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Pion decay constant in Dense Skyrmion Matter

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Title: Pion decay constant in Dense Skyrmion Matter


1
Pion decay constant in Dense Skyrmion Matter
Hee-Jung Lee ( Chungbuk Natl Univ.)
Collaborators Byung-Yoon Park (Chungnam Natl
Univ.) Mannque Rho (Saclay) Vicente Vento (Univ.
of Valencia) Dong-Pil Min (Seoul Natl Univ.)
2
Contents
Overview SU(2) Skyrme Model Pion decay
constant in Skyrmion Matter Results
Summary and discussion
3
Overview
Properties of Pion in free space
Properties of Pion in Nuclear Matter
4
1. Chiral Perturbation Theory -
H. Yabu et al, PRD 50 (1994) 3549. -
V. Thorsson et al, NPA 589 (1995) 633.
- T. S. Park et al, PLB 409 (1997) 26.
- U. Meissner et al, Ann.Phys297(2002)27.
Fermi Gas Mean Field Approx.
5
2. Optical Potential Theory - T. Waas et al,
PLB 405 (1997) - T. Yamazaki et al, PLB 418
(1998) S-wave pion- nucleon potential of
the deeply bound states in Pb nucleus
observed at GSI
Pion mass increases - a 7 at the
center Pb nucleus - a 3 in symmetric
nuclear matt.
6
SU(2) Skymion Model Approach
- Baryons are appeared as static solitons of
the Skyrme Lagrangian. - The pion-matter
interactions are generated from the same
Skyrme Lagrangian as classical potentials. -
The results contain higher orders in density.
7
SU(2) Skymion Model
1. The Model Lagrangian
2. Hedgehog Ansatz Single Baryon by topology
Baryon number density
8
3. Skyrmion Matter Skyrmion Crystal - I.
Klevanov, NPB 262(1985) 133 - M. Kugler et
al, PRD 40 (1989) 3421.
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4. Pions in Skyrmion Matter The dynamics
of the pion in dense skyrmion matter. - S.
Saito et al, Prog. Theor. Phys. 75 (1986) 68.
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- Lagrangian
14
Classical potentials
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- The Pion Effective Mass ( )
Pole equation of the Pion Propagator
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- The in medium decay constant ( )
PCAC Relation
19
- Results
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At high den., the Chiral symm. is restored.
Trace (Scale) Anomaly in QCD
Introduce a scalar field into the Skyme theory

21
QCD Trace Anomaly
  • The classical QCD action is scale-invariant in
    the chiral limit under
  • At quantum level, this invariance becomes broken
    even for the chiral limit.
  • The dilatation current is not conserved

22
Modified Skyrme Lagrangian - J. Ellis and
J. Lanik, PLB150 (1985) 289 - G. E. Brown and
M. Rho, PRL 66 (1991) 2720
The scalar field ( ) with unity scale dim. and
the potential energy generate the trace anomaly
in this effective Lagrangian -
Furnstahl, et al, PRC 52 (1995) 1368
23
! If one interpret the scalar field as a pure
glueball, the gluon condensation gives the mass
of the scalar field as
  • 1. Set A R. J. Furnstahl, et al, PRC 52 (1995)
    1368
  • 2. Set B C. Song, et al, PRC 56 (1997) 2244
  • 3. Set C M. S. Shifman, et al, NPB 147 (1979)
    385

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Energy per baryon
Potential Energy for the scalar field
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Energy per single skyrmion as a function of the
scalar field X for a given lattice size with the
parameter sets B.
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Phases of skyrmion matter
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Pions and Scalar in Skyrmion Matter
Fluctuations on top of the static skyrmion
crystal
Lagrangian for pions and the scalar field
Lagrangian for the static background skyrmion
matter
29
Lagrangian for pions on the matter
Lagrangian for the scalar field on the matter
Lagrangian for the interaction between pions
and the scalar field on the matter
30
Pion decay constants
External axial vector current
Axial vector current and vector current of SM
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Pion decay constants
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Pion velocity
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Pion propagator in medium


for massless pion
Pion velocity in medium
38
Pion velocity in medium
H.-J. Lee, B.-Y. Park, M. Rho, V. Vento, Nucl.
Phys. A (2004)
39
Relation between two kinds of constants
For massless pion
40
Summary and ..
  • Phase transition with respect to chiral symmetry
  • happens with density in skyrmion matter.
  • Mass and decay constants of pion decrease
  • with density of skyrmion matter.
  • 3. Velocity of pion decreases to minimum and
  • returns the value in free space when chiral
    sym.
  • is restored.
  • 4. Relation in two kinds of constants for
    massive pion?
  • This approach would be too simple to be a
  • real physical situation.
  • need to quantize skyrmions in skyrmion
    matter.
  • 6. Heating skyrmion matter, what happens?

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