 15 7 ϕ 2       < 0 Finite energy sum rules (FESR)
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SLIDE 20 Solutions of FESRs μ=0 ϕ = 0 ( ) mV (8) ( ) 2 → 448π 3αs 27 σ 2       1/3 μ≠0 t 4 + 6t 2 − 4(1+ r (8))t − 3 = 0 From FESRs, we have the following quartic equation: t = S0 (2µ) 2 r (8) = − 2π 2 (2µ) 6 O (8) In a situation where one finds a unique solution: 0 < r (8) <<1, S0 ≅ (2µ) 2 + mV (8) ( ) 2 and mV (8) ( ) 2 ≅ 56π 3αs 81µ 4 σ 2 + 15 7 ϕ 2       a new formula relating
  • ctet vector meson mass
to chiral condensate and diquark one !! (σ) (ϕ)
  • N. V. Krasnikov et al.,
  • Z. Phys.C19 (1983) 301
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SLIDE 21 mV (8) → 20 3 Δ ≅ 2.6Δ Octet (cont’d) mV (8) ( ) 2 ≅ 56π 3αs 81µ 4 σ 2 + 15 7 ϕ 2       For and µ = 500MeV, αs ~ 1 σ ~ ϕ ~ (150MeV) 3, mV (8) ≅100MeV. At asymptotic high density, we have σ~0 and the weak coupling relation : ϕ = 3µ 2π 3αs (Δ: fermion gap) μ mV (8) ∝ q q 1/3 ∝ qq µ 2 ∝Δ (T. Schafer, Nucl.Phys.B575(‘00)269) ① ② .. Spectral change of
  • ctet vector meson
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SLIDE 22 ρ (1)(u) = FHδ(u 2) + Fδ(u 2 − mV 2 ) + Aθ(u 2 − S0)
  • 4. Flavor-singlet vector mesons in QSR
In this case, unlike the flavor octet, the NG scalar boson associated with U(1) breaking contributes to the spectral function B Spectral function FESRs F + FH − AS0 = 0 2FmV 2 − AS0 2 = − (2µ) 4 2 3FmV 4 − AS0 3 = − (2µ)6 2 + O (1) O (1) = − 448παs 27 σ 2 − 66 7 ϕ 2       This could be either positive or negative!! a1
  • cf. this is analogous to the situation where not only meson but also the
pion contribute to the axial-vector current correlation in the vacuum.
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SLIDE 23 Although sum rules are not closed due to the extra parameter
  • ne can still select a possible solution under physical constraints
such as positivity of the spectral function and the small magnitude of From FESRs, we have the following set of equations: where Singlet (cont’d) FH, ρ(u) r (1) ≡ − 2π 2 (2µ) 6 O (1) . 2t 3 − 3m 2t 2 + 3m 2 − 2 − 2r (1) = 0 2 fm2 − t 2 +1= 0 t ≡ S0 (2µ) 2 , m ≡ mV (1) 2µ , f ≡ F FH , r (1) ≡ − 2π 2 (2µ) 6 O (1) could be positive
  • r negative!!
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SLIDE 24 Level crossing/repulsion [the case with ] r (1) = 0 t=1 is a trivial solution from the cubic eq. and there is another positive solution . As the result we find two solutions for :
  • ne is massless (A) and the other is heavier
than (B). (see the right cartoon) (t+) mV (1) [the case with ] r (1) ≠ 0 In this case, t=1 is not a solution any more. According to the sign of the resultant picture gets dramatically different. r (1), m 2 t 1 t = 2 fm2 +1 A B 2/3 (a) r (1) > 0 m 2 t 2/3 1 t = 2 fm2 +1 B r (1) < 0 (b) m 2 t 2/3 1 t = 2 fm2 +1 t = t+ A B t =1 1 “level crossing” “level repulsion” solution disappears!
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SLIDE 25 Physical interpretations Let us assume that chiral condensate is an increasing function and diquark condensate is a decreasing function of μ. Then starts from some positive value at low density and will change its sign to negative at a certain intermediate chemical potential which is given by the condition, At lower density, as seen from the left panel of the previous cartoon, a light solution (A) exists. However as soon as changes the sign, the light solution is gone (right panel) and only the heavy solution (B)
  • exists. Since this heavy solution is above the threshold for decay,
it is not expected to appear as a sharp resonance in reality. Therefore, unlike the octet case, (σ) (ϕ) r (1) µc, σ 2 = (66/7)ϕ 2. r (1) q q the singlet vector meson disappears from the low-energy spectrum at high density !
