activity
20002026
most citedThe First Data Release of the Sloan Digital Sky Survey

972 citations · 8.4k across the 124 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2023

Orbital evolution of LIGO/Virgo binaries in stellar clusters driven by cluster tides, stellar encounters and general relativity

Alexander Rasskazov, Roman R. Rafikov

Origin of LIGO/Virgo gravitational wave events may involve production of binaries with relativistic components in dense stellar systems - globular or nuclear star clusters - and th…

astro-ph.GA2023

Gravitational torque in circumbinary discs: global radial oscillations

Nicolas P. Cimerman, Roman R. Rafikov

Circumbinary discs (CBDs) arise in many astrophysical settings, including young stellar binaries and supermassive black hole binaries. Their structure is mediated by gravitational…

astro-ph.GA2023

Relativistic phase space diffusion of compact object binaries in stellar clusters and hierarchical triples

Chris Hamilton, Roman R. Rafikov

The LIGO/Virgo detections of compact object mergers have posed a challenge for theories of binary evolution and coalescence. One promising avenue for producing mergers dynamically…

astro-ph.GA2021★ 26 cited

Eclipse timing the Milky Way's gravitational potential

Sukanya Chakrabarti, Daniel J. Stevens, Jason Wright +4

We show that a small, but \textit{measurable} shift in the eclipse mid-point time of eclipsing binary (EBs) stars of 0.1 seconds over a decade baseline can be used to direct…

astro-ph.GA2020★ 14 cited

Secular dynamics of binaries in stellar clusters -- III. Doubly-averaged dynamics in the presence of general relativistic precession

Chris Hamilton, Roman R. Rafikov

Secular evolution of binaries driven by an external (tidal) potential is a classic astrophysical problem. Tidal perturbations can arise due to an external point mass, as in the Lid…

astro-ph.GA2020★ 4 cited

Doppler Boosting of the S-stars in the Galactic Center

Roman R. Rafikov

Astrometry and spectroscopy of the S-stars in the Galactic Center provide a unique way to probe the properties of the central supermassive black hole, as well as the post-Newtonian…