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[1]
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Phenomenological Model for the Maximum Mass of a Rotating Magnetized Neutron Star
Research in Astronomy and Astrophysics,
2026
DOI:10.1088/1674-4527/ae21c8
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[2]
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Evidence for False Vacuum States inside the Cores of Massive Pulsars and the Ramification on the Measurements of Their True Masses
Journal of Modern Physics,
2023
DOI:10.4236/jmp.2023.1411081
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[3]
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The EOSs and the Blatant Discrepancy in Modelling Massive Neutron Stars: Origin and a Possible Solution Method
Journal of Modern Physics,
2023
DOI:10.4236/jmp.2023.1411085
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[4]
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Why the Spacetime Embedding Incompressible Cores of Pulsars Must Be Conformally Flat?
Journal of Modern Physics,
2020
DOI:10.4236/jmp.2020.1111110
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[5]
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The Remnant of GW170817: A Trapped Neutron Star with a Massive Incompressible Superfluid Core
Journal of Modern Physics,
2020
DOI:10.4236/jmp.2020.1111111
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[6]
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How Massive Are the Superfluid Cores in the Crab and Vela Pulsars and Why Their Glitch-Events Are Accompanied with under and Overshootings?
Journal of Modern Physics,
2020
DOI:10.4236/jmp.2020.113025
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[7]
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Glitching Pulsars: Unraveling the Interactions of General Relativistic and Quantum Fields in the Strong Field Regimes
Journal of Modern Physics,
2019
DOI:10.4236/jmp.2019.1014111
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[8]
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Evidence of Pulsars Metamorphism and Their Connection to Stellar Black Holes
Journal of Modern Physics,
2018
DOI:10.4236/jmp.2018.94037
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[9]
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Glitches: The Exact Quantum Signatures of Pulsars Metamorphosis
Journal of Modern Physics,
2018
DOI:10.4236/jmp.2018.94038
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