Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Antonio Pasqua"'
Publikováno v:
Universe, Vol 8, Iss 12, p 623 (2022)
In this paper, we study the inflationary scenario in logarithmic f(R) gravity, where the rate of inflation roll is constant. On the other hand, our gravitational f(R) model is a polynomial plus a logarithmic term. We take advantage of constant-roll c
Externí odkaz:
https://doaj.org/article/843a5b81ee4341c39a457c5da49e4ac6
Autor:
Irina Radinschi, Theophanes Grammenos, Farook Rahaman, Andromahi Spanou, Marius Mihai Cazacu, Surajit Chattopadhyay, Antonio Pasqua
Publikováno v:
Advances in High Energy Physics, Vol 2018 (2018)
The evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant nonzero topological Euler density is performed by using the energy-momentum complexes
Externí odkaz:
https://doaj.org/article/919bf65ac7774d7089283dbed9876acc
Autor:
Irina Radinschi, Theophanes Grammenos, Farook Rahaman, Andromahi Spanou, Sayeedul Islam, Surajit Chattopadhyay, Antonio Pasqua
Publikováno v:
Advances in High Energy Physics, Vol 2017 (2017)
The energy-momentum of a new four-dimensional, charged, spherically symmetric, and nonsingular black hole solution constructed in the context of general relativity coupled to a theory of nonlinear electrodynamics is investigated, whereby the nonlinea
Externí odkaz:
https://doaj.org/article/dc709aedaf3b4b55953e0e45582e4727
Publikováno v:
Advances in High Energy Physics, Vol 2014 (2014)
We consider two-component dark energy models in Lyra manifold. The first component is assumed to be a quintessence field while the second component may be a viscous polytropic gas, a viscous Van der Waals gas, or a viscous modified Chaplygin gas. We
Externí odkaz:
https://doaj.org/article/48afe99e9f1748308b63e474094c9319
Autor:
Antonio Pasqua, Khudhair A. Assaf
Publikováno v:
Advances in Astronomy, Vol 2014 (2014)
The perturbation caused by planet-moon binarity on the time-of-arrival (TOA) signal of a pulsar with an orbiting planet is derived for the case of the orbit of the planet-moon system inclined of an angle α with respect to the plane of
Externí odkaz:
https://doaj.org/article/92fddacfc5d8438db127cec643858be2
Publikováno v:
BMC Ophthalmology, Vol 24, Iss 1, Pp 1-5 (2024)
Abstract Background To describe a case of bilateral multifocal chorioretinitis as the only presentation of acute West Nile virus (WNV) infection in the absence of neurological involvement. Case presentation A 78-year-old Italian woman was admitted to
Externí odkaz:
https://doaj.org/article/8eb5d69f65a7455d8bb639de3913d474
Autor:
Ratbay Myrzakulov, Surajit Chattopadhyay, Antonio Pasqua, Kairat Myrzakulov, Martiros Khurshudyan
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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In this paper, we study the main cosmological properties of the classical Friedmann equations in the case of homogeneous and isotropic Friedmann-Robertson-Walker Universe and we also generalized the expression of the Friedmann equation in the case of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a79b5786c985d64e967f5b74edad8448
http://hdl.handle.net/10261/236746
http://hdl.handle.net/10261/236746
Publikováno v:
Canadian Journal of Physics. 96:112-125
In this paper, we study the effects that are produced by the interaction between a brane Universe and the bulk in which the Universe is embedded. Taking into account the effects produced by the interaction between a brane Universe and the bulk, we de
Publikováno v:
Zeitschrift für Naturforschung A. 71:949-960
The present paper reports a study on accreting tachyon, Dirac-Born-Infeld essence and h-essence scalar field models of dark energy onto Morris-Thorne wormhole. Using three different parameterisation schemes and taking H = H 0 + H 1 t $H\, = \,{H_0}\,
Publikováno v:
Canadian Journal of Physics. 94:201-208
In this paper, we consider the generalized ghost dark energy in a Bianchi type-I metric (which is a spatially homogeneous and anisotropic) in the framework of Brans–Dicke theory. For this purpose, we use the squared sound speed [Formula: see text]