activity
20242026
collaborators

10 papers

math-ph2026

Existence of nonrelativistic - and multi--boson stars and their radial stability

Emmanuel Chávez Nambo, Olivier Sarbach

Using direct methods of the calculus of variations we establish the existence of an infinite class of spherically-symmetric solutions to the multi-field Schrödinger-Poisson system…

gr-qc2026

Linear stability of nonrelativistic Proca stars

Emmanuel Chávez Nambo, Galo Diaz-Andrade, Alberto Diez-Tejedor +3

We study the linear stability of nonrelativistic Proca stars under generic perturbations. Using a combination of analytic and numerical methods, we demonstrate that, as expected, t…

gr-qc2026

Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number

Miguel Alcubierre, Juan Barranco, Argelia Bernal +5

We present new spherically symmetric solutions of the Einstein-Klein-Gordon equations in a quasi-stationary approximation that describe self-gravitating scalar field configurations…

gr-qc2026

Bondi-type accretion onto a Kerr black hole in the kinetic regime

Patryk Mach, Mehrab Momennia, Olivier Sarbach

We derive an exact solution representing a Bondi-type stationary accretion of a kinetic (Vlasov) gas onto the Kerr black hole. The solution is exact in the sense that relevant phys…

gr-qc2026

Accretion of a Vlasov gas by a Kerr black hole

Patryk Mach, Mehrab Momennia, Olivier Sarbach

We investigate the accretion of a collisionless, relativistic kinetic gas by a rotating Kerr black hole, assuming that at infinity the state of the gas is described by a distributi…

physics.gen-ph2026

Cosmological evolution of collisionless relativistic gases as dark matter

Francisco X. Linares Cedeño, Ulises Nucamendi, Olivier Sarbach

We study a phenomenological dark matter model described as a collisionless relativistic kinetic gas in a spatially flat Friedmann-Lemaître-Robertson-Walker universe. After normali…