Preprint PUBDB-2023-03695

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Electromagnetic fields in compact binaries: post-Newtonian wave generation and application to double white dwarfs systems

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2023

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Report No.: DESY-23-074; arXiv:2310.03785

Abstract: The aim of this work is twofold: (i) to properly define a wave-generation formalism for compact-supported sources embedded in Einstein-Maxwell theory, relying on matched post-Newtonian and multipolar-post-Minkowskian expansions; (ii) to apply this formalism (which is valid for any type of post-Newtonian sources) to the case of two stars with constant and aligned magnetic dipoles, by computing the fluxes of energy and angular momentum to the next-to-leading order, as well as the gravitational amplitude modes. Assuming eccentric orbits, we derive the evolution of orbital parameters, as well as the observables of the system, notably the gravitational phase for quasi-circular orbits. Finally, we give some numerical estimates for the contribution of the magnetic dipoles for some realistic systems.

Keyword(s): dipole, magnetic ; higher-order, 1 ; binary, compact ; gravitation ; orbit ; star ; electromagnetic field ; Einstein-Maxwell equation ; angular momentum


Note: 44 pages

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. LHCtoLISA - Precision Gravity: From the LHC to LISA (817791) (817791)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2023
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Creative Commons Attribution CC BY 4.0 ; OpenAccess ; Published
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http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Journal Article  ;  ;
Electromagnetic fields in compact binaries: Post-Newtonian wave generation and application to double white dwarfs systems
Physical review / D 109(8), 084048 () [10.1103/PhysRevD.109.084048]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2023-06-09, last modified 2024-06-09