Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Mateja Gosenca"'
Autor:
Mateja Gosenca, Peter Coles
Publikováno v:
The Open Journal of Astrophysics, Vol 1 (2016)
We explore the dynamical behaviour of cosmological models involving a scalar field (with an exponential potential and a canonical kinetic term) and a matter fluid with spatial curvature included in the equations of motion. Using appropriately defined
Externí odkaz:
https://doaj.org/article/2f3aa5d1f2ca4ac8bf2c394f95e32a17
Autor:
Mateja Gosenca, Andrew Eberhardt, Yourong Wang, Benedikt Eggemeier, Emily Kendall, J. Luna Zagorac, Richard Easther
Publikováno v:
INSPIRE-HEP
Ultralight dark matter (ULDM) is usually taken to be a single scalar field. Here we explore the possibility that ULDM consists of $N$ light scalar fields with only gravitational interactions. This configuration is more consistent with the underlying
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eceb72d4573d75618c7634edbb7473d9
http://arxiv.org/abs/2301.07114
http://arxiv.org/abs/2301.07114
Publikováno v:
Physical Review D. 102
The distinctive effects of fuzzy dark matter are most visible at nonlinear galactic scales. We present the first simulations of mixed fuzzy and cold dark matter, obtained with an extended version of the nyx code. Fuzzy (or ultralight or axionlike) da
Publikováno v:
Physical Review D. 100
We recently showed that postulated ultracompact minihalos with a steep density profile do not form in realistic simulations with enhanced initial perturbations. In this paper we assume that a small fraction of the dark matter consists of primordial b
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2019, 99 (8), pp.083524. ⟨10.1103/PhysRevD.99.083524⟩
Physical Review D
Physical Review D, American Physical Society, 2019, 99 (8), pp.083524. ⟨10.1103/PhysRevD.99.083524⟩
Phys.Rev.D, 2019, 99 (8), pp.083524. ⟨10.1103/PhysRevD.99.083524⟩
Physical Review D
Physical Review D, American Physical Society, 2019, 99 (8), pp.083524. ⟨10.1103/PhysRevD.99.083524⟩
We chart a path toward solving for the nonlinear gravitational dynamics of cold dark matter by relying on a semiclassical description using the propagator. The evolution of the propagator is given by a Schr\"odinger equation, where the small paramete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9fe72ba12b211d73151bc5cf40075034
http://arxiv.org/abs/1812.05633
http://arxiv.org/abs/1812.05633
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2017, 96 (12), pp.123519. ⟨10.1103/PhysRevD.96.123519⟩
Physical Review D
Physical Review D, American Physical Society, 2017, 96 (12), pp.123519. ⟨10.1103/PhysRevD.96.123519⟩
Phys.Rev.D, 2017, 96 (12), pp.123519. 〈10.1103/PhysRevD.96.123519〉
Phys.Rev.D, 2017, 96 (12), pp.123519. ⟨10.1103/PhysRevD.96.123519⟩
Physical Review D
Physical Review D, American Physical Society, 2017, 96 (12), pp.123519. ⟨10.1103/PhysRevD.96.123519⟩
Phys.Rev.D, 2017, 96 (12), pp.123519. 〈10.1103/PhysRevD.96.123519〉
We perform three-dimensional simulations of structure formation in the early Universe, when boosting the primordial power spectrum on approximately kpc scales. We demonstrate that our simulations are capable of producing power-law profiles close to t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8093d46d6f295b2bec1f117f07b08214
https://hal.archives-ouvertes.fr/hal-01703589
https://hal.archives-ouvertes.fr/hal-01703589
Autor:
Peter Coles, Mateja Gosenca
Publikováno v:
The Open Journal of Astrophysics, Vol 1 (2016)
The Open Journal of Astrophysics
The Open Journal of Astrophysics
We explore the dynamical behaviour of cosmological models involving a scalar field (with an exponential potential and a canonical kinetic term) and a matter fluid with spatial curvature included in the equations of motion. Using appropriately defined
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39be99efe6c9841d91b41cc9a4af4d52
Within a cosmological context, we study the behaviour of collisionless particles in the weak field approximation to General Relativity, allowing for large gradients of the fields and relativistic velocities for the particles. We consider a sphericall
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::faf610eedfde933ac4dd021d2655edd1
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2015:013-013
We develop a needlet approach to estimate the amplitude of general (including non-separable) bispectra and trispectra in the cosmic microwave background, and apply this to the WMAP 9-year data. We obtain estimates for the `orthogonal' bispectrum mode