English

Holographic bottomonium formation in a cooling strong-interaction medium at finite baryon density

High Energy Physics - Theory 2021-11-24 v1

Abstract

The shrinking of the bottomonium spectral function towards narrow quasi-particle states in a cooling strong-interaction medium at finite baryon density is followed within a holographic bottom-up model. The 5-dimensional Einstein-dilaton-Maxwell background is adjusted to lattice-QCD results of sound velocity and susceptibilities. The zero-temperature bottomonium spectral function is adjusted to experimental Υ\Upsilon ground-state mass and first radial excitations. At baryo-chemical potential μB=0\mu_B = 0, these two pillars let emerge the narrow quasi-particle state of the Υ\Upsilon ground state at a temperature of about 150 MeV. Excited states are consecutively formed at lower temperatures by about 10 (20) MeV for the 2S2S (3S3S) vector states. The baryon density, i.e. μB>0\mu_B > 0, pulls that formation pattern to lower temperatures. At μB=\mu_B = 200 MeV, we find a shift by about 15 MeV.

Keywords

Cite

@article{arxiv.2109.05824,
  title  = {Holographic bottomonium formation in a cooling strong-interaction medium at finite baryon density},
  author = {Rico Zöllner and Burkhard Kämpfer},
  journal= {arXiv preprint arXiv:2109.05824},
  year   = {2021}
}