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SLIDE 26
  • 5. “Spectral Continuity” of vector mesons
1. Flavors and colors are mixed in the CFL phase 2. The light gluonic mode (the CFL plasmon) mpl. CFL ≅ O(Δ) Flavor-octet vector mesons Flavor-singlet vector meson mV (8) ≅ O(Δ) ( ) disappears at high density survive Our results On the other hand… Strongly suggest the QH continuity of vector mesons?
  • H. Malekzadeh and D. Rischke,
Phys.Rev.D73 (2006) 114006
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SLIDE 27 Schematic plot of the vector meson masses μ mV ∝ q q 1/3 ∝ qq µ 2 ∝Δ
  • ctet
singlet µc lower density almost degenerate (nonet) with the mass governed by chiral condensate medium density mass splitting b/w octet and singlet developed due to diquark condensates higher density
  • ctet survive as light modes, while singlet disappears from the low-energy spectrum
q q qq
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SLIDE 28
  • 6. Sum-mary and Per-spect-ives
・”Spectral Continuity” of hadrons ・Vector mesons in quark matter using in-medium QSR ・New mass formula (diquark condensate) ・Fate of octet/singlet vector mesons at high density
  • ctet ~ survive as the light excitations of
singlet ~disappears from the low-energy spectrum Diquark says “Yeah, I can smell you” ・Possible connection to the quark-hadron continuity ・Spectral continuity of baryons (connected to gapped quarks?) ・Width of the excitations ・Incorporating nonzero quark masses ・Effect of confinement (OPE is a local-operator expansion) ・Utilizing gauge/gravity duality (field-operator correspondence) O(Δ) Summary Perspectives
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SLIDE 29 Back-up slides
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SLIDE 30
  • T. Schafer and F. Wilczek, Phys.Rev.Lett.82 (1999) 3956
…This superfluidity, whatever its source, supplies us with the key to the riddle of the missing vector meson. For once there is a massless singlet scalar, the putative singlet vector becomes radically unstable, and should not appear in the effective theory. … Finally, there is the question of the “extra” singlet
  • baryon. This is the most straightforward. In the original
calculations, it was found that the singlet gap is much larger than the octet gap. Thus the singlet baryon is predicted to be considerably heavier than the octet.
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SLIDE 31 How about photon? (Jean-Paul Blaizot) Zero density ρ-ωーphoton mixing (Vector dominance) High density (CFL) gluonーphoton mixing em em c U U SU ) 1 ( ~ ) 1 ( ) 3 ( → × “Weinberg-Salam” How the photon branch is connected from low to high density?
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SLIDE 32 What governs the QCD phase diagram? 1. Structures of interactions and their changes in T and ρ 2. Order parameters, i.e., vacuum condensates 3. Existence of external parameters (e.g., quark mass) 4. Physical constraints (neutrality conditions,etc. )
  • 5. Universality arguments in critical phenomena
  • 6. Models to be applied
  • 7. Assumptions and approximations to be made
Each person may propose its own phase diagram… M M 蓋然性?
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SLIDE 33 Ginzburg Ginzburg-Landau theory of
  • Landau theory of tricritical
tricritical/critical point /critical point Taken from “Quark-Gluon Plasma” Yagi, Hatsuda and Miake (Cambridge Univ. Press, 2005)
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SLIDE 34 Prediction for the location of the critical point Prediction for the location of the critical point Taken from hep-lat/0701002, M. Stephanov
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SLIDE 35 Recipe to construct Recipe to construct Ginzburg Ginzburg-Landau (GL) free-energy
  • Landau (GL) free-energy
Diquark Diquark condensate condensate Chiral Chiral condensate condensate Terms to appear in GL expansions Terms to appear in GL expansions Chiral Chiral: : Diquark Diquark: : Breaking U(1)A(Axial anomaly)
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SLIDE 36 ・ ・ Mass term: Mass term: ・ ・ Mixing term: Mixing term: Ginzburg Ginzburg-Landau effective
  • Landau effective Lagrangian
Lagrangian Effective Effective Lagrangian Lagrangian ・ ・ Kinetic term: Kinetic term: Pion Pion at low density at low density Generalized Generalized pion pion at high density at high density
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SLIDE 37 A toy model A toy model diagonalize diagonalize: : Lagrangian Lagrangian: : Mass formula: Mass formula:
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SLIDE 38 Axial-vector mesons at high density Axial-vector mesons at high density [preliminary] 1/Q2 1/Q4 1/Q6
  • Finite Energy Sum Rules:
  • Weak coupling QCD Son-Stephanov (’01)
  • Solution:
expected not to appear as a sharp resonance in reality.