Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole
Author(s)
Zhang, Dan, Li, Shulan, Fu, Guoyang, Wu, Jian-Pin
Abstract
This letter presents an assessment of quantum gravity effects on extreme-mass-ratio inspirals (EMRIs) for the rotating quantum Oppenheimer-Snyder (qOS) black hole. Employing the adiabatic evolution, we compute the gravitational wave (GW) dephasing, which quantifies the cumulative phase shift induced by the quantum correction α . We further generate the augmented analytic kludge (AAK) waveform and investigate the faithfulness between the waveforms with and without the quantum parameter α for different values of a. Our results reveal that the quantum gravity effect induces detectable imprints in LISA, while the presence of rotation suppresses these signatures. This suggests that rotational degrees of freedom must be carefully accounted for when probing quantum gravity with EMRI observations.
Figures
Caption
Phase diagram of the rotating qOs model in the parameter space of $a/M$ and $\alpha/M^2$. The blue line corresponds to the extremal BH.Caption
Dependence of the dephasing on the quantum parameter $\alpha$ for different values of $a$. The red dashed line indicates the detection threshold of $\Delta\Phi\sim0.1$ rad.Caption
The AAK waveform for the rotation qOS background with different $a$ and $\alpha$.Caption
The AAK waveform for the rotation qOS background with different $a$ and $\alpha$.Caption
Faithfulness between the with and without quantum gravity correction with varying $a$. The red dashed line denotes the distinguishability criterion $\mathcal{F}\simeq0.965$.References
- [1] R. Penrose, Gravitational collapse and space-time singularities, Phys. Rev. Lett. 14 (1965) 57–59.
- [2] S. W. Hawking and R. Penrose, The Singularities of gravitational collapse and cosmology, Proc. Roy. Soc. Lond. A 314 (1970) 529–548.
- [3] C. Rovelli, Loop quantum gravity, Living Rev. Rel. 1 (1998) 1, [gr-qc/9710008].
- [4] T. Thiemann, Lectures on loop quantum gravity, Lect. Notes Phys. 631 (2003) 41–135, [gr-qc/0210094].
- [5] A. Ashtekar and J. Lewandowski, Background independent quantum gravity: A Status report, Class. Quant. Grav. 21 (2004) R53, [gr-qc/0404018].
- [6] M. Han, W. Huang, and Y. Ma, Fundamental structure of loop quantum gravity, Int. J. Mod. Phys. D 16 (2007) 1397–1474, [gr-qc/0509064].
- [7] M. Bojowald, Absence of singularity in loop quantum cosmology, Phys. Rev. Lett. 86 (2001) 5227–5230, [gr-qc/0102069].
- [8] A. Ashtekar, T. Pawlowski, and P. Singh, Quantum nature of the big bang, Phys. Rev. Lett. 96 (2006) 141301, [gr-qc/0602086].
- [9] A. Ashtekar, Introduction to loop quantum gravity and cosmology, Lect. Notes Phys. 863 (2013) 31–56, [arXiv:1201.4598].
- [10] A. Peltola and G. Kunstatter, A Complete, Single-Horizon Quantum Corrected Black Hole Spacetime, Phys. Rev. D 79 (2009) 061501, [arXiv:0811.3240].
- [11] A. Peltola and G. Kunstatter, Effective Polymer Dynamics of D-Dimensional Black Hole Interiors, Phys. Rev. D 80 (2009) 044031, [arXiv:0902.1746].
- [12] L. Modesto, Semiclassical loop quantum black hole, Int. J. Theor. Phys. 49 (2010) 1649–1683, [arXiv:0811.2196].
- [13] A. Ashtekar, J. Olmedo, and P. Singh, Quantum Transfiguration of Kruskal Black Holes, Phys. Rev. Lett. 121 (2018), no. 24 241301, [arXiv:1806.00648].
- [14] A. Ashtekar, J. Olmedo, and P. Singh, Quantum extension of the Kruskal spacetime, Phys. Rev. D 98 (2018), no. 12 126003, [arXiv:1806.02406].
- [15] R. Gambini, J. Olmedo, and J. Pullin, Spherically symmetric loop quantum gravity: analysis of improved dynamics, Class. Quant. Grav. 37 (2020), no. 20 205012, [arXiv:2006.01513].
- [16] N. Bodendorfer, F. M. Mele, and J. Münch, Effective Quantum Extended Spacetime of Polymer Schwarzschild Black Hole, Class. Quant. Grav. 36 (2019), no. 19 195015, [arXiv:1902.04542].
- [17] N. Bodendorfer, F. M. Mele, and J. Münch, (b,v)-type variables for black to white hole transitions in effective loop quantum gravity, Phys. Lett. B 819 (2021) 136390, [arXiv:1911.12646].
