Supermassive DEOs (SMDEOs) are cosmologically evolved objects made of irreducible incompressible supranuclear dense superfluids: The state we consider to govern the matter inside the cores of massive neutron stars. These cores are practically trapped in false vacua, rendering their detection by outside observers impossible. Based on massive parallel computations and theoretical investigations, we show that SMDEOs at the centres of spiral galaxies that are surrounded by massive rotating torii of normal matter may serve as powerful sources for gravitational waves carrying away roughly 1042 erg/s. Due to the extensive cooling by GWs, the SMDEO-Torus systems undergo glitching, through which both rotational and gravitational energies are abruptly ejected into the ambient media, during which the topologies of the embedding spacetimes change from curved into flatter ones, thereby triggering a burst gravitational energy of order 1059 erg. Also, the effects of glitches found to alter the force balance of objects in the Lagrangian-L1 region between the central SMDEO-Torus system and the bulge, enforcing the enclosed objects to develop violent motions, that may explain the origin of the rotational curve irregularities observed in the innermost part of spiral galaxies. Our study shows that the generated GWs at the centres of galaxies, which traverse billions of objects during their outward propagations throughout the entire galaxy, lose energy due to repeatedly squeezing and stretching the objects. Here, we find that these interactions may serve as damping processes that give rise to the formation of collective forces
, that point outward, endowing the objects with the observed flat rotation curves. Our approach predicts a correlation between the baryonic mass and the rotation velocities in galaxies, which is in line with the Tully-Fisher relation. The here-presented self-consistent approach explains nicely the observed rotation curves without invoking dark matter or modifying Newtonian gravitation in the low-field approximation.
References
[1]
Milgrom, M. (2001) MOND: A Pedagogical Review. Acta Physica Polonica B, 32, 3613.
[2]
Peebles, P.J.E. (2017) Growth of the Nonbaryonic Dark Matter Theory. NatureAstronomy, 1, Article No. 0057. https://doi.org/10.1038/s41550-017-0057
[3]
Bertone, G. and Hooper, D. (2018) History of Dark Matter. ReviewsofModernPhysics, 90, Article ID: 045002. https://doi.org/10.1103/revmodphys.90.045002
[4]
Haddad, F. and Haddad, N. (2020) A Black Hole inside Dark Matter and the Rotation Curves of Galaxies. arXiv: 2002.12772.
[5]
De-Chang, D., Glenn, S. and Dejan, S., (2022) Milky Way and M31 Rotation Curves: ΛCDM vs. MOND. Physical Review D, 105, Article ID: 104067.
[6]
Riess, A.G., Casertano, S., Yuan, W., Macri, L.M. and Scolnic, D. (2019) Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond Λcdm. TheAstrophysicalJournal, 876, Article 85. https://doi.org/10.3847/1538-4357/ab1422
[7]
Di Valentino, E., Mena, O., etal. (2021) In the Realm of the Hubble Tension—A Review of Solutions. arXiv: 2103.0118.
[8]
Dainotti, M.G., De Simone, B., Schiavone, T., Montani, G., Rinaldi, E. and Lambiase, G. (2021) On the Hubble Constant Tension in the Sne IA Pantheon Sample. TheAstrophysicalJournal, 912, Article 150. https://doi.org/10.3847/1538-4357/abeb73
[9]
Hujeirat, A.A. (2023) Foundation of the Unicentric Model of the Observable Universe—UNIMOUN. JournalofModernPhysics, 14, 415-431. https://doi.org/10.4236/jmp.2023.144023
[10]
Hujeirat, A. (2023) Hubble Tension versus the Cosmic Evolution of Hubble Parameter in the Unicentric Model of the Observable Universe. JournalofModernPhysics, 14, 183-197. https://doi.org/10.4236/jmp.2023.143013
[11]
Hujeirat, A.A. and Wicker, M. (2024) Why the Central Monster in M87 Should Be a Massive DEO Rather than a SMBH? JournalofModernPhysics, 15, 537-549. https://doi.org/10.4236/jmp.2024.155026
[12]
Einstein, A., (1918) Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften zu Berlin. Deutsche Akademie der Wissenschaften zu Berlin, 154-167.
