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Иш: Vacuum and plasma magnetosphere around rotating magnetized neutron stars in Bocharova–Bronnikov–Melnikov–Bekenstein geometry

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>C</mml:mi></mml:math>metric with a conformally coupled scalar field in a magnetic universe
Marco Astorino
Мақола20135 иқтибос
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Pulsar death lines and death valley
Kaiyou Chen, M. Ruderman
Мақола19935 иқтибос
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Gravitational lensing effects of black hole with conformally coupled scalar hair
Qi Qi, Yuan Meng, Xi-Jing Wang +1
Мақола20234 иқтибос
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The Bocharova–Bronnikov–Melnikov–Bekenstein black hole’s exact quasibound states and Hawking radiation
David Senjaya
Мақола20244 иқтибос
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Radio loudness and spindown of pulsars in Einstein-aether gravity
Ashfaque H. Bokhari, Javlon Rayimbaev, Bobomurat Ahmedov
МақолаPulsars and Gravitational Waves ResearchPhysics of the Dark Universe20213 иқтибос
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Exact black hole solutions with a conformally coupled scalar field and dynamic Ricci curvature in
Thanasis Karakasis, Eleftherios Papantonopoulos, Zi-Yu Tang +1
Мақола20213 иқтибос
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On thermodynamics of AdS black holes with scalar hair
Li Li
Мақола20212 иқтибос
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Endowing black holes with beyond-Horndeski primary hair: An exact solution framework for scalarizing in every dimension
Olaf Baake, Adolfo Cisterna, Mokhtar Hassaı̈ne +1
Мақола20242 иқтибос
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Photon ring bounds of scalar hairy charged black holes
Yun Soo Myung
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