Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Concept of Gravito-Rotational Acceleration and its Consequences for Compact Stellar Objects

Version 1 : Received: 4 April 2021 / Approved: 6 April 2021 / Online: 6 April 2021 (10:08:23 CEST)
Version 2 : Received: 8 April 2021 / Approved: 9 April 2021 / Online: 9 April 2021 (13:28:53 CEST)

How to cite: Hassani, M. Concept of Gravito-Rotational Acceleration and its Consequences for Compact Stellar Objects. Preprints 2021, 2021040163 (doi: 10.20944/preprints202104.0163.v1). Hassani, M. Concept of Gravito-Rotational Acceleration and its Consequences for Compact Stellar Objects. Preprints 2021, 2021040163 (doi: 10.20944/preprints202104.0163.v1).

Abstract

In a previous series of papers relating to the Combined Gravitational Action (CGA), we have exclusively studied orbital motion without spin. In the present paper, we apply CGA to any self-rotating material body, i.e., an axially spinning massive object, which itself may be locally seen as a gravito-rotational source because it is capable of generating the gravito-rotational acceleration, which seems to be unknown to previously existing theories of gravity. The consequences of such an acceleration are very interesting, particularly for Compact Stellar Objects. Independently of the equation of state, it is found that the critical and maximum internal magnetic field strength of a stable neutron star cannot exceed the value of 3x1018G.

Subject Areas

CGA; gravito-rotational acceleration; gravito-rotational energy; neutron stars; pulsars

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