The EOSs and the Blatant Discrepancy in Modelling Massive Neutron Stars: Origin and a Possible Solution Method

ISSN Print: 2153-1196
ISSN Online: 2153-120X
www.scirp.net/journal/jmp
E-mail: [email protected]

Citations

"The EOSs and the Blatant Discrepancy in Modelling Massive Neutron Stars: Origin and a Possible Solution Method"
written by Ahmad A. Hujeirat, Mauritz M. Wicker,
published by Journal of Modern Physics, Vol.14 No.11, 2023

has been cited by the following article(s):

[1]	Why the Central Monster in M87 Should Be a Massive DEO Rather than a SMBH?
	Journal of Modern Physics, 2024

[1]	Phenomenological Model for the Maximum Mass of a Rotating Magnetized Neutron Star Research in Astronomy and Astrophysics, 2026 DOI:10.1088/1674-4527/ae21c8

[2]	Axion Gamma-Ray Signatures from Quark Matter in Neutron Stars and Gravitational Wave Comparisons Journal of Modern Physics, 2025 DOI:10.4236/jmp.2025.161007

[3]	Why the Central Monster in M87 Should Be a Massive DEO Rather than a SMBH? Journal of Modern Physics, 2024 DOI:10.4236/jmp.2024.155026