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Massive Neutron Stars and White Dwarfs as Noncommutative Fuzzy Spheres

Kalita, S and Mukhopadhyay, B (2022) Massive Neutron Stars and White Dwarfs as Noncommutative Fuzzy Spheres. In: Universe, 8 (8).

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Official URL: https://doi.org/10.3390/universe8080388

Abstract

Over the last couple of decades, there have been direct and indirect evidences for massive compact objects than their conventional counterparts. A couple of such examples are super-Chandrasekhar white dwarfs and massive neutron stars. The observations of more than a dozen peculiar over-luminous type Ia supernovae predict their origins from super-Chandrasekhar white dwarf progenitors. On the other hand, recent gravitational wave detection and some pulsar observations provide arguments for massive neutron stars, lying in the famous mass-gap between lowest astrophysical black hole and conventional highest neutron star masses. We show that the idea of a squashed fuzzy sphere, which brings in noncommutative geometry, can self-consistently explain either of the massive objects as if they are actually fuzzy or squashed fuzzy spheres. Noncommutative geometry is a branch of quantum gravity. If the above proposal is correct, it will provide observational evidences for noncommutativity.

Item Type: Journal Article
Publication: Universe
Publisher: MDPI
Additional Information: The copyright for this article belongs to the Authors.
Keywords: Chandrasekhar limit; equation of state; neutron star; noncommutative geometry; white dwarf
Department/Centre: Division of Physical & Mathematical Sciences > Physics
Date Deposited: 24 Sep 2022 03:37
Last Modified: 24 Sep 2022 03:37
URI: https://eprints.iisc.ac.in/id/eprint/76659

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