Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Mario A. Rodriguez-Meza"'
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 81, Iss 4, Pp 1-9 (2021)
European Physical Journal
European Physical Journal
Motivated by two seminal models proposed to explain the Universe acceleration, this paper is devoted to study a hybrid model which is constructed through a generalized Chaplygin gas with the addition of a bulk viscosity. We call the model a Viscous G
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:5127-5144
We present a non-parametric reconstruction of the rotation curves (RC) for 88 spiral galaxies under the LOESS+SIMEX technique. In order to compare methods we also perform the parametric approach assuming core and cuspy dark matter (DM) profiles: PISO
Autor:
Jorge L. Cervantes-Cota, Alejandro Aviles, Mario A. Rodriguez-Meza, Georgios Valogiannis, Baojiu Li, Rachel Bean
Publikováno v:
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics, 2021, Vol.2021(04), pp.039 [Peer Reviewed Journal]
Journal of Cosmology and Astroparticle Physics, 2021, Vol.2021(04), pp.039 [Peer Reviewed Journal]
We develop a framework to compute the redshift space power spectrum (PS), with kernels beyond Einstein-de Sitter (EdS), that can be applied to a wide variety of generalized cosmologies. We build upon a formalism that was recently employed for standar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41c6b91c971f233f06d05090b5703928
http://arxiv.org/abs/2012.05077
http://arxiv.org/abs/2012.05077
Publikováno v:
RSC Advances. 8:10785-10793
Understanding the behaviour of nanoscale systems is of great importance to tailor their properties. To this aim, we investigate the Young's modulus (YM) of defect-free and defective armchair bilayer silicene nanoribbons (SNRs), at room temperature, a
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 475:1447-1468
Cold dark matter (CDM) has shown to be an excellent candidate for the dark matter (DM) of the Universe at large scales, however it presents some challenges at the galactic level. The scalar field dark matter (SFDM), also called fuzzy, wave, Bose-Eins
Autor:
Mario A. Rodriguez-Meza
Publikováno v:
Ciencia Ergo Sum, Vol 24, Iss 1, Pp 65-74 (2017)
We describe the main scientific developments that lead LIGO project to the detection of the gravitational waves: general relativity, black holes and gravitational waves predictions; numerical relativity and the collision and coalescence simulations o
Scalar fields have been used as candidates for dark matter in the universe, from axions with masses $\sim10^{-5}$eV until ultra-light scalar fields with masses $\sim10^{-22}$eV. Axions behave as cold dark matter while the ultra-light scalar fields ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e92515073b4995b84a1856a3e855a17
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2018:013-013
In this work we extend the perturbation theory for modified gravity (MG) in two main aspects. First, the construction of matter overdensities from Lagrangian displacement fields is shown to hold in a general framework, allowing us to find Standard Pe
Publikováno v:
Journal of Physics: Conference Series. 1010:012006
We present in this work a study of brane theory phenomenology focusing on the brane tension parameter, which is the main observable of the theory. We show the modifications steaming from the presence of branes in the rotation curves of spiral galaxie
Publikováno v:
NASA Astrophysics Data System
We report results on the Young's modulus (YM) of defect-free and defective silicene nanoribbons (SNRs) as a function of length and temperature. In this study, we perform molecular dynamics simulations using the Environment-Dependent Interatomic Poten
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e66bd184a490c8d2ce10b8f28c7f62f0
http://arxiv.org/abs/1510.01174
http://arxiv.org/abs/1510.01174