English

Thermodynamics of absolute stiff matter

Cosmology and Nongalactic Astrophysics 2011-10-06 v5 Solar and Stellar Astrophysics Statistical Mechanics High Energy Physics - Phenomenology

Abstract

The 'absolute stiff' matter (P=EP=E) can be a Fermi or Bose gas of particles with the energy spectrum ϵppq\epsilon_p \sim p^q in qq-dimensional space, particularly ϵp=p3/m2\epsilon_p =p^3/m^2 in 3-dimensional space. We obtain its pressure, particle number density and heat capacity at finite temperature. The behavior of 'absolute stiff' medium is determined by characteristic temperature Tc=6π2n/(γm2)T_c=6\pi ^2n/(\gamma m^2). At low temperature the heat capacity obeys the linear law CVTC_V\sim T for both fermionic and bosonic matter, the pressure of 'absolute stiff' fermions Pn2+O(T2)P\sim n^2+O(T^2), while the 'absolute stiff' Bose gas never reveals Bose-Einstein condensation.

Keywords

Cite

@article{arxiv.1107.1782,
  title  = {Thermodynamics of absolute stiff matter},
  author = {Ernst Trojan and George V. Vlasov},
  journal= {arXiv preprint arXiv:1107.1782},
  year   = {2011}
}

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14 pages