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arxiv: 2605.08582 · v1 · submitted 2026-05-09 · 🌀 gr-qc · astro-ph.GA· hep-th· physics.class-ph

Recognition: 2 theorem links

· Lean Theorem

Black hole mass and distance from accretion disk astrophysical observables

Authors on Pith no claims yet

Pith reviewed 2026-05-12 01:20 UTC · model grok-4.3

classification 🌀 gr-qc astro-ph.GAhep-thphysics.class-ph
keywords Schwarzschild black holefrequency shiftredshift rapidityorbital observablesblack hole massdistance to Earthpeculiar motion
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The pith

Analytical expressions determine Schwarzschild black hole mass and distance from orbital frequency shifts.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper derives novel analytical expressions for the mass and distance of a Schwarzschild black hole as well as the orbital radius of test particles in terms of astrophysical observables from frequency shifts measured throughout the orbit. By modeling photons from symmetrically opposite emitters relative to the line of sight and introducing redshift rapidity, the expressions for mass and distance become independent. The work also provides closed formulas when the system has peculiar motion. A reader might care because this offers a direct way to infer black hole properties solely from observable frequency changes without additional assumptions about the system.

Core claim

Using a general relativistic description of frequency shifts from two emitters located symmetrically opposite each other with respect to the observer's line of sight, and defining the redshift rapidity, we obtain independent analytical expressions for the black hole mass and its distance to Earth, along with the orbital radius, in terms of observables measured along the entire orbit of the revolving particle. The study extends these closed formulas to the case of systems with peculiar motion.

What carries the argument

Redshift rapidity, which decouples the black hole mass and distance expressions from frequency shift data collected symmetrically around the orbit.

If this is right

  • Mass and distance are determined separately via redshift rapidity.
  • Orbital radius is expressed directly from the same observables.
  • Closed formulas hold even when the astrophysical system has peculiar motion.
  • All quantities follow from frequency shift measurements throughout the orbit.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The method could apply to real accretion disk data around supermassive black holes to estimate parameters without dynamical modeling.
  • If the symmetry assumption holds only approximately, the formulas might still provide first-order estimates for mass and distance.
  • Extension to Kerr black holes would require generalizing the symmetric emitter positions and rapidity definition.
  • Comparison with existing mass estimates from stellar orbits or other techniques could validate or refine the approach.

Load-bearing premise

That frequency shifts can be measured cleanly along the full orbit from symmetrically opposite positions without dominant interference from other effects like disk turbulence or absorption.

What would settle it

Measuring the mass and distance for a known system like the black hole in the Milky Way center using this method and finding significant disagreement with established values from independent observations.

read the original abstract

In this work we derive novel analytical expressions for the mass and distance of a Schwarzschild black hole (BH), as well as for the orbital radius of test particles orbiting it, it terms of astrophysical observables measured throughout the entire orbit of the revolving particle. We use a general relativistic method to describe the frequency shifts of photons emitted in the vivinity of a BH by considering two emitters (or two positions of the same emitter) located symmetrically opposite to each other with respect to the observer's line of sight (LOS) when performing measurements along the orbit. Furthermore, the introduction of the redshift rapidity allows us to write independent expressions for the BH mass and its distance to Earth. We also extend our study to the case when astrophysical systems have a peculiar motion and derive the corresponding closed formulas.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 3 minor

Summary. The paper derives novel analytical expressions for the mass and distance of a Schwarzschild black hole, as well as for the orbital radius of test particles orbiting it, in terms of astrophysical observables (frequency shifts) measured throughout the entire orbit of the revolving particle. The approach uses a general relativistic description of photon frequency shifts by considering two emitters (or positions of the same emitter) located symmetrically opposite each other with respect to the observer's line of sight, and introduces a redshift rapidity variable to obtain independent expressions for mass and distance. Extensions to the case of peculiar motion are also provided with corresponding closed formulas.

