Pages that link to "Item:Q5696074"
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The following pages link to Relativistic thick discs in the Kerr–de Sitter backgrounds (Q5696074):
Displaying 11 items.
- Aspects of GRMHD in high-energy astrophysics: geometrically thick disks and tori agglomerates around spinning black holes (Q2060526) (← links)
- Conformastationary disk-haloes in Einstein-Maxwell gravity (Q2353203) (← links)
- Equatorial circular orbits in Kerr-anti-de Sitter spacetimes (Q2435123) (← links)
- Proto-jet configurations in RADs orbiting a Kerr SMBH: symmetries and limiting surfaces (Q3177489) (← links)
- RELATIVISTIC DYNAMICS WITH COSMOLOGICAL CONSTANT: SPINNING TEST PARTICLES AND PERFECT FLUID TORI (Q3397911) (← links)
- ROTATING RELATIVISTIC THIN DISKS AS SOURCES OF CHARGED AND MAGNETIZED KERR–NUT SPACE–TIMES (Q3401063) (← links)
- PSEUDO-NEWTONIAN GRAVITATIONAL POTENTIAL FOR SCHWARZSCHILD–DE SITTER SPACE–TIMES (Q3631021) (← links)
- COMPARISON OF GENERAL RELATIVISTIC AND PSEUDO-NEWTONIAN DESCRIPTION OF MAGELLANIC-CLOUDS MOTION IN THE FIELD OF MILKY WAY (Q4911485) (← links)
- Shadow of the rotating black hole with quintessential energy in the presence of plasma (Q4976096) (← links)
- Retrograde polish doughnuts around boson stars (Q5026022) (← links)
- Charged fluids encircling compact objects: force representations and conformal geometries (Q5162438) (← links)