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Does entropic gravity bound the masses of the photon and graviton?...symmetry.Stronger bounds emerge from consideration of ultradense matter such as neutronstars, yielding limits of $m \geq 10^{-48}-10^{-50}~$kg, barely within theexperimental photon range and outside that of the graviton....
général - core.ac.uk - PDF: arxiv.org
“day 1 ” physics at rhic: predictions from rqmd... Here I focus on the question whether hadronic observables are sensitive to the Equation of State (EOS) in the ultradense matter....
Ultra-dense neutron star matter, strange quark stars, and the nuclear equation of state... This article gives a brief overview of the phases of ultradense matter predicted to exist deep inside neutron stars and discusses the equation of state (EoS) associated with such matter....
General relativistic effects on the evolution of binary systems.... We show that this relativistic effect can be indeed observable if the neutron star is fast and magnetized enough and that, if observed, it will help to put tight constraints to the equation of state of ultradense matter....
Strobe-x: x-ray timing and spectroscopy on dynamical timescales from microseconds to yearsThe Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) probes strong gravity for stellar mass to supermassive black holes and ultradense matter with unprecedented effective area, high time-resolution, and good spectral resolution, while providing a powerful time-domain X-ray observatory....
 PDF: doaj.org

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