JMP  Vol.9 No.4 , March 2018
Glitches: The Exact Quantum Signatures of Pulsars Metamorphosis
The observed recurrence of glitches in pulsars and neutron stars carries rich information about the evolution of their internal structures. In this article, I show that the glitch-events observed in pulsars are exact quantum signatures for their metamorphosis into dark super-baryons (SBs), whose interiors are made of purely incompressible superconducting gluon-quark superfluids. Here the quantum nuclear shell model is adopted to describe the permitted energy levels of the SB, which are assumed to be identical to the discrete spinning rates ΩSB that SBs are allowed to rotate with. Accordingly, a glitch-event corresponds to a prompt spin-down of the superconducting SB from one energy level to the next, thereby expelling a certain number of vortices, which in turn spins up the ambient medium. The process is provoked mainly by the negative torque of the ambient dissipative nuclear fluid and by a universal scalar field ∅ at the background of a supranuclear dense matter. As dictated by the Onsager-Feynman equation, the prompt spin-down must be associated with increase of the dimensions of the embryonic SB to finally convert the entire pulsar into SB-Objects on the scale of Gyrs. Based on our calculations, a Vela-like pulsar should display billions of glitches during its lifetime, before it metamorphoses entirely into a maximally compact SB-object and disappears from our observational windows. The present model predicts the mass of SBs and ΔΩ/Ω in young pulsars to be relatively lower than their older counterparts.
Cite this paper
Hujeirat, A. (2018) Glitches: The Exact Quantum Signatures of Pulsars Metamorphosis. Journal of Modern Physics, 9, 554-572. doi: 10.4236/jmp.2018.94038.
[1]   Haensel, P., Potekhin, A.Y. and Yakovlev, D.G. (2007) Neutron Stars 1. Springer, Heidelberg-Berlin.

[2]   Espinoza, C.M., Lyne, A.G., Stappers, B.W. and Kramer, C. (2011) MNRAS, 414, 1679-1704.

[3]   Eya, I.O. and Urama, J.O. (2014) International Journal of Astrophysics and Space Science, 2, 16-21.

[4]   Baym, G. and Chin, S.A. (1976) Physics Letters B, 62, 241-244.

[5]   Chapline, G. and Nauenberg, M. (1977) Physical Review D, 16, 450.

[6]   Hujeirat, A.A. (2017) Cornell University Library. Ithaca, New York.

[7]   LHCb Collaboration (2015) Physical Review Letters, 115, Article ID: 072001.

[8]   Camenzind, M. (2007) Compact Objects in Astrophysics. Springer, Heidelberg.

[9]   Glendenning, N. (2007) Special and General Relativity. Springer, Berlin.

[10]   Hujeirat, A.A. and Thielemann, F-K. (2009) MNRAS, 400, 903-916.

[11]   Yarmchuk, E.J., Gordon, M.J.V. and Packard, R.E. (1979) Physical Review Letters, 43, 214.

[12]   Haensel, P., Lasota, J.P. and Zdunik, J.L. (1999) A&A, 344, 151.

[13]   Bethke, S. (2007) Progress in Particle and Nuclear Physics, 351, 58.

[14]   Cook, G.B., Shapiro, S.L. and Teukolsky, S.A. (1994) APJ Letters, 423, L117.

[15]   Baggaley, A.W. and Laurie, J. (2014) Physical Review B, 89, Article ID: 014504.

[16]   Witten, E. (1984) Physical Review D, 30, 272-285.

[17]   Hujeirat, A.A. (2018) Journal of Modern Physics, 9, 51-69.

[18]   Hujeirat, A.A. (2018) Journal of Modern Physics, 9, 70-83.

[19]   Hujeirat, A.A. (2012) MNRAS, 423, 2893.