- Open Access
Effective Field Theory Constraints on Primordial Black Holes from the High-Redshift Lyman- Forest
Phys. Rev. Lett. 136, 171402 – Published 29 April, 2026
DOI: https://doi.org/10.1103/8g8z-bmxd
Abstract
We present updated constraints on the abundance of primordial black hole (PBH) dark matter from the high-redshift Lyman- forest data from MIKE/HIRES experiments. Our analysis leverages an effective field theory (EFT) description of the 1D flux power spectrum, allowing us to analytically predict the Lyman- fluctuations on quasilinear scales from first principles. Our EFT-based likelihood enables robust inference across redshifts and down to scales of 100 kpc, within previously unexplored regions of parameter space for this dataset. We derive new bounds on the PBH fraction with respect to the total dark matter , excluding populations with for masses . This offers the leading constraint for PBHs heavier than and highlights the Lyman- forest as a uniquely sensitive probe of new physics models that modify the structure formation history of our Universe.
Physics Subject Headings (PhySH)
Article Text
Supplemental Material
References (86)
- C. S. Frenk and S. D. M. White, Ann. Phys. (Berlin) 524, 507 (2012).
- B. A. Reid et al., Mon. Not. R. Astron. Soc. 404, 60 (2010).
- N. Banik, J. Bovy, G. Bertone, D. Erkal, and T. J. L. de Boer, J. Cosmol. Astropart. Phys. 10 (2021) 043.
- T. M. C. Abbott et al. (DES Collaboration), Phys. Rev. D 105, 023520 (2022).
- N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A1 (2020).
- N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020).
- K. N. Abazajian et al. (CMB-S4 Collaboration), arXiv:1610.02743.
- M. R. Buckley, P. Du, N. Fernandez, and M. J. Weikert, J. Cosmol. Astropart. Phys. 12 (2025) 006.
- S. Chabanier, M. Millea, and N. Palanque-Delabrouille, Mon. Not. R. Astