← Ishga qaytish
Ushbu ish iqtibos qilgan ishlar
92 ta ish
Ish: Black holes surrounded by a Murnaghan-fluid scalar gas in a global-monopole background
Black Hole Mass Decreasing due to Phantom Energy Accretion
Eugeny Babichev, V. I. Dokuchaev, Yu. Eroshenko
Maqola20044 iqtibosABIA wide star–black-hole binary system from radial-velocity measurements
Jifeng Liu, Haotong Zhang, Andrew W. Howard +52
Maqola20193 iqtibosABIBehavior of quasinormal modes and high dimension RN–AdS black hole phase transition
M. Chabab, H El Moumni, S. Iraoui +1
Maqola20163 iqtibosABIFour <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mrow> <mml:mi>S</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>T</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>U</mml:mi> </mml:mrow> </mml:mrow> </mml:math> black holes shadows
Yassine Sekhmani, Dhruba Jyoti Gogoi, Ratbay Myrzakulov +2
Maqola20243 iqtibosABIUnified Dark Matter Scalar Field Models
Daniele Bertacca, Nicola Bartolo, Sabino Matarrese
Maqola20102 iqtibosABI