Significance. If the derivations are correct, this work could offer a useful new method for determining black hole mass and distance directly from accretion disk frequency shift data, complementing existing techniques such as stellar dynamics or gravitational wave observations. The closed-form expressions and explicit treatment of peculiar motion represent strengths that could enable practical applications, provided the symmetry assumption can be realized in observations.

minor comments (3)
  1. [Abstract] Abstract contains typographical errors: 'it terms' should be 'in terms' and 'vivinity' should be 'vicinity'.
  2. [Methods or derivation section] The symmetry assumption for emitter positions is central but its practical selection from observational data (e.g., how to identify or approximate symmetric points along the orbit) would benefit from additional clarification to aid reproducibility.
  3. [Results or discussion] Verification of the new expressions against known limits (such as the weak-field or Newtonian regime) is not mentioned in the provided abstract and should be included to strengthen confidence in the results.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for the positive and accurate summary of our manuscript, which correctly identifies the novel closed-form expressions for Schwarzschild black hole mass, distance, and orbital radius derived from full-orbit frequency shift observables using symmetric emitter positions and redshift rapidity. We also appreciate the note on the extension to peculiar motion. The recommendation for minor revision is noted; however, the report contains no specific major comments requiring point-by-point rebuttal or manuscript changes.

Circularity Check

0 steps flagged

Derivation is self-contained from standard GR redshift formulas plus explicit symmetry assumption

full rationale

The paper constructs closed-form expressions for Schwarzschild mass M, distance D, and orbital radius directly from frequency-shift observables measured along the full orbit. It employs the standard general-relativistic photon frequency-shift formula in Schwarzschild spacetime, introduces the auxiliary redshift-rapidity variable to separate the M–D degeneracy, and invokes an explicit modeling assumption that two emitters (or positions) lie symmetrically opposite with respect to the line of sight. No step reduces by algebraic identity to a fitted parameter, no self-citation supplies a uniqueness theorem or ansatz, and the symmetry assumption is stated as an input rather than derived from the target quantities. The resulting formulas are therefore independent outputs of the chosen coordinate system and redshift definitions, not tautological restatements of the inputs.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 1 invented entities

Only the abstract is available, so the ledger is necessarily incomplete and based on stated elements.

axioms (2)
  • domain assumption Spacetime around the black hole is described by the Schwarzschild metric of general relativity
    Invoked to compute gravitational and Doppler frequency shifts for orbiting emitters
  • domain assumption Test particles follow geodesic orbits and emit photons whose frequency shifts can be measured throughout the full orbit
    Required for the symmetric-emitter construction and extraction of observables
invented entities (1)
  • redshift rapidity no independent evidence
    purpose: To obtain independent expressions for black-hole mass and distance from the same set of frequency-shift observables
    Introduced in the abstract as the key new device that decouples mass from distance

pith-pipeline@v0.9.0 · 5453 in / 1431 out tokens · 42677 ms · 2026-05-12T01:20:28.146534+00:00 · methodology

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Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
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uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Reference graph

Works this paper leans on

33 extracted references · 33 canonical work pages · 1 internal anchor

  1. [1]

    B. P . Abbott, et al., Observation of Gravitational Waves from a Binary Black Hole Merger, Phys. Rev. Lett. 116 (2016) 061102, 10.1103/PhysRevLett.116.061102

  2. [2]

    E. H. T. Collaboration, et al., First M87 Event Horizon Tele- scope Results. I. The Shadow of the Supermassive Black Hole, The Astrophysical Journal Letters 875 (2019) L1, 10.3847/ 2041-8213/ab0ec7

  3. [3]

    E. H. T. Collaboration, et al., First Sagittarius A* Event Hori- zon Telescope Results. VI. Testing the Black Hole Metric, The Astrophysical Journal Letters 930 (2022) L17, 10.3847/ 2041-8213/ac6756

  4. [4]

    D. R. John Kormendy, Inward BoundThe Search for Super- massive Black Holes in Galactic Nuclei, Annual Review As- tronomy and Astrophysics 35 (1995) 581, https://doi. org/10.1146/annurev.aa.33.090195.003053

  5. [5]

    and Tremaine, S

    J. Magorrian, et al., The Demography of Massive Dark Objects in Galaxy Centers, The Astronomical Journal 115 (1998) 2285, 10.1086/300353

  6. [6]

