We compute gravitational self-force (conservative) corrections to tidal invariants for spinning particles moving along circular orbits in a Schwarzschild spacetime. In particular, we consider the square and the cube of the gravitoelectric quadrupolar tidal tensor and the square of the gravitomagnetic quadrupolar tidal tensor. Our results are accurate to first order in spin and through the 9.5 post-Newtonian order. We also compute the associated electric-type and magnetic-type eigenvalues.

Gravitational self-force corrections to tidal invariants for spinning particles on circular orbits in a Schwarzschild spacetime

Bini Donato;
2018

Abstract

We compute gravitational self-force (conservative) corrections to tidal invariants for spinning particles moving along circular orbits in a Schwarzschild spacetime. In particular, we consider the square and the cube of the gravitoelectric quadrupolar tidal tensor and the square of the gravitomagnetic quadrupolar tidal tensor. Our results are accurate to first order in spin and through the 9.5 post-Newtonian order. We also compute the associated electric-type and magnetic-type eigenvalues.
2018
Istituto Applicazioni del Calcolo ''Mauro Picone''
Inglese
98
8
084021
16
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.98.084021
Sì, ma tipo non specificato
Gravitational Self-Force
Spinning particles
arXiv:1806.03495 [gr-qc]
2
info:eu-repo/semantics/article
262
Bini, Donato; Geralico, Andrea
01 Contributo su Rivista::01.01 Articolo in rivista
none
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/348038
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 5
  • ???jsp.display-item.citation.isi??? 6
social impact