← Ishga qaytish
Ushbu ish iqtibos qilgan ishlar
70 ta ish
Ish: Kalb-Ramond black holes sourced by ModMax electrodynamics: Some perturbative properties in the phantom sector
Observation of Gravitational Waves from a Binary Black Hole Merger
B. P. Abbott, R. Abbott, T. D. Abbott +97
MaqolaOchiq kirish2016189 iqtibosABIModified gravity and cosmology
Timothy Clifton, Pedro G. Ferreira, Antonio Padilla +1
MaqolaOchiq kirish201258 iqtibosABIQuasinormal modes of black holes: From astrophysics to string theory
MaqolaOchiq kirish201152 iqtibosABIGeodesic stability, Lyapunov exponents, and quasinormal modes
Vítor Cardoso, Alex S. Miranda, Emanuele Berti +2
MaqolaOchiq kirish200945 iqtibosABIModified gravity theories on a nutshell: Inflation, bounce and late-time evolution
S. Nojiri, S.D. Odintsov, V.K. Oikonomou
MaqolaOchiq kirish201741 iqtibosABIOptical high harmonic generation in Dirac materials
S. Rakhmanov, Kuvonchbek Matchonov, H. Yusupov +2
MaqolaOchiq kirishLaser-Matter Interactions and ApplicationsThe European Physical Journal B202531 iqtibosABIA phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state
MaqolaOchiq kirish200227 iqtibosABIBlack hole normal modes - A semianalytic approach
B. F. Schutz, Clifford M. Will
MaqolaOchiq kirish198525 iqtibosABIQuasinormal modes of black holes: The improved semianalytic approach
MaqolaOchiq kirish201719 iqtibosABILate-time behavior of stellar collapse and explosions. I. Linearized perturbations
Carsten Gundlach, Richard H. Price, Jorge Pullin
MaqolaOchiq kirish199418 iqtibosABIGreybody factor for black string in dRGT massive gravity
P. Boonserm, T. Ngampitipan, Pitayuth Wongjun
MaqolaOchiq kirish201914 iqtibosABIHigher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
R. A. Konoplya, A. Zhidenko, A F Zinhailo
MaqolaOchiq kirish201913 iqtibosABIBOUNDING THE GREYBODY FACTORS FOR NON-ROTATING BLACK HOLES
Tritos Ngampitipan, Petarpa Boonserm
MaqolaOchiq kirish201313 iqtibosABI