Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Ksh. Newton Singh"'
Autor:
Ksh. Newton Singh, Bidisha Samanta, S. K. Maurya, Farook Rahaman, N. Kamal Singh, Anil K. Aria
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 84, Iss 11, Pp 1-10 (2024)
Abstract A shear-free, collapsing compact object, described by an embedding class I solution and emitting radiation, is presented here. Because of the properties of embedding class I, this four-dimensional interior spacetime can be embedded in pseudo
Externí odkaz:
https://doaj.org/article/65891458a12b43e8b93961e4a44260b7
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 84, Iss 3, Pp 1-17 (2024)
Abstract In the present article anisotropic solutions with vanishing complexity in the framework of f(Q) gravity are generated. At first, the field equations in f(Q)-gravity are gravitationally decoupled where the isotropic fluid component correspond
Externí odkaz:
https://doaj.org/article/17de340ef63c47caa771f0d7edbd77d2
Autor:
S. K. Maurya, Abdelghani Errehymy, Ksh. Newton Singh, Nuha Al-Harbi, Kottakkaran Sooppy Nisar, Abdel-Haleem Abdel-Aty
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 83, Iss 10, Pp 1-16 (2023)
Abstract In this paper, we introduce an anisotropic model using a dark matter (DM) density profile in Einstein–Gauss–Bonnet (EGB) gravity using a gravitational decoupling method introduced by Ovalle (Phys Rev D 95:104019, 2017), which has provide
Externí odkaz:
https://doaj.org/article/29f64843909d494899f95b620aae4f67
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 82, Iss 9, Pp 1-11 (2022)
Abstract In the present work we have investigated a new anisotropic solution for polytropic stars in the framework of 4D Einstein–Gauss–Bonnet (EGB) gravity. The possibility of determining the masses and radii of compact stars which puts some lim
Externí odkaz:
https://doaj.org/article/fd1d5ca6d0ef43abbdc2b6627cdf0c05
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 2, p 175 (2024)
We present a rigorous study of compact objects within f ( Q ) gravity where electrical fields and dark matter are studied and provide novel mass–radius relations with models falling in the mass gap of the events GW190814 and GW200210. After formula
Externí odkaz:
https://doaj.org/article/9c5c2caa0ee848539f0cbc284505a350
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 82, Iss 1, Pp 1-13 (2022)
Abstract In this work we explore the characteristics of a polytropic solution for the anisotropic stellar object within the framework of Einstein–Gauss–Bonnet (EGB) gravity. We introduce anisotropy via the minimally gravitational decoupling metho
Externí odkaz:
https://doaj.org/article/7a897be03c024087af4ed0e6f10ed8bc
Publikováno v:
Frontiers in Physics, Vol 10 (2023)
This paper supplements the article (Eur. Phys. J. C 76: 246, 2016) by extending some more new wormhole solutions in the background of Finslerian geometry. Here, we present six more solutions by considering i) a linear equation of state (EoS) pr = ω
Externí odkaz:
https://doaj.org/article/46faf7aebb934c2c8821e2bf86f6e57e
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 81, Iss 10, Pp 1-10 (2021)
Abstract The article explores the first exact solution in a four-dimensional EGB-gravity with an anisotropic matter source. The solution has been found by two assumptions, a metric potential and the MIT-bag equation of state. Further, the solution ha
Externí odkaz:
https://doaj.org/article/4e25592e32ce411bb576ce4e1bd14bd3
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 81, Iss 8, Pp 1-19 (2021)
Abstract In the present article, the solution of the Einstein–Maxwell field equations in the presence of a massive scalar field under the Brans-Dicke (BD) gravity is obtained via embedding approach, which describes a charged anisotropic strange sta
Externí odkaz:
https://doaj.org/article/d7925aaae90d488baccd6f7c8ab1ea14
Publikováno v:
Universe, Vol 9, Iss 5, p 208 (2023)
In the present paper, we focused on exploring the possibility of providing a new class of exact solutions for viable anisotropic stellar systems by means of the massive Brans–Dicke (BD) theory of gravity. In this respect, we used the decoupling of
Externí odkaz:
https://doaj.org/article/a379385fc744479c954ccc1556593795