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FIAS Scientific Report 2011 - Frankfurt Institute for Advanced Studies ...

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Trace anomaly and the vector coupling in dense matter<br />

Collaborators: C. Sasaki 1 , H.K. Lee 2 , W.-G. Paeng 2 , M. Rho 2,3<br />

1 <strong>Frankfurt</strong> <strong>Institute</strong> <strong>for</strong> <strong>Advanced</strong> <strong>Studies</strong>, 2 Department of Physics, Hanyang University, Seoul, Korea 3 Institut de<br />

Physique Théorique, CEA Saclay, Gif-sur-Yvette cédex, France<br />

In nuclear physics, a scalar meson plays an essential role as known from Walecka model that works fairly well<br />

<strong>for</strong> phenomena near nuclear matter density. On the other hand, at high density, the relevant Lagrangian that has<br />

correct symmetry is the linear sigma model, and the scalar needed there is the fourth component of the chiral<br />

four-vector (�π,σ). Thus in order to probe highly hot/dense matter, we have to figure out how the chiral scalar<br />

at low temperature/density transmutes to the fourth component of the four-vector.<br />

In this work we have presented how an effective theory near chiral symmetry restoration emerges from the<br />

dilaton-implemented HLS Lagrangian as illustrated in Fig. 1, and discussed its phenomenological implications<br />

at high baryon density. The soft dilaton is responsible <strong>for</strong> the spontaneous breaking of the scale symmetry and<br />

its condensate vanishes when the chiral symmetry is restored. In fact, topological stability of the half-skyrmion<br />

phase has been observed. This is a strong indication that the configuration is robust and it could be associated<br />

with the scale symmetry restoration at high density in continuum theories.<br />

Our main observation on the suppressed repulsive interaction is a common feature in the two different assignments,<br />

“naive” and mirror, of chirality. The nucleon mass near chiral symmetry restoration exhibits a striking<br />

difference in the two scenarios. How the suppression of the repulsion at the dilaton limit – which seems to be<br />

universal independent of the assignments but may manifest itself differently in the two cases – will affect the<br />

EoS <strong>for</strong> compact stars is an interesting question to investigate.<br />

π<br />

1<br />

σ<br />

π<br />

P<br />

2<br />

Q<br />

π<br />

3<br />

dilaton limit chiral restoration<br />

T or<br />

NLSM<br />

ms >> mpi<br />

LSM<br />

ms > mpi ms = mpi<br />

Figure 1: (Left) A chiral sphere in (�π,σ) space. P on the sphere is mapped to another point Q via chiral trans<strong>for</strong>mations.<br />

(Right) Expected changeover of effective theories near chiral symmetry restoration.<br />

Related publications in <strong>2011</strong>:<br />

1) C. Sasaki, H. K. Lee, W. -G. Paeng and M. Rho, Con<strong>for</strong>mal anomaly and the vector coupling in dense<br />

matter, Phys. Rev. D84, 034011 (<strong>2011</strong>), arXiv:1103.0184 [hep-ph].<br />

2) W. -G. Paeng, H. K. Lee, M. Rho and C. Sasaki, Dilaton-limit fixed point in hidden local symmetric parity<br />

doublet model, arXiv:1109.5431 [hep-ph], submitted to Physical Review D.<br />

45<br />

ρ

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