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Lattice QCD, Random Matrix Theory and chiral condensates

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[Asahi shimbun, 25Apr07, Nikkei shimbun,30Apr07, Yomiuri shimbun 28May07 ] ... [Fodor et al. 2004] 16. 3. Lattice QCD with. exact chiral symmetry ... – PowerPoint PPT presentation

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Title: Lattice QCD, Random Matrix Theory and chiral condensates


1
Lattice QCD, Random Matrix Theory and chiral
condensates
  • JLQCD and TWQCD collaboration, Phys.Rev.Lett.98,17
    2001(2007) (hep-lat/0702003), arXiv0705.3322
    hep-lat to appear in Phys.Rev.D.
  • Asahi shimbun, 25Apr07, Nikkei shimbun,30Apr07,
    Yomiuri shimbun 28May07
  • Nature 47, 118 (10 May 2007), CERN COURIER,
    Vol47, number 5
  • Hidenori Fukaya (RIKEN Wako)
  • with S.Aoki, T.W.Chiu, S.Hashimoto, T.Kaneko,
    H.Matsufuru, J.Noaki, K.Ogawa,M.Okamoto,T.Onogi
    and N.Yamada
  • JLQCD collaboration

2
1. Introduction
  • Chiral symmetry
  • and its spontaneous breaking are important !
  • Mass gap between pion and the other hadrons
  • pion as (pseudo) Nambu-Goldstone boson
  • while the other hadrons acquire the mass ?QCD.
  • Soft pion theorem
  • Chiral phase transition at finite temperature
  • Banks-Casher relation Banks Casher, 1980
  • Chiral SSB is caused by Dirac zero-modes.

3
1. Introduction
  • Chiral Random Matrix Theory (ChRMT)
  • is an equivalent description of the moduli
    integrals of chiral perturbation theory.
  • The spectrum of ChRMT is expected to match with
    the QCD Dirac spectrum ChRMT predicts
  • Distribution of individual Dirac eigenvalues
  • Spectral density
  • Spectral correlation functions
  • as functions of
    m, S and V,
  • which is helpful to analyze lattice
    data.
  • Shuryak Verbaarschot,1993,
  • Verbaarschot Zahed,
    1993,Damgaard Nishigaki, 2001

4
1. Introduction
  • Chiral Random Matrix Theory (ChRMT)
  • For example, ChRMT knows finite V and m
    corrections in Banks-Casher relation
  • In m-gt0 limit with V8
  • ?(?) is flat and the height
  • gives S (Banks-Casher).
  • Finite m and V corrections
  • are analytically known.
  • Note the same S
  • with finite V and m !

5
1. Introduction
  • Lattice QCD
  • is the most promising approach to confirm
    chiral SSB
  • from 1-st principle calculation of QCD. But
  • Chiral symmetry is difficult. Nielsen Ninomiya
    1981
  • m ? 0 is difficult (large numerical cost).
  • V ? 8 is difficult (large numerical cost).
  • Therefore, the previous works were limited, with
  • Dirac operator which breaks chiral symmetry.
    (Wilson or staggered fermions, Domain-wall
    fermion is better but still has the breaking
    effects 5MeV. )
  • Heavier u-d quark masses 20-50MeV than real
    value a few MeV.
  • ? needs unwanted operator mixing with opposite
    chirality, and m-gt0 extrapolations.
  • ? large systematic errors.

6
1. Introduction
  • This work
  • We achieved 2-flavor lattice QCD simulations with
    exact chiral symmetry.
  • The Ginsparg-Wilson relation -gt exact chiral
    symmetry.
  • Lueschers admissibility condition -gt smooth
    gauge fields.
  • On (1.8fm)4 lattice, achieved m3MeV !
  • Finite V effects evaluated by ChRMT.
  • m, V, Q dependences of QCD Dirac spectrum are
    calculated.
  • A good agreement of Dirac spectrum with ChRMT.
  • Strong evidence of chiral SSB from 1st principle.
  • obtained

7
Contents
  1. Introduction
  2. QCD Dirac spectrum ChRMT
  3. Lattice QCD with exact chiral symmetry
  4. Numerical results
  5. Conclusion

8
2. QCD Dirac spectrum ChRMT
  • Banks-Casher relation
  • In the free theory,
  • ?(?) is given by the surface of S3 with the
    radius ?
  • With the strong coupling
  • The eigenvalues feel the repulsive force
    from each other?becoming non-degenerate? flowing
    to the low-density region around zero? results in
    the chiral condensate.

Banks Casher 1980
9
2. QCD Dirac spectrum ChRMT
  • Chiral Random Matrix Theory (ChRMT)
  • Consider the QCD partition function at a
    fixed topology Q,
  • High modes (? gtgt ?QCD) -gt weak coupling
  • Low modes (?ltlt ?QCD) -gt strong coupling
  • ? Let us make an assumption For low-lying
    modes,
  • with an unknown action V(?) ?
    ChRMT.

