activity
20242026
most citedIndirect forces in disc-planet interaction

2 citations · 3 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2026

Debris Disc Substructures Induced by Secular Planetary Perturbations

Roman R. Rafikov, Deniz Akansoy, Antranik A. Sefilian

Observations of debris discs have the potential to provide us with valuable information about massive planets perturbing them gravitationally. In this work, we explore the evolutio…

astro-ph.EP2026

-mapping of planet-induced density wave damping in protoplanetary discs

Amelia J. Cordwell, Roman R. Rafikov

Planets embedded in protoplanetary discs are capable of creating a wide variety of substructures through gravitational interactions. This process is mediated through the excitation…

astro-ph.EP20262 cited

Indirect forces in disc-planet interaction

Roman R. Rafikov, Nicolas P. Cimerman, Callum W. Fairbairn +1

Gravitational coupling between a protoplanetary disc and an embedded planet is often studied in a frame attached to a central star. This frame is non-inertial because of the stella…

astro-ph.EP20261 cited

Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem

Roman R. Rafikov

The dynamics of systems of multiple gravitationally interacting bodies is often studied in a frame attached to one of the objects (e.g. a central star in a planetary system). As th…

astro-ph.EP2025

How two-dimensional are planet-disc interactions? II. Radiation hydrodynamics and suitable cooling prescriptions

Alexandros Ziampras, Amelia J. Cordwell, Roman R. Rafikov +1

The ring and gap structures found in observed protoplanetary disks are often attributed to embedded gap-opening planets and typically modeled with simplified thermodynamics in the…

astro-ph.HE2025

Wave-Mediated Boundary Layers of Accretion Discs: Role of Internal Structure of the Accretor

Samuel G. D. Turner, Roman R. Rafikov, Alexander A. Philippov

Disc accretion onto astrophysical objects with a material surface proceeds through the boundary layer (BL) -- a radially narrow region in the inner disc where the incoming gas must…