Mass of Neutron Star in SdS space-time
Vinayaraj O K, V C Kuriakose
TL;DR
This paper introduces a modified TOV equation that includes the cosmological constant to analyze neutron star structure in SdS space-time, providing insights into the maximum mass limits consistent with accelerated universe expansion.
Contribution
It presents a novel modification of the TOV equation incorporating the cosmological constant for neutron star modeling in SdS space-time.
Findings
Calculated maximum neutron star mass limits in SdS space-time.
Demonstrated the impact of the cosmological constant on neutron star structure.
Aligned neutron star models with recent cosmological observations.
Abstract
In this work we present a modified TOV equation which incorporates the cosmological constant with regard to the recent astronomical observations that the Universe is in a phase of accelerated expansion. Using this modified TOV equation we considered the structure of a neutron star in SdS space-time and calculated maximum mass limit for neutron stars.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Stellar, planetary, and galactic studies