Zobrazeno 1 - 10
of 901
pro vyhledávání: '"Flores, A. V."'
We investigated the radial and non-radial fundamental ($f$) mode oscillations of self-bound (quark) stars obtained after employing the Vector MIT (vMIT) bag model. Within this model, we computed the equation of state for strange quark matter satisfyi
Externí odkaz:
http://arxiv.org/abs/2412.05752
We analyze the sensitivity of non-radial fluid oscillation modes and tidal deformations in neutron stars to high-order nuclear empirical parameters (NEP). In particular, we study the impact of the curvature and skewness of the symmetry energy $K_{\rm
Externí odkaz:
http://arxiv.org/abs/2411.09322
The influence of the dark matter mass~($M_{\chi}$) and the Fermi momentum~($k_{F}^{\dm}$) on the $f_0$-mode oscillation frequency, damping time parameter, and tidal deformability of hadronic stars are studied by employing a numerical integration of h
Externí odkaz:
http://arxiv.org/abs/2402.12600
The effects of the anisotropy on the fluid pulsation modes adopting the so-called Cowling approximation and tidal deformability of strange quark stars are investigated by using the numerical integration of the hydrostatic equilibrium, nonradial oscil
Externí odkaz:
http://arxiv.org/abs/2305.13468
Autor:
Mota, Clésio E., Santos, Luis C. N., da Silva, Franciele M., Flores, Cesar V., Lobo, Iarley P., Bezerra, Valdir B.
In this work, we investigate the existence of neutron stars (NS) in the framework of $f$($\mathbb{T}$,$\mathcal{T}$) gravity, where $\mathbb{T}$ is the torsion tensor and $\mathcal{T}$ is the trace of the energy-momentum tensor. The hydrostatic equil
Externí odkaz:
http://arxiv.org/abs/2301.03067
Autor:
Flores, Eduardo V.
We reveal that the mechanism driving the manifestation of wave effects is fundamentally embedded within quantum field theory. These wave effects become real when conservation laws are satisfied, allowing quantum effects to fully materialize, and rema
Externí odkaz:
http://arxiv.org/abs/2208.12267
Publikováno v:
Eur. Phys. J. C 82 (2022) 527
In this work, we have made a systematic study of how the gravitational wave frequency of the fundamental mode from compact stars is affected by anisotropic effects using realistic equations of state. Our study is an extension of the seminal research
Externí odkaz:
http://arxiv.org/abs/2206.09260
Publikováno v:
In Journal of Cleaner Production 1 December 2024 482
Publikováno v:
In Journal of the Franklin Institute November 2024 361(16)
Autor:
Obeso, Juan L., Flores, Catalina V., Boujnah, Mourad, Viltres, Herlys, Celaya, Christian A., Rosas, Pablo Marín, Esparza-Schulz, J. Marcos, Ibarra, Ilich A., Cordero-Sánchez, Salomón, Peralta, Ricardo A., Leyva, Carolina
Publikováno v:
In Journal of Solid State Chemistry October 2024 338