Tilted thin accretion disks in the full Kerr spacetime and their implications

arXiv:2607.08728 · astro-ph.HE, gr-qc · Submitted 2026-07-09 · Read on arXiv

K. S. Sruthy, Chandrachur Chakraborty, Sudip Bhattacharyya

MCNS, India · MCNS, India · TIFR, India and MIT, USA

astro-ph.HE, gr-qc

Submitted: 2026-07-09

Comments: 25 pages, 17 figures, 2 tables, matches published version

Journal ref: Phys. Rev. D 114, 043004 (2026)

DOI: 10.1103/rxqz-kk68

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Alignment — 51× in this paper · explained in 1 episode
• Anisotropy — 2× in this paper · explained in 3 episodes
• Manipal Academy of Higher Education — 2× in this paper
• AGN — 1× in this paper · explained in 1 episode
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
• Multiwavelength Classification of Chandra Sources in Omega Centauri
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2