- [18] J. G. Kelly, R. Santacruz, and E. Wilson-Ewing, Effective loop quantum gravity framework for vacuum spherically symmetric spacetimes, Phys. Rev. D 102 (2020), no. 10 106024, [arXiv:2006.09302].
- [19] A. Parvizi, T. Pawlowski, Y. Tavakoli, and J. Lewandowski, Rainbow black hole from quantum gravitational collapse, Phys. Rev. D 105 (2022), no. 8 086002, [arXiv:2110.03069].
- [20] J. Lewandowski, Y. Ma, J. Yang, and C. Zhang, Quantum Oppenheimer-Snyder and Swiss Cheese Models, Phys. Rev. Lett. 130 (2023), no. 10 101501, [arXiv:2210.02253].
- [21] K. Giesel, M. Han, B.-F. Li, H. Liu, and P. Singh, Spherical symmetric gravitational collapse of a dust cloud: Polymerized dynamics in reduced phase space, Phys. Rev. D 107 (2023), no. 4 044047, [arXiv:2212.01930].
- [22] A. Alonso-Bardaji, D. Brizuela, and R. Vera, An effective model for the quantum Schwarzschild black hole, Phys. Lett. B 829 (2022) 137075, [arXiv:2112.12110].
- [23] A. Alonso-Bardaji, D. Brizuela, and R. Vera, Nonsingular spherically symmetric black-hole model with holonomy corrections, Phys. Rev. D 106 (2022), no. 2 024035, [arXiv:2205.02098].
- [24] C. Zhang, J. Lewandowski, Y. Ma, and J. Yang, Black Holes and Covariance in Effective Quantum Gravity, arXiv:2407.10168.
- [25] E. T. Newman and A. I. Janis, Note on the Kerr spinning particle metric, 1965.
- [26] M. Azreg-Aı̈nou, Generating rotating regular black hole solutions without complexification, Phys. Rev. D 90 (2014), no. 6 064041, [arXiv:1405.2569].
- [27] M. Azreg-Aı̈nou, From static to rotating to conformal static solutions: Rotating imperfect fluid wormholes with(out) electric or magnetic field, Eur. Phys. J. C 74 (2014), no. 5 2865, [arXiv:1401.4292].
- [28] F. Caravelli and L. Modesto, Spinning Loop Black Holes, Class. Quant. Grav. 27 (2010) 245022, [arXiv:1006.0232].
- [29] C. Liu, T. Zhu, Q. Wu, K. Jusufi, M. Jamil, M. Azreg-Aı̈nou, and A. Wang, Shadow and quasinormal modes of a rotating loop quantum black hole, Phys. Rev. D 101 (2020), no. 8 084001, [arXiv:2003.00477]. [Erratum: Phys.Rev.D 103, 089902 (2021)].
- [29] C. Liu, T. Zhu, Q. Wu, K. Jusufi, M. Jamil, M. Azreg-Aı̈nou, and A. Wang, Shadow and quasinormal modes of a rotating loop quantum black hole, Phys. Rev. D 101 (2020), no. 8 084001, [arXiv:2003.00477]. [Erratum: Phys.Rev.D 103, 089902 (2021)].
- [30] S. Brahma, C.-Y. Chen, and D.-h. Yeom, Testing Loop Quantum Gravity from Observational Consequences of Nonsingular Rotating Black Holes, Phys. Rev. Lett. 126 (2021), no. 18 181301, [arXiv:2012.08785].
- [31] C.-Y. Chen, On the possible spacetime structures of rotating loop quantum black holes, Int. J. Geom. Meth. Mod. Phys. 19 (2022), no. 11 2250176, [arXiv:2207.03797].
- [32] J. Kumar, S. U. Islam, and S. G. Ghosh, Loop Quantum Gravity motivated multihorizon rotating black holes, JCAP 11 (2022) 032, [arXiv:2209.13562].
- [33] Y. Huang and Z. Cao, Finite-distance gravitational deflection of massive particles by a rotating black hole in loop quantum gravity, Eur. Phys. J. C 83 (2023), no. 1 80, [arXiv:2212.04254].
- [34] F. Fazzini, Effective Kerr geometry from loop quantum gravity, Phys. Rev. D 111 (2025), no. 4 046025, [arXiv:2409.17099].
- [35] H. Ali, S. U. Islam, and S. G. Ghosh, Shadows and parameter estimation of rotating quantum corrected black holes and constraints from EHT observation of M87* and Sgr A*, JHEAp 47 (2025) 100367, [arXiv:2410.09198].
