Parametric instability induced scalar gravitational waves from a model pulsating neutron star

Wang, Charles H.-T. and Bonifacio, Paolo M. and Bingham, Robert and Mendonça, J. Tito (2011) Parametric instability induced scalar gravitational waves from a model pulsating neutron star. Modern Physics Letters B, 705 (1-2). pp. 148-151. ISSN 0217-9849 (https://doi.org/10.1016/j.physletb.2011.09.111)

Abstract

We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.

ORCID iDs

Bingham, Robert ORCID: https://orcid.org/0000-0002-9843-7635

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  Item type:	Article
  ID code:	36053
  Dates:	Date Event 3 November 2011 Published
  Subjects:	Science > Physics
  Department:	Faculty of Science > Physics
  Depositing user:	Pure Administrator
  Date deposited:	22 Nov 2011 14:15
  Last modified:	11 Nov 2024 10:01
  Related URLs:	Scopus publication http://www.sciencedirect.com/science/art...
  URI:	https://strathprints.strath.ac.uk/id/eprint/36053