Advanced search
Start date
Betweenand

Relativistic Astrophysics and Gravitational Waves

Abstract

This project focuses on the study of compact objects, such as black holes and neutron stars, by using their emitted gravitational waves in a number of different configurations. The theoretical study of gravitational waves, described as time-evolving small perturbations in a background spacetime, can provide relevant information on their sources. Cosmological models, equations of state describing the interior of a neutron star and the possible dynamics of binary systems can be compared and clarified by this analysis. The proposed research lines are already ongoing work. (AU)

Articles published in Agência FAPESP Newsletter about the research grant:
Articles published in other media outlets (0 total):
More itemsLess items
VEICULO: TITULO (DATA)
VEICULO: TITULO (DATA)

Scientific publications (4)
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
CHIRENTI, CECILIA; GOLD, ROMAN; MILLER, M. COLEMAN. Gravitational Waves from F-modes Excited by the Inspiral of Highly Eccentric Neutron Star Binaries. ASTROPHYSICAL JOURNAL, v. 837, n. 1, . (15/50421-8, 15/20433-4)
DE SOUZA, GIBRAN H.; CHIRENTI, CECILIA. Torsional oscillations of magnetized neutron stars with mixed poloidal-toroidal fields. Physical Review D, v. 100, n. 4, . (15/20433-4)
CHIRENTI, CECILIA; JASIULEK, MICHAEL. M/R estimates for two neutron stars in LMXBs with possible r-mode frequencies detected. Monthly Notices of the Royal Astronomical Society, v. 476, n. 1, p. 354-358, . (15/20433-4)
CHIRENTI, CECILIA; REZZOLLA, LUCIANO. Did GW150914 produce a rotating gravastar?. Physical Review D, v. 94, n. 8, . (15/20433-4)

Please report errors in scientific publications list by writing to: cdi@fapesp.br.