Dynamical behavior of boson stars and dark matter cores

dynamical behavior of boson stars and dark matter cores - arXiv

We study the dynamical response of Newtonian boson stars (NBS) when excited by external matter (stars, planets or black holes) in their vicinities.

We study the dynamical response of Newtonian boson stars (NBS) when excited by external matter (stars, planets or black holes) in their vicinities.

Dynamical behavior of boson stars and dark matter cores - INSPIRE

We study the dynamical response of Newtonian boson stars (NBS) when excited by external matter (stars, planets or black holes) in their vicinities.

dynamical behavior of boson stars and dark matter cores

We study the dynamical response of Newtonian boson stars (NBS) when excited by external matter (stars, planets or black holes) in their vicinities. Our setup ...

Dynamical behavior of boson stars and dark matter cores - LIP Indico

Dynamical behavior of boson stars and dark matter cores. Lorenzo Annulli, PhD@CENTRA, Instituto Superior Técnico. June 25, 2020. 6th IDPASC/LIP PhD Students ...

Dynamical behavior of boson stars and dark matter cores

PDF | Bosonic fields can give rise to self-gravitating structures. These are interesting hypothetical new “dark matter stars” and good descriptions of.

Stirred and shaken: Dynamical behavior of boson stars and dark ...

Mentioning: 16 - Stirred and shaken: Dynamical behavior of boson stars and dark matter cores - Annulli, Lorenzo, Cardoso, Vítor, Vicente, Rodrigo.

dynamical behavior of boson stars and dark matter cores - LIP Indico

Stirred and shaken: dynamical behavior of boson stars and dark matter cores. Thursday, 25 June 2020 10:35 (12 minutes). The nature and properties of dark ...

Stirred and shaken: Dynamical behavior of boson stars ... - Altmetric

Stirred and shaken: Dynamical behavior of boson stars and dark matter cores. Published in. Physics Letters B, December 2020. DOI, 10.1016/j.physletb.2020.135944.

Stirred and shaken: dynamical behavior of boson stars and dark ...

Bosonic fields can give rise to self-gravitating structures. These are interesting hypothetical new "dark matter stars" and good descriptions of dark matter ...

Educast Player: 2020-07-09 Stirred and shaken: dynamical behavior ...

Clip #47920 - 2020-07-09 Stirred and shaken: dynamical behavior of boson stars and dark matter cores - Vertical linkbox.

Dynamical boson stars - PMC - PubMed Central

Scalar field dark matter: nonspherical collapse and late-time behavior. Phys Rev ... stars with dark matter cores. PhD thesis, Lisboa University. arXiv ...

Dynamical Boson Stars

and Guzmán, F.S., “Scalar field dark matter: Nonspherical collapse and late-time behavior”, Phys. ... ant instabilities and Stars with dark matter cores”, ArXiv e ...

Dynamical boson stars - Inspire HEP

Dynamical boson stars. Steven L. Liebling(. Long Island U. and; Perimeter Inst ... Stirred and shaken: Dynamical behavior of boson stars and dark matter cores.

New insights into the formation and growth of boson stars in dark ...

Dynamical boson star formation in this case has not been studied using non-linear numerical methods. One example is for. QCD axions, where the ...

arXiv:2007.03700v2 [astro-ph.HE] 8 Nov 2020

Stirred and shaken: dynamical behavior of boson stars and dark matter cores. Lorenzo Annulli, Vitor Cardoso, Rodrigo Vicente. 1 Centro de ...

Dynamical boson stars - OUCI

... dynamical behavior of boson stars and dark matter cores. Phys Lett B 811:135944. https://doi.org/10.1016/j.physletb.2020.135944. arXiv:2007.03700 [astro-ph ...

Bosonic dark matter dynamics in hybrid neutron stars

... dark matter anisotropy, reveals a unique low-density core halo profile, distinguishing it from alternative approaches. Insights gleaned from ...

Boson stars - ScienceDirect.com

... dark matter. If so, scalar particles may be found in the Universe as diffuse gas clouds, as compact objects-boson stars-or mixed up with baryonic matter and ...

Dynamical Boson Stars - PMC - NCBI

Instead, if constructed larger than a galaxy, could a boson star serve as the dark matter halo that explains the flat rotation curve observed for most galaxies?