    López-Cruz, et al., The Brightest Cluster Galaxy in A85: The Largest Core Known so Far, The Astrophysical Journal Letters 795 (2014) L31, 10.1088/2041-8205/795/2/ L31

    O. López-Cruz, et al., The Brightest Cluster Galaxy in A85: The Largest Core Known so Far, The Astrophysical Journal Letters 795 (2014) L31, 10.1088/2041-8205/795/2/ L31

  7. [7]

    Nucamendi, M

    U. Nucamendi, M. Salgado, and D. Sudarsky, An alternative approach to the galactic dark matter problem, Phys. Rev. D 63 (2001) 125016, 10.1103/PhysRevD.63.125016

  8. [8]

    Kormendy and L

    J. Kormendy and L. C. Ho, Coevolution (Or Not) of Super- massive Black Holes and Host Galaxies, Annual Review of Astronomy and Astrophysics 51 (2013) 511653, 10.1146/ annurev-astro-082708-101811

  9. [9]

    Herrera-Aguilar and U

    A. Herrera-Aguilar and U. Nucamendi, Kerr black hole pa- rameters in terms of the redshift/blueshift of photons emit- Rev. Mex. Fis. ?? (*?*) (????) ???–??? A LATEXTEMPLA TE FOR THE RMF, RMF-E, SRMF 9 ted by geodesic particles, Phys. Rev. D 92 (2015) 045024, 10.1103/PhysRevD.92.045024

  10. [10]

    González-Juárez and A

    A. González-Juárez and A. Herrera-Aguilar, Reviewing the GR Method for Estimating Black Hole Parameters of Megamaser Systems, Astronomische Nachrichten 346 (2025) e20250016, https://doi.org/10.1002/asna.20250016

  11. [11]

    U. Nucamendi, et al., Toward the Gravitational Redshift De- tection in NGC 4258 and the Estimation of Its Black Hole Mass-to-distance Ratio, The Astrophysical Journal Letters 917 (2021) L14, 10.3847/2041-8213/ac151b

  12. [12]

    M. Momennia, et al., Schwarzschild black hole and redshift ra- pidity: a new approach towards measuring cosmic distances, The European Physical Journal C 84 (2024) 583, https: //doi.org/10.1140/epjc/s10052-024-12933-0

  13. [13]

    S. González-Salud, et al., A differential-geometry approach to black hole characterization of megamaser systems in static spherically symmetric spacetimes (2026), URL https:// arxiv.org/abs/2601.16308

  14. [14]

    Mass and distance of AGN black holes from warped accretion disks

    A. González-Juárez and A. Herrera-Aguilar, Mass and distance of AGN black holes from warped accretion disks (2025), URL https://arxiv.org/abs/2509.23029

  15. [15]

    Becerril, S

    R. Becerril, S. V aldez-Alvarado, and U. Nucamendi, Obtain- ing mass parameters of compact objects from redshifts and blueshifts emitted by geodesic particles around them, Phys. Rev. D 94 (2016) 124024, 10.1103/PhysRevD.94. 124024

  16. [16]

    Herrera-Aguilar, R

    A. Herrera-Aguilar, R. Lizardo-Castro, and U. Nucamendi, General relativistic formulas for mass and spin of a Kerr black hole in terms of redshifts and orbital parameters, arXiv e- prints (2018) arXiv:1805.10512, 10.48550/arXiv.1805. 10512

  17. [17]

    Becerril, et al., Mass parameter and the bounds on redshifts and blueshifts of photons emitted from geodesic particle orbit- ing in the vicinity of regular black holes, Phys

    R. Becerril, et al., Mass parameter and the bounds on redshifts and blueshifts of photons emitted from geodesic particle orbit- ing in the vicinity of regular black holes, Phys. Rev. D 103 (2021) 084054, 10.1103/PhysRevD.103.084054

  18. [18]

    Tinto and J

    P . Banerjee, et al., Mass and spin of Kerr black holes in terms of observational quantities: The dragging effect on the redshift, Phys. Rev. D 105 (2022) 124037, 10.1103/PhysRevD. 105.124037

  19. [19]

