Does Our Universe Conform with the Existence of a Universal Maximum Energy-Density <i>p<sub>max</sub><sup style="margin-left:-30px;">uni</sup></i> — Oak Academic Publishing
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Does Our Universe Conform with the Existence of a Universal Maximum Energy-Density <i>p<sub>max</sub><sup style="margin-left:-30px;">uni</sup></i>
Recent astronomical observations of high redshift quasars, dark matter-dominated galaxies, mergers of neutron stars, glitch phenomena in pulsars, cosmic microwave background and experimental data from hadronic colliders do not rule out, but they even support the hypothesis that the energy-density in our universe most likely is upper-limited by p max uni which is predicted to lie between 2 to 3 the nuclear density p 0 . Quantum fluids in the cores of massive NSs with p ≈ p max uni e a ch the maximum compressibility state, where they become insensitive to further compression by the embedding spacetime and undergo a phase transition into the purely incompressible gluon-quark superfluid state. A direct correspondence between the positive energy stored in the embedding spacetime and the degree of compressibility and superfluidity of the trapped matter is proposed. In this paper relevant observational signatures that support the maximum density hypothesis are reviewed, a possible origin of p max uni i s pr oposed and finally the consequences of this scenario on the spacetime’s topology of the universe as well as on the mechanisms underlying the growth rate and power of the high redshift QSOs are discussed.
KeywordsGeneral Relativity: Neutron StarsIncompressible SuperfluidsQuantum ChromodynamicsCosmology: Big Bang PhysicsDark Matter and Dark EnergyQuasarsFirst Generation of Stars
Abbott, et al. (2017) The Astrophysical Journal Letters, 848, L12.
Falcke, H., Laing, R., Testi, L. and Zensus, A. (2012) ESO Headquarters Astronomical News.
Nicholl, M., Margalit, B., Schmidt, P., et al. (2021) Tight Multi-Messenger Constraints on the Neutron Star Equation of State from GW170817 and a Forward Model for Kilonova Light Curve Synthesis.
Psaltis, D., et al. (2020) Physical Review Letters, 125, Article ID: 141104.
Yang, J., Wang, F., Fan, X., et al. (2020) Pōniuā’ena: A Luminous z = 7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole.
Pasechnik, R. and Sumbera, M. (2017) Universe, 3, 7. https://doi.org/10.3390/universe3010007
Shuryak, E.V. (2004) What RHIC Experiments and Theory Tell Us about Properties of Quark-Gluon Plasma?
Hujeirat, A.A. and Samtaney, R. (2020) Journal of Modern Physics, 11, 1779-1784. https://doi.org/10.4236/jmp.2020.1111110
Fan, X., Wang, F., Yang, J., et al. (2019) The Astrophysical Journal Letters, 870, L11. https://doi.org/10.3847/2041-8213/aaeffe
Oesch, P.A., et al. (2016) The Astrophysical Journal, 819, 129.
Shimasaku, K. and Izumi, T. (2019) The Astrophysical Journal Letters, 872, L29. https://doi.org/10.3847/2041-8213/ab053f
Smith, A., Bromm, V. and Abraham Loeb, A. (2017) The First Supermassive Black Holes.
Carr, B.J., Kohri, K., Sendouda, Y. and Yokoyama, J. (2010) New Cosmological Constraints on Primordial Black Holes.
Hujeirat, A.A. (2018) Journal of Modern Physics, 9, 532-553. https://doi.org/10.4236/jmp.2018.94037
Hujeirat, A.A. and Samtaney, R. (2020) Journal of Modern Physics, 11, 1779-1784. https://doi.org/10.4236/jmp.2020.1111110
Hujeirat, A.A. and Samtaney, R. (2020) Journal of Modern Physics, 11, 1785-1798. https://doi.org/10.4236/jmp.2020.1111111
Ashton, G., Lasky, P.D., Graber, V. and Palfreyman, J. (2019) Rotational Evolution of the Vela Pulsar during the 2016 Glitch.
Bogdan, A. (2020) The Archetypal Ultra-Diffuse Galaxy, Dragonfly 44, Is Not a Dark Milky Way.
Argueelles, C.R., Dieaz, M.I., Krut, A., et al. (2021) Monthly Notices of the Royal Astronomical Society, 502, 4227-4246. https://doi.org/10.1093/mnras/staa3986
Gustafsson, B., Ross, P. and Church, M.B.D. (2016) AandA, 593, A85. https://doi.org/10.1051/0004-6361/201423916
Barkana, R. (2018) Nature, 555, 71-74. https://doi.org/10.1038/nature25791
Arbey, A., Ellis, J., Mahmoudi, F. and Robbins, G. (2018) Journal of High Energy Physics, 2018, Article No. 132. https://doi.org/10.1007/JHEP10(2018)132
Sivakumer, A., Muruganandam, P. and Hujeirat, A.A. (2021) On the Merger of Superfluid Cores of Neutron Stars the Nature of the Remnant of GW170817. (In Preparation)
Roy, J., Yashwant Gupta, Y. and Lewandowski, W. (2012) Monthly Notices of the Royal Astronomical Society, 424, 2213-2221. https://doi.org/10.1111/j.1365-2966.2012.21380.x
Espinoza, C.M., Lyne, A.G., Stappers, B.W. and Kramer, C. (2011) Monthly Notices of the Royal Astronomical Society, 414, 1679-1704. https://doi.org/10.1111/j.1365-2966.2011.18503.x
Ashton, G., Prix, R. and Jones, D.I. (2017) Physical Review D, 96, Article ID: 063004. https://doi.org/10.1103/PhysRevD.96.063004
Ng, C., Champion, D.J., Bailes, M., et al. (2015) The High Time Resolution Universe Pulsar Survey XII: Galactic Plane Acceleration Search and the Discovery of 60 Pulsars.
Hujeirat, A.A. (2020) Journal of Modern Physics, 11, 1779-1784. https://doi.org/10.4236/jmp.2020.1111110
Bromm, V. (2013) Formation of the First Stars.
Fischer, T., Wu, M.-R., Benjamin Wehmeyer, B., et al. (2021) Core-Collapse Supernova Explosions Driven by the Hadron-Quark Phase Transition as a Rare r-Process Site.
Chon, S., Hosokawa, T., Kazuyuki Omukai, K., et al. (2021) Monthly Notices of the Royal Astronomical Society, 502, 700-713. https://doi.org/10.1093/mnras/stab061
McInnes, B. (2017) Nuclear Physics B, 921, 39-58. https://doi.org/10.1016/j.nuclphysb.2017.05.004
Mueller, B. (2007) From Quark-Gluon Plasma to the Perfect Liquid.
Witten, E. (1981) Communications in Mathematical Physics, 80, 381-402. https://doi.org/10.1007/BF01208277
Karr, J.-P. and Marchand, D. (2019) Nature, 575, 61. https://doi.org/10.1038/d41586-019-03364-z
Bombaci, I. (2016) The Hyperon Puzzle in Neutron Stars.