10
2. QCD Dirac spectrum ChRMT
  • Chiral Random Matrix Theory (ChRMT)
  • Namely, we consider the partition function
    (for low-modes)
  • Universality of RMT Akemann et al. 1997
  • IF V(?) is in a certain universality class, in
    large n limit (n size of matrices) the low-mode
    spectrum is proven to be equivalent, or
    independent of the details of V(?) (up to a
    scale factor) !
  • From the symmetry, QCD should be in the same
    universality class with the chiral unitary
    gaussian ensemble,
  • and share the same
    spectrum, up to a overall

11
2. QCD Dirac spectrum ChRMT
  • Chiral Random Matrix Theory (ChRMT)
  • In fact, one can show that the ChRMT is
    equivalent to the moduli integrals of chiral
    perturbation theory.
  • The second term in the exponential is written as
  • where
  • Let us introduce Nf x Nf real matrix s1 and s2
    as

12
2. QCD Dirac spectrum ChRMT
  • Chiral Random Matrix Theory (ChRMT)
  • Then the partition function becomes
  • where is a NfxNf complex matrix.
  • With large n, the integrals around the suddle
    point, which satisfies
  • leaves the integrals over U(Nf) as
  • equivalent to the ChPT modulis integral
    in the eregime.
  • ?

13
2. QCD Dirac spectrum ChRMT
  • Eigenvalue distribution of ChRMT
  • Damgaard Nishigaki 2001 analytically derived
    the distribution of each eigenvalue of ChRMT.
  • For example, in Nf2 and Q0 case, it is
  • where and
  • where
  • -gt spectral density or correlation can be
    calculated, too.

14
2. QCD Dirac spectrum ChRMT
Note We made a stronger assumption QCD -gt
ChRMT ChPT than usual, QCD
-gt ChPT
  • Summary of QCD Dirac spectrum
  • IF QCD dynamically breaks the chiral symmetry,
  • the Dirac spectrum in finite V should look like

?
Banks-Casher S
Note Analytic solution is not known -gt
lets study lattice QCD!
?
15
3. Lattice QCD with exact chiral symmetry
  • The overlap Dirac operator
  • We use Neubergers overlap Dirac operator
    Neuberger 1998
  • (we take m0a1.6) satisfies the
    Ginsparg-Wilson 1982 relation
  • realizes modified exact chiral symmetry on
    the lattice
  • the action is invariant under
    Luescher 1998
  • However, Hw?0 ( topology boundary ) is
    dangerous.
  • D is theoretically ill-defined. Hernandez et al.
    1998
  • Numerical cost is suddenly enhanced. Fodor et
    al. 2004

16
3. Lattice QCD with exact chiral symmetry
  • Lueschers admissibility condition Luescher
    1999
  • In order to achieve Hw gt 0 Lueschers
    admissibility condition,
  • we add topology stabilizing term Vranas
    2006, HF et al(JLQCD), 2006
  • with µ0.2. Note Stop ?8 when Hw?0 and Stop?0
    when a?0.
  • ( Note
  • is extra Wilson fermion and twisted mass
    bosonic spinor with a cut-off
    scale mass. )
  • With Stop, topological charge , or the index of
    D, is fixed along
  • the hybrid Monte Carlo simulations -gt ChRMT at
    fixed Q.
  • Ergodicity in a fixed topological sector ? -gt
    O.K.
  • (Local fluctuation of topology is consistent
    with ChPT.)
  • JLQCD, in preparation

17
3. Lattice QCD with exact chiral symmetry
  • Sexton-Weingarten method
  • Sexton Weingarten 1992, Hasenbusch, 2001
  • We divide the overlap fermion determinant as
  • with heavy m and performed finer (coarser)
    hybrid Monte Carlo step
  • for the former (latter) determinant -gt factor
    4-5 faster.
  • Other algorithmic efforts
  • Zolotarev expansion of D -gt 10 -(7-8) accuracy.
  • Relaxed conjugate gradient algorithm to invert D.
  • Multishift conjugate gradient for the 1/Hw2.
  • Low-mode projections of Hw.

18
3. Lattice QCD with exact chiral symmetry
  • Numerical cost
  • Simulation of overlap fermion was thought to be
    impossible
  • D_ov is a O(100) degree polynomial of D_wilson.
  • The non-smooth determinant on topology boundaries
    requires extra factor 10 numerical cost.
  • ? The cost of D_ov 1000 times of
    D_wilsons .
  • However,
  • Stop can cut the latter numerical cost 10
    times faster
  • Stop can reduce the degree of polynomial 2-3
    times
  • New supercomputer at KEK 60TFLOPS 50 times
  • Many algorithmic improvements
    5-10 times
  • We can overcome this difficulty !