- [36] Z. Ban, J. Chen, and J. Yang, Shadows of rotating black holes in effective quantum gravity, Eur. Phys. J. C 85 (2025), no. 8 878, [arXiv:2411.09374].
- [37] A. Vachher and S. G. Ghosh, Strong gravitational lensing by rotating quantum-corrected black holes: Insights and constraints from EHT observations of M87* and Sgr A*, JHEAp 45 (2025) 75–86, [arXiv:2410.11332].
- [38] M. A. Raza, M. Zubair, F. Atamurotov, and A. Abdujabbarov, Influence of quantum correction on Kerr black hole in effective loop quantum gravity via shadows and EHT results, Eur. Phys. J. C 85 (2025), no. 9 973, [arXiv:2501.01308].
- [39] U. Fatima and G. Abbas, Penrose process in rotating black holes with quantum corrections: implications for energy extraction and irreducible mass, Eur. Phys. J. C 86 (2026), no. 2 166, [arXiv:2508.01683].
- [40] J.-N. Chen, Z.-K. Guo, and L.-B. Wu, The quasinormal modes of the rotating quantum corrected black holes, arXiv:2510.27320.
- [41] LIGO Scientific, Virgo Collaboration, B. P. Abbott et al., GW150914: The Advanced LIGO Detectors in the Era of First Discoveries, Phys. Rev. Lett. 116 (2016), no. 13 131103, [arXiv:1602.03838].
- [42] LIGO Scientific, Virgo Collaboration, B. P. Abbott et al., GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral, Phys. Rev. Lett. 119 (2017), no. 16 161101, [arXiv:1710.05832].
- [43] LIGO Scientific, Virgo Collaboration, B. P. Abbott et al., GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs, Phys. Rev. X 9 (2019), no. 3 031040, [arXiv:1811.12907].
- [44] LIGO Scientific, Virgo Collaboration, R. Abbott et al., GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run, Phys. Rev. X 11 (2021) 021053, [arXiv:2010.14527].
- [45] LIGO Scientific, VIRGO Collaboration, R. Abbott et al., GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run, Phys. Rev. D 109 (2024), no. 2 022001, [arXiv:2108.01045].
- [46] KAGRA, VIRGO, LIGO Scientific Collaboration, R. Abbott et al., GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run, Phys. Rev. X 13 (2023), no. 4 041039, [arXiv:2111.03606].
- [47] LISA Collaboration, P. Amaro-Seoane et al., Laser Interferometer Space Antenna, arXiv:1702.00786.
- [48] LISA Collaboration, M. Colpi et al., LISA Definition Study Report, arXiv:2402.07571.
- [49] TianQin Collaboration, J. Luo et al., TianQin: a space-borne gravitational wave detector, Class. Quant. Grav. 33 (2016), no. 3 035010, [arXiv:1512.02076].
- [50] TianQin Collaboration, J. Mei et al., The TianQin project: current progress on science and technology, PTEP 2021 (2021), no. 5 05A107, [arXiv:2008.10332].
- [51] Y. Gong, J. Luo, and B. Wang, Concepts and status of Chinese space gravitational wave detection projects, Nature Astron. 5 (2021), no. 9 881–889, [arXiv:2109.07442].
- [52] W.-R. Hu and Y.-L. Wu, The Taiji Program in Space for gravitational wave physics and the nature of gravity, Natl. Sci. Rev. 4 (2017), no. 5 685–686.
- [53] S. Babak, J. Gair, A. Sesana, E. Barausse, C. F. Sopuerta, C. P. L. Berry, E. Berti, P. Amaro-Seoane, A. Petiteau, and A. Klein, Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals, Phys. Rev. D 95 (2017), no. 10 103012, [arXiv:1703.09722].
- [54] J. R. Gair, L. Barack, T. Creighton, C. Cutler, S. L. Larson, E. S. Phinney, and M. Vallisneri, Event rate estimates for LISA extreme mass ratio capture sources, Class. Quant. Grav. 21 (2004) S1595–S1606, [gr-qc/0405137].
- [55] M. Mapelli, E. Ripamonti, A. Vecchio, A. W. Graham, and A. Gualandris, A cosmological view of extreme mass-ratio inspirals in nuclear star clusters, Astron. Astrophys. 542 (2012) A102, [arXiv:1205.2702].
- [56] P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals, Class. Quant. Grav. 24 (2007) R113–R169, [astro-ph/0703495].
- [57] L. Barack and C. Cutler, Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes, Phys. Rev. D 75 (2007) 042003, [gr-qc/0612029].