    Momennia, A

    M. Momennia, A. Herrera-Aguilar, and U. Nucamendi, Kerr black hole in de Sitter spacetime and observational redshift: To- ward a new method to measure the Hubble constant, Phys. Rev. D 107 (2023) 104041, 10.1103/PhysRevD.107.104041

  20. [20]

    D. A. Martínez-V alera, M. Momennia, and A. Herrera-Aguilar, Observational redshift from general spherically symmetric black holes, The European Physical Journal C 84 (2024), 10.1140/epjc/s10052-024-12649-1

  21. [21]

    G. Morales-Herrera, et al., Mass, charge, and distance to ReissnerNordström black hole in terms of directly measur- able quantities, The European Physical Journal C 84 (2024), 10.1140/epjc/s10052-024-12880-w

  22. [22]

    Momennia, Kerr black hole parameters and its distance from the Earth in terms of directly measurable quantities of accretion disk (2025), URL https://arxiv.org/abs/ 2501.04677

    M. Momennia, Kerr black hole parameters and its distance from the Earth in terms of directly measurable quantities of accretion disk (2025), URL https://arxiv.org/abs/ 2501.04677

  23. [23]

    A. J. Barger, ed., Supermassive black holes in the distant universe (Kluwer Academic, Dordrecht, Netherlands, 2004), 10.1007/978-1-4020-2471-9

  24. [24]

    Lo, Mefa-masers and Galaxies, Annual Review of Astron- omy and Astrophysics 43 (2005) 625, https://doi.org/ 10.1146/annurev.astro.41.011802.094927

    K. Lo, Mefa-masers and Galaxies, Annual Review of Astron- omy and Astrophysics 43 (2005) 625, https://doi.org/ 10.1146/annurev.astro.41.011802.094927

  25. [25]

    J. R. Herrnstein, et al., The Geometry of and Mass Accretion Rate through the Maser Accretion Disk in NGC 4258, The As- trophysical Journal 629 (2005) 719738, 10.1086/431421

  26. [26]

    J. A. Braatz, et al., The Megamaser Cosmology Project. II. The Angular-diameter Distance to UGC 3789, Astrophysical Jour- nal 718 (2010) 657, 10.1088/0004-637X/718/2/657

  27. [28]

    C. Y . Kuo, et al., The Megamaser Cosmology Project. V . An Angular-diameter Distance to NGC 6264 at 140 Mpc, Astro- physical Journal 767 (2013) 155, 10.1088/0004-637X/ 767/2/155

  28. [29]

    C. Y . Kuo, et al., The Megamaser Cosmology Project. VI. Ob- servations of NGC 6323, Astrophysical Journal 800 (2015) 26, 10.1088/0004-637X/800/1/26

  29. [30]

    Gao, et al., The Megamaser Cosmology Project

    F. Gao, et al., The Megamaser Cosmology Project. VIII. A Ge- ometric Distance to NGC 5765b, Astrophysical Journal 817 (2016) 128, 10.3847/0004-637X/817/2/128

  30. [31]

    Gao, et al., The Megamaser Cosmology Project

    F. Gao, et al., The Megamaser Cosmology Project. IX. Black Hole Masses for Three Maser Galaxies, Astrophysical Journal 834 (2017) 52, 10.3847/1538-4357/834/1/52

  31. [32]

    Balasin and H

    H. Balasin and H. Nachbagauer, The energy-momentum ten- sor of a black hole, or what curves the Schwarzschild ge- ometry?, Classical and Quantum Gravity 10 (1993) 2271, 10.1088/0264-9381/10/11/010

  32. [33]

    E. M. L. Humphreys, et al., Toward a New Geometric Distance to the Active Galaxy NGC 4258. II. Centripetal Accelerations and Investigation of Spiral Structure, The Astrophysical Jour- nal 672 (2008) 800, 10.1086/523637

  33. [34]

    T. M. Davis and M. I. Scrimgeour, Deriving accurate peculiar velocities (even at high redshift), Monthly Notices of the Royal Astronomical Society 442 (2014) 1117, 10.1093/mnras/ stu920 Rev. Mex. Fis. ?? (*?*) (????) ???–???