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Gravitational waves and neutron star oscillations


The goal of this SPRINT collaboration is to investigate the production, impact and dectability of gravitational waves from neutron star oscillations. The proposed collaboration will complement well the FAPESP Regular Research Award "Relativistic Astrophysics and Gravitational Waves) (process number 2015/20433-4) of UFABC PI Chirenti, and the dynamics and gravitational wave research of UMD PI Miller. Each PI will spend a few weeks per year at the other's instituion during two years of the project, in order further the proposed scientific collaboration. (AU)

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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)
ROSOFSKY, SHAWN G.; GOLD, ROMAN; CHIRENTI, CECILIA; HUERTA, E. A.; MILLER, M. COLEMAN. Probing neutron star structure via f-mode oscillations and damping in dynamical spacetime models. Physical Review D, v. 99, n. 8, . (15/50421-8)
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)
MILLER, M. COLEMAN; CHIRENTI, CECILIA; STROHMAYER, TOD E.. On the Persistence of QPOs during the SGR 1806-20 Giant Flare. ASTROPHYSICAL JOURNAL, v. 871, n. 1, . (15/50421-8)
POSADA, CAMILO; CHIRENTI, CECILIA. On the radial stability of ultra-compact Schwarzschild stars beyond the Buchdahl limit. Classical and Quantum Gravity, v. 36, n. 6, . (15/50421-8)

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