- [58] G. Fu, Y. Liu, B. Wang, J.-P. Wu, and C. Zhang, Probing quantum gravity effects with eccentric extreme mass-ratio inspirals, Phys. Rev. D 111 (2025), no. 8 084066, [arXiv:2409.08138].
- [59] T. Zi and S. Kumar, Eccentric extreme mass-ratio inspirals: a gateway to probe quantum gravity effects, Eur. Phys. J. C 85 (2025), no. 5 592, [arXiv:2409.17765].
- [60] Y. Liu and X. Zhang, Gravitational waves for eccentric extreme mass ratio inspirals of self-dual spacetime, JCAP 10 (2024) 056, [arXiv:2404.08454].
- [61] S. Yang, Y.-P. Zhang, L. Zhao, and Y.-X. Liu, Constraints on quantum Oppenheimer-Snyder black holes with eccentric extreme mass-ratio inspirals, arXiv:2509.24835.
- [62] F. Ahmed, Q. Wu, S. G. Ghosh, and T. Zhu, Signatures of Quantum-Corrected Black Holes in Gravitational Waves from Periodic Orbits, arXiv:2512.24036.
- [63] H. Gong, S. Long, X.-J. Wang, Z. Xia, J.-P. Wu, and Q. Pan, Gravitational waveforms from periodic orbits around a novel regular black hole, arXiv:2509.23318.
- [64] R.-T. Chen, G. Fu, D. Zhang, and J.-P. Wu, Imprints of quantum gravity effects on gravitational waves: a comparative study using extreme mass-ratio inspirals, arXiv:2601.00185.
- [65] D. Zhang, C. Zhang, Q. Pan, G. Fu, and J.-P. Wu, Probing Quantum Gravity effects with Extreme Mass Ratio Inspirals around Rotating Hayward Black Holes, arXiv:2602.07436.
- [66] A. J. K. Chua, M. L. Katz, N. Warburton, and S. A. Hughes, Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis, Phys. Rev. Lett. 126 (2021), no. 5 051102, [arXiv:2008.06071].
- [67] M. L. Katz, A. J. K. Chua, L. Speri, N. Warburton, and S. A. Hughes, Fast extreme-mass-ratio-inspiral waveforms: New tools for millihertz gravitational-wave data analysis, Phys. Rev. D 104 (2021), no. 6 064047, [arXiv:2104.04582].
- [68] K. S. Thorne, Multipole Expansions of Gravitational Radiation, Rev. Mod. Phys. 52 (1980) 299–339.
- [69] F. D. Ryan, Effect of gravitational radiation reaction on circular orbits around a spinning black hole, Phys. Rev. D 52 (1995) R3159–R3162, [gr-qc/9506023].
- [70] P. C. Peters and J. Mathews, Gravitational radiation from point masses in a Keplerian orbit, Phys. Rev. 131 (1963) 435–439.
- [71] C. Cutler, D. Kennefick, and E. Poisson, Gravitational radiation reaction for bound motion around a Schwarzschild black hole, Phys. Rev. D 50 (1994) 3816–3835.
- [72] K. Glampedakis and D. Kennefick, Zoom and whirl: Eccentric equatorial orbits around spinning black holes and their evolution under gravitational radiation reaction, Phys. Rev. D 66 (2002) 044002, [gr-qc/0203086].
- [73] P. Gupta, B. Bonga, A. J. K. Chua, and T. Tanaka, Importance of tidal resonances in extreme-mass-ratio inspirals, Phys. Rev. D 104 (2021), no. 4 044056, [arXiv:2104.03422].
- [74] B. Bonga, H. Yang, and S. A. Hughes, Tidal resonance in extreme mass-ratio inspirals, Phys. Rev. Lett. 123 (2019), no. 10 101103, [arXiv:1905.00030].
- [75] A. J. K. Chua, C. J. Moore, and J. R. Gair, Augmented kludge waveforms for detecting extreme-mass-ratio inspirals, Phys. Rev. D 96 (2017), no. 4 044005, [arXiv:1705.04259].
- [76] L. Barack and C. Cutler, Lisa capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy, Phys. Rev. D 69 (Apr, 2004) 082005.
- [77] A. J. K. Chua and J. R. Gair, Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis, Class. Quant. Grav. 32 (2015) 232002, [arXiv:1510.06245].
- [78] T. Robson, N. J. Cornish, and C. Liu, The construction and use of LISA sensitivity curves, Class. Quant. Grav. 36 (2019), no. 10 105011, [arXiv:1803.01944].
- [79] K. Chatziioannou, A. Klein, N. Yunes, and N. Cornish, Constructing Gravitational Waves from Generic Spin-Precessing Compact Binary Inspirals, Phys. Rev. D 95 (2017), no. 10 104004, [arXiv:1703.03967].