Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Victor H Robles"'
Autor:
Dhruba Dutta Chowdhury, Frank C. van den Bosch, Pieter van Dokkum, Victor H. Robles, Hsi-Yu Schive, Tzihong Chiueh
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 2, p 68 (2023)
Fuzzy dark matter (FDM), consisting of ultralight bosons, is an intriguing alternative to cold dark matter. Numerical simulations solving the Schrödinger–Poisson (SP) equation, which governs FDM dynamics, show that FDM halos consist of a central s
Externí odkaz:
https://doaj.org/article/548cdf8570ab4bd094dcf8e7c78d8c15
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:2418-2435
We explore the properties of Milky Way subhalos in self-interacting dark matter models for moderate cross sections of 1 to 5 cm$^2$g$^{-1}$ using high-resolution zoom-in N-body simulations. We include the gravitational potential of a baryonic disk an
Autor:
Philip Mocz, Anastasia Fialkov, Mark Vogelsberger, Michael Boylan-Kolchin, Pierre-Henri Chavanis, Mustafa A Amin, Sownak Bose, Tibor Dome, Lars Hernquist, Lachlan Lancaster, Matthew Notis, Connor Painter, Victor H Robles, Jesús Zavala
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023, Vol.521(2), pp.2608-2615 [Peer Reviewed Journal]
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2023, 521 (2), pp.2608-2615. ⟨10.1093/mnras/stad694⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2023, 521 (2), pp.2608-2615. ⟨10.1093/mnras/stad694⟩
We investigate cosmological structure formation in Fuzzy Dark Matter (FDM) with an attractive self-interaction (SI) with numerical simulations. Such a SI would arise if the FDM boson were an ultra-light axion, which has a strong CP symmetry-breaking
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c71439018b9bc32f87ebf300b841de9
http://dro.dur.ac.uk/38499/
http://dro.dur.ac.uk/38499/
Autor:
Helen Meskhidze, Francisco J Mercado, Omid Sameie, Victor H Robles, James S Bullock, Manoj Kaplinghat, James O Weatherall
Self-interacting dark matter (SIDM) models have received great attention over the past decade as solutions to the small-scale puzzles of astrophysics. Though there are different implementations of dark matter (DM) self-interactions in N-body codes of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cedbf6c2091595afc300c26fafeb9471
Autor:
Victor H. Robles, Robyn E. Sanderson, Omid Sameie, Michael Boylan-Kolchin, Drona Vargya, Philip F. Hopkins, Andrew Wetzel, Andrew S. Graus, James S. Bullock
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 507, iss 1
We present a suite of baryonic cosmological zoom-in simulations of self-interacting dark matter (SIDM) haloes within the ``Feedback In Realistic Environment'' (FIRE) project. The three simulated haloes have virial masses of $\sim 10^{12}\, \text{M}_\
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec2a3dd55f462d9a35e5bd4eca24c7b3
https://resolver.caltech.edu/CaltechAUTHORS:20211020-212403723
https://resolver.caltech.edu/CaltechAUTHORS:20211020-212403723
Autor:
Frank C. van den Bosch, Dhruba Dutta Chowdhury, Tzihong Chiueh, Tom Broadhurst, Hsi-Yu Schive, Victor H. Robles, Pieter G. van Dokkum
Fuzzy Dark Matter (FDM), consisting of ultralight bosons ($m_{\rm b} \sim 10^{-22}\ \rm eV$), is an intriguing alternative to Cold Dark Matter. Numerical simulations that solve the Schr\"odinger-Poisson (SP) equation show that FDM halos consist of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af81dd68c4a20e14b2908885d96aaa0d
http://arxiv.org/abs/2105.05268
http://arxiv.org/abs/2105.05268
Publikováno v:
Physical Review D. 103
In recent years, the scalar field dark matter (SFDM), also called ultralight bosonic dark matter, has received considerable attention due to the number of problems it might help to solve. Among these are the cusp-core problem and the abundance of sma
Autor:
James S. Bullock, Victor H. Robles
Using the phat-ELVIS suite of Milky Way-size halo simulations, we show that subhalo orbital pericenters, $r_{\rm peri}$, correlate with their dark matter halo structural properties. Specifically, at fixed maximum circular velocity, $V_{\rm max}$, sub
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ed44dfdc3ff00e8215c4910e47335dc
http://arxiv.org/abs/2012.07865
http://arxiv.org/abs/2012.07865
Autor:
James S. Bullock, Victor H. Robles, Christopher C. Hayward, Michael Boylan-Kolchin, Alejandro González-Samaniego, Philip F. Hopkins, Dušan Kereš, Claude André Faucher-Giguère, Oliver D. Elbert, Alex Fitts
Publikováno v:
NASA Astrophysics Data System
We compare a suite of four simulated dwarf galaxies formed in 10$^{10} M_{\odot}$ haloes of collisionless Cold Dark Matter (CDM) with galaxies simulated in the same haloes with an identical galaxy formation model but a non-zero cross-section for dark
Autor:
James S. Bullock, Kareem El-Badry, Andrew Wetzel, Andrew S. Graus, Brandon Bozek, Alex Fitts, Dušan Kereš, Victor H. Robles, Claude André Faucher-Giguère, Shea Garrison-Kimmel, Philip F. Hopkins, Michael Boylan-Kolchin
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 490, iss 1
We present a suite of FIRE-2 cosmological zoom-in simulations of isolated field dwarf galaxies, all with masses of $M_\mathrm{halo} \approx 10^{10}\,$M$_\odot$ at $z=0$, across a range of dark matter models. For the first time, we compare how both se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::356da42ed0b58616caf5551f4590c6c9
https://resolver.caltech.edu/CaltechAUTHORS:20190206-105636977
https://resolver.caltech.edu/CaltechAUTHORS:20190206-105636977