- DSpace Home
- →
- 08 Faculty of Arts and Sciences
- →
- Department of Physics
- →
- PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics
- →
- Browsing PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics by Title
JavaScript is disabled for your browser. Some features of this site may not work without it.
Browsing PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics by Title
Now showing items 78-97 of 193
-
(International Journal of Modern Physics D, World Scientific Publishing, 2009)Generalization of a known theorem to generate static, spherically symmetric black-hole solutions in higher dimensional Lovelock gravity is presented. Particular limits, such as Gauss-Bonnet (GB) and/or Einstein-Hilbert ...
-
(World Scientific Publishing, 2014-06-24)In this paper, we analyze the Hawking radiation (HR) of a non-asymptotically flat (NAF) dyonic black hole (dBH) in four-dimensional (4D) Einstein–Maxwell–Dilaton (EMD) gravity by using one of the semiclassical approaches ...
-
(Astrophysics and Space Science, Springer, 2015-08-19)Recent research shows that Hawking radiation (HR) is also possible around the trapping horizon of a wormhole. In this article, we show that the HR of gravitino (spin-3/2 ) particles from the traversable Lorentzian wormholes ...
-
(Foundations of Physics, Springer, 2012)Within the context of Born-Infeld (BI) nonlinear electrodynamics (NED) we revisit the non-relativistic, spinless H-atom. The pair potential computed from the Born-Infeld equations is approximated by the Morse type potential ...
-
(Springer, 2016-09-13)Recent studies (Steinhauer in Nat. Phys. 10:864, 2014, Phys. Rev. D 92:024043, 2015) provide compelling evidences that Hawking radiation could be experimentally proven by using an analogue black hole. In this paper, taking ...
-
(Communications in Theoretical Physics, Institute of Physics (IOP) Publishing, 2014)In this paper, we consider the relativistic Hamilton-Jacobi (HJ) equation and study the Hawking radiation (HR) of scalar particles from uncharged Grumiller black hole (GBH) which is affordable for testing in astrophysics. ...
-
(International Journal of Theoretical Physics, Springer, 2009)Using the Damour-Ruffini-Sannan, the Parikh-Wilczek and the thin film brick-wall models, we investigate the Hawking radiation of uncharged massive particles from 4-dimensional linear dilaton black holes, which are the ...
-
(Springer, 2016-08-20)The Hawking radiation is considered as a quantum tunneling process, which can be studied in the framework of the Hamilton–Jacobi method. In this study, we present the wave equation for a mass generating massive and charged ...
-
(Journal of Experimental and Theoretical Physics, 2015-09-27)We study the Hawking radiation of spin-1 particles (so-called vector particles) from a three-dimensional rotating black hole with scalar hair using a Hamilton–Jacobi ansatz. Using the Proca equation in the WKB approximation, ...
-
(Classical and Quantum Gravity, Institute of Physics (IOP) Publishing: Hybrid Open Access - Green Policies in RoMEO, 2011)We present thin-shell wormhole solutions in Einstein-Yang-Mills-Gauss-Bonnet (EYMGB) theory in higher dimensions d\geq5. Exact black hole solutions are employed for this purpose where the radius of thin-shell lies outside ...
-
(Physics Letters B, Elsevier, 2008)By employing the higher (N\TEXTsymbol{>}5) dimensional version of the Wu-Yang Ansatz we obtain magnetically charged new black hole solutions in the Einstein-Yang-Mills-Lovelock (EYML) theory with second (α2) and third ...
-
(The European Physical Journal C, Springer, 2015-11-19)Recently we have shown that for 2+1−dimensional thin-shell wormholes a non-circular throat may lead to a physical wormhole in the sense that the energy conditions are satisfied. By the same token, herein we consider angular ...
-
(Springer, 2017-02-16)Despite impressive phenomenological success, cosmological models are incomplete without an understanding of what happened at the big bang singularity. Maxwell electrodynamics, considered as a source of the classical Einstein ...
-
(Nuovo Cimento B, Societa Italiana di Fisica, 1987)We study the interacting electromagnetic shock waves with nonconstant profiles in general relativity. It is shown that by modifying the metric functions of the Bell-Szekeres solution, such solutions can be obtained.
-
(Lettere Al Nuovo Cimento, Italian Physical Society, 1982)We present a solution of the Einstein-Maxwell field equations describing the collision of superposed electromagnetic shock plane waves
-
(General Relativity and Gravitation, Springer, 1993)The two well-known solutions of general relativity, the Schwarzschild and the Bertotti-Robinson solutions, are shown to be described by a common metric. In a particular coordinate system we show the connection between ...
-
(Physics Letters B, Elsevier, 2009)We consider the standard Yang-Mills (YM) invariant raised to the power q, i.e., (F(a)μνF(a)μν)q as the source of our geometry and investigate the possible black hole solutions. How does this parameter q modify the black ...
-
(INST PHYSICS ACAD SCI CZECH REPUBLIC, Springer (Online Publishing), 2002)Magnetic fingerprints on the spectra of an interacting electron with a negatively charged ion in a parabolic quantum dot (QD), and of two interacting electrons in such a dot, are investigated via a pseudoperturbative ...
-
(Springer, 2016-05-30)In this paper, we investigate the tunneling process of charged massive bosons W± (spin-1 particles) from noncommutative charged black holes such as charged RN black holes and charged BTZ black holes. By applying the WKB ...
-
(Physics Letters A, Elsevier, 1981)We present another method of generating new solutions from old ones in general relativity. In particular we apply the method to some well-known classes of gravitational fields.
Now showing items 78-97 of 193
EMU I-Rep by Eastern Mediterranean University Institutional Repository is licensed under a Creative Commons Attribution-Gayriticari-NoDerivs 3.0 Unported License
EMU I-Rep:
