Implications of GW241011 for rotating exotic compact objects Article Swipe

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N. V. Krishnendu , Tamara Evstafyeva , A. Vijaykumar , William E. East , Ranjana Das , Nils Siemonsen , N. Uchikata , Poulami Dutta Roy , Pawan Kumar Gupta , Syed Naqvi , E. M. Sänger , Pratyusava Baral , Sajad A. Bhat , T. A. Callister , M. Emma , C.‐J. Haster ·

YOU? · · 2025 · Open Access · · DOI: https://doi.org/10.48550/arxiv.2511.17341

A number of theoretical proposals have been made for horizonless compact objects with masses and spins similar to those of black holes. While gravitational wave signatures from their mergers can resemble those of black holes, features like the spin-induced quadrupole moment may reveal their distinct nature. Using the tight bounds on the spin-induced quadrupole moment of GW241011, we place gravitational wave constraints on the nature of its primary. We find that large classes of exotic compact objects (including rotating boson stars) cannot explain its nature, however, models of sufficiently large compactness of $C \gtrsim 0.24$ may still be viable contenders.

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Type: preprint
Landing Page: http://arxiv.org/abs/2511.17341
PDF: https://arxiv.org/pdf/2511.17341
OA Status: green
OpenAlex ID: https://openalex.org/W4416667793

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DOI: https://doi.org/10.48550/arxiv.2511.17341

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Title: Implications of GW241011 for rotating exotic compact objects

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Type: preprint

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Publication year: 2025

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Publication date: 2025-11-21

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Authors: N. V. Krishnendu, Tamara Evstafyeva, A. Vijaykumar, William E. East, Ranjana Das, Nils Siemonsen, N. Uchikata, Poulami Dutta Roy, Pawan Kumar Gupta, Syed Naqvi, E. M. Sänger, Pratyusava Baral, Sajad A. Bhat, T. A. Callister, M. Emma, C.‐J. Haster

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Landing page: https://arxiv.org/abs/2511.17341

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PDF URL: https://arxiv.org/pdf/2511.17341

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Cited by: 0

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