[13]
Abbott, B.P., Abbott, R., Abbott, T.D., Acernese, F., Ackley, K., Adams, C., etal. (2019) Properties of the Binary Neutron Star Merger Gw170817. PhysicalReviewX, 9, Article ID: 011001. https://doi.org/10.1103/physrevx.9.011001
[14]
Ligo Cooperation (2023) Another Long Hard Look for a Remnant of GW170817. https://www.ligo.org/science/Publication-GW170817PostMergerLong/index.php
[15]
Hujeirat, A.A. (2018) Glitches: The Exact Quantum Signatures of Pulsars Metamorphosis. JournalofModernPhysics, 9, 554-572. https://doi.org/10.4236/jmp.2018.94038
[16]
Hujeirat, A.A. and Samtaney, R. (2020) The Remnant of GW170817: A Trapped Neutron Star with a Massive Incompressible Superfluid Core. JournalofModernPhysics, 11, 1785-1798. https://doi.org/10.4236/jmp.2020.1111111
[17]
Espinoza, C.M., Lyne, A.G., Stappers, B.W. and Kramer, M. (2011) A Study of 315 Glitches in the Rotation of 102 Pulsars. MonthlyNoticesoftheRoyalAstronomicalSociety, 414, 1679-1704. https://doi.org/10.1111/j.1365-2966.2011.18503.x
[18]
Roy, J., Gupta, Y. and Lewandowski, W. (2012) Observations of Four Glitches in the Young Pulsar J1833−1034 and Study of Its Glitch Activity. MonthlyNoticesoftheRoyalAstronomicalSociety, 424, 2213-2221. https://doi.org/10.1111/j.1365-2966.2012.21380.x
[19]
Ashton, G., Lasky, P.D., Graber, V. and Palfreyman, J. (2019) Rotational Evolution of the Vela Pulsar during the 2016 Glitch. NatureAstronomy, 3, 1143-1148. https://doi.org/10.1038/s41550-019-0844-6
[20]
Hujeirat, A.A. and Samtaney, R. (2020) How Massive Are the Superfluid Cores in the Crab and Vela Pulsars and Why Their Glitch-Events Are Accompanied with under and Overshootings? JournalofModernPhysics, 11, 395-406. https://doi.org/10.4236/jmp.2020.113025
[21]
Hujeirat, A.A. and Wicker, M.M. (2023) Evidence for False Vacuum States Inside the Cores of Massive Pulsars and the Ramification on the Measurements of Their True Masses. JournalofModernPhysics, 14, 1409-1425. https://doi.org/10.4236/jmp.2023.1411081
[22]
Shapiro, S.L. and Teukolsky, S.A. (1983). Black Holes, White Dwarfs, and Neutron Stars. Wiley. https://doi.org/10.1002/9783527617661
[23]
Thorne, K. (1995) Gravitational Waves. arXiv: gr-qc/9506086.
[24]
Kenath, A. and Sivaram, C. (2023) Physics of Gravitational Waves. Springer.
[25]
Barausse, E. (2023) The Physics of Gravitational Waves. arXiv: 2303.11713.
[26]
Bishop, N.T., Kakkat, V., Kubeka, A.S., Naidoo, M. and van der Walt, P.J. (2024) The Interaction of Gravitational Waves with Matter. https://arxiv.org/abs/2405.07743
[27]
Baym, G., Pathik, C.J. and Patil, S.P. (2017) Damping of Gravitational Waves by Matter. arXiv: 1707.05192.
[28]
Sofue, Y. (2015) Dark Halos of M31 and the Milky Way. arXiv: astro-ph1504.05368.
[29]
Miyamoto, M. and Nagai, R. (1975) Three-Dimensional Models for the Distribution of Mass in Galaxies. PublicationsoftheAstronomicalSocietyofJapan, 27, 533-543.
[30]
Tully, R.B. and Fisher, J.R. (1977) A New Method of Determining Distances to Galaxies. AstronomyandAstrophysics, 54, 661-673.
[31]
McGaugh, S.S., Schombert, J.M., Bothun, G.D. and de Blok, W.J.G. (2000) The Baryonic Tully-Fisher Relation. TheAstrophysicalJournal, 533, L99-L102. https://doi.org/10.1086/312628
[32]
Witten, E. (1984) Cosmic Separation of Phases. PhysicalReviewD, 30, 272-285. https://doi.org/10.1103/physrevd.30.272
[33]
Haensel, P., Lasota, J.P. and Zdunik, J.L. (1999) On the Minimum Period of Uniformly Rotating Neutron Stars. AstronomyandAstrophysics, 344, 151-153.
[34]
Garcia, M.R., Hextall, R., Baganoff, F.K., Galache, J., Melia, F., Murray, S.S., etal. (2010) X-Ray and radio Variability of M31*, the Andromeda Galaxy Nuclear Supermassive Black hole. TheAstrophysicalJournal, 710, 755-763. https://doi.org/10.1088/0004-637x/710/1/755
[35]
Berczik, P., Spurzem, R., Zhong, S., Wang, L., Nitadori, K., Hamada, T., etal. (2013) Up to 700k GPU Cores, Kepler, and the Exascale Future for Simulations of Star Clusters around Black Holes. In: Kunkel, J.M., Ludwig, T. and Meuer, H.W., Eds., Supercomputin, Springer, 13-25. https://doi.org/10.1007/978-3-642-38750-0_2
[36]
Li, S., Liu, F.K., Berczik, P., Chen, X. and Spurzem, R. (2012) Interaction of Recoiling Supermassive Black Holes with Stars in Galactic Nuclei. TheAstrophysicalJournal, 748, Article 65. https://doi.org/10.1088/0004-637x/748/1/65