Maeda, Spacetime structure of static solutions in Gauss–Bonnet gravity: charged case. Maeda, Spacetime structure of static solutions in Gauss–Bonnet gravity: neutral case. Chakraborty, Role of modified Chaplygin gas in accelerated universe. Benaoum, Accelerated universe from modified Chaplygin gas and tachyonic fluid. Xing, Charged Lovelock black holes in the presence of dark fluid with a nonlinear equation of state. Ogawa, A Note on classical solution of Chaplygin gas as d-branes. In this paper, we study the spontaneous scalarization of ReissnerNordström (RN) black holes enclosed by a cavity in an EinsteinMaxwell-scalar (EMS) model with non-minimal couplings between the scalar and Maxwell fields. Dore, Are Chaplygin gases serious contenders to the dark energy throne? Phys. Browse 4512 incredible Black Hole Background vectors, icons, clipart graphics, and backgrounds for royalty-free download from the creative contributors at. Carturan, WMAP and the generalized Chaplygin gas. Finelli, Cosmological effects of a class of fluid dark energy models. Sen, Generalized Chaplygin gas, accelerated expansion and dark energy-matter unification. Viollier, Unification of dark matter and dark energy: the Inhomogeneous Chaplygin gas. Pasquier, An alternative to quintessence. Richarte, Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background. S. Habib Mazharimousavi, M. Halilsoy, 5D black hole solution in Einstein-Yang-Mills-Gauss-Bonnet theory. Mahmoudi, Thermodynamic analysis of topological black holes in Gauss–Bonnet gravity with nonlinear source. Martinez, Lovelock black holes with a nonlinear Maxwell field. Wiltshire, Black holes in string-generated gravity models. Gallo, Radiating black hole solutions in Einstein–Gauss–Bonnet gravity. Bezerra, Black holes with cloud of strings and quintessence in Lovelock gravity. Lee, Lovelock black holes surrounded by quintessence. Maharaj, Quintessence background for 5D Einstein–Gauss–Bonnet black holes. For asymptotically de Sitter black hole, no \(P-r_\)m black hole. For asymptotically anti-de Sitter black hole, there exists the so-called small/large black hole phase transition, and we obtain critical values of pressure, volume and temperature and investigate the effects of both the Gauss–Bonnet gravity and the modified Chaplygin gas on these values. The short linear feature near the center of the image is a jet produced by the black hole. This image was captured by FORS2 on ESO's Very Large Telescope. The supermassive black hole imaged by the EHT is located in the center of the elliptical galaxy M87, located about 55 million light years from Earth. We analyze the parametric regions for both kinds of solutions. This is the first picture of a black hole. The spacetime structure of the obtained black hole solution could be asymptotically anti-de Sitter or de Sitter, according to the specific values of modified Chaplygin gas parameters versus the cosmological constant. Supposing the existence of modified Chaplygin gas with the equation of state \(p=A\rho -B/\rho ^\beta\) as a cosmic background, we obtain a static spherically symmetric solution to the Einstein–Gauss–Bonnet gravitational equations in 5D spacetime.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |