Emission of gravitational radiation in scalar-tensor and f(R)-theories

  1. Laurentis, Mariafelicia De 2
  2. Martino, Ivan De 1
  1. 1 Universidad de Salamanca, Departamento de Física Fundamental, Salamanca, Spain
  2. 2 Dipartimento di Fisica, Università di Napoli “Federico II”, Compl. Univ. di Monte S. Angelo, Napoli, Italy
Libro:
Handbook of Gravitational Wave Astronomy

ISBN: 9789811547027

Año de publicación: 2021

Páginas: 1-38

Tipo: Capítulo de Libro

DOI: 10.1007/978-981-15-4702-7_40-1 GOOGLE SCHOLAR

Resumen

The recent detections of gravitational waves by the advanced LIGO and Virgo detectors open a formidable way to set constraints on alternative metric theories of gravity in the strong field regime. Such tests rely sensitively on the phase evolution of the gravitational waves, which is controlled by the energy momentum carried by such waves out of the system. The weak-field limit of alternative metric theories shows new aspects of gravitation which are not present in general relativity and exhibits new gravitational field modes which can easily be interpreted as massive gravitons. The study of the generation, propagation, and detection of gravitational waves in the weak-field limit of a given relativistic theory of gravity is an important part of astrophysics.

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