Glitches: The Exact Quantum Signatures of Pulsars Metamorphosis

• 作者: Ahmad A. Hujeirat
• 来源期刊: 现代物理(英文)
• 学科: 医学
• 关键词: RELATIVITY General Black Hole Physics PULSARS Neutron Stars SUPERFLUIDITY QCD DARK Energy DARK Matter
• 年，卷（期）: 2018,（4）
• 页码范围: 554-572
• 页数: 19页
• 分类号: R73

摘要

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/Ωin young pulsars to be relatively lower than their older counterparts.