Effective sound speed in relativistic accretion discs around Schwarzschild black holes
Md Arif Shaikh, Susovan Maity, Sankhasubhra Nag, Tapas Kumar Das

TL;DR
This paper introduces an effective dynamical sound speed in relativistic accretion discs around Schwarzschild black holes, resolving the discrepancy between critical and sonic points by ensuring the Mach number equals unity at the critical point.
Contribution
The study proposes a novel effective sound speed derived from linear acoustic perturbations, unifying the critical and sonic points in relativistic accretion disc models.
Findings
Effective sound speed aligns critical and sonic points.
Modified disc structure with unified critical and sonic points.
Enhanced analytical simplicity in accretion flow modeling.
Abstract
For low angular momentum axially symmetric accretion flow maintained in hydrostatic equilibrium along the vertical direction, the value of the Mach number at the critical points deviates from unity, resulting in the non-isomorphism of the critical and the sonic points. This introduces several undesirable complexities while analytically dealing with the stationary integral accretion solutions and the corresponding phase portraits. We propose that introduction of an effective dynamical sound speed may resolve the issue in an elegant way. We linear perturb the full spacetime-dependent general relativistic Euler and the continuity equations governing the structure and the dynamics of accretion disc in vertical equilibrium around Schwarzschild black holes and identify the sonic metric embedded within the stationary background flow. Such metric describes the propagation of the linear acoustic…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