19
3. Lattice QCD with exact chiral symmetry
  • Simulation summary
  • On a 163 32 lattice with a 1.6-1.9GeV (L
    1.8-2fm), we
  • achieved 2-flavor QCD simulations with the
    overlap quarks with
  • the quark mass down to 3MeV.
    e-regime
  • Note m gt50MeV with Wilson fermions in previous
    JLQCD works.
  • Iwasaki (beta2.3,2.35) Stop(µ0.2) gauge
    action
  • Quark masses ma0.002(3MeV) 0.1.
  • 1 samples per 10 trj of Hybrid Monte Carlo
    algorithm.
  • 5000 trj for each m are performed.
  • Q0 topological sector (No topology change.)
  • The lattice spacings a is calculated from quark
    potential(consistent with rho meson mass input).
  • Eigenvalues are calculated by Lanzcos algorithm.
  • (and projected to imaginary axis.)

20
4. Numerical results
  • In the following, we mainly focus on the data
    with m3MeV.
  • Bulk spectrum
  • Almost consistent with the Banks-Cashers
    scenario !
  • Low-modes
  • accumulation.
  • The height
  • suggests
  • S (240MeV)3.
  • gap from 0.
  • ? need ChRMT analysis
  • for the precise
  • measurement of S !

21
4. Numerical results
  • Low-mode spectrum
  • Lowest eigenvalues qualitatively agree with
    ChRMT.

22
4. Numerical results
  • Low-mode spectrum
  • Cumulative histogram
  • is useful to compare the shape of the
    distribution.
  • The width agrees with RMT within 2s.

23
4. Numerical results
  • Heavier quark masses
  • For heavier quark masses, 30160MeV, the
    good agreement
  • with RMT is not expected, due to finite m effects
  • of non-zero modes.
  • But our data of the ratio of the eigenvalues
    still show a qualitative
  • agreement.
  • NOTE
  • massless Nf2 Q0 gives
  • the same spectrum with
  • Nf0, Q2. (flavor-topology
  • duality)
  • m -gt large limit is
  • consistent with QChRMT.

24
4. Numerical results
  • Heavier quark masses
  • However, the value of S, determined by the
    lowest-eigenvalue,
  • significantly depend on the quark mass.
  • But, the chiral limit is still consistent with
    the data with 3MeV.

25
4. Numerical results
  • Renormalization
  • Since S240(2)(6)3 is the lattice bare
    value, it should be
  • renormalized.
  • We calculated
  • the renormalization factor in a non-perturbative
    RI/MOM scheme on the lattice,
  • match with MS bar scheme, with the perturbation
    theory,
  • and obtained

(non-perturbative)
(tree)
26
4. Numerical results
  • Systematic errors
  • finite m -gt small.
  • As seen in the chiral extrapolation
  • of S, m3MeV is very close to
  • the chiral limit.
  • finite lattice spacing a -gt O(a2) -gt (probably)
    small.
  • the observables with overlap Dirac operator are
    automatically free from O(a) error,
  • NLO finite V effects -gt 5-10.
  • Higher eigenvalue feel pressure from bulk modes.
  • higher k data are smaller than RMT. (5-10)
  • 1-loop ChPT calculation also suggests 10 .

systematic
statistical
27
5. Conclusion
  • We achieved lattice QCD simulations with
  • exactly chiral symmetric Dirac operator,
  • On (2fm)4 lattice, simulated Nf2 dynamical
    quarks with m3MeV,
  • found a good consistency with Banks-Cashers
    scenario,
  • compared with ChRMT where finite V and m effects
    are taken into account,
  • found a good agreement with ChRMT,
  • Strong evidence of chiral SSB from 1st principle.
  • obtained

28
5. Conclusion
  • Future works
  • Reduce the NLO V effects (or 1/N effects) of S.
  • Larger lattices (prepared).
  • NLO calculations of meson correlators in
    (partially quenched) ChPT. analytic part is
    done.
  • P.H.Damgaard HF, arXiv0707.3740
  • Hadron spectrum
  • Test of ChPT (chiral log)
  • Pion form factor
  • pp0 difference
  • BK
  • Topological susceptibility
  • 21 flavor simulations
  • Finer and larger lattices

29
6. NLO V effects (preliminary)
  • Meson correlators compared with ChPT
  • With a direct comparison of meson correlators
    with
  • (partially quenched) ChPT, we obtain
  • P.H.Damgaard HF, arXiv0707.3740
  • where NLO V correction is taken into account.
  • JLQCD, in preparation.

30
6. NLO V effects (preliminary)
  • Meson correlators compared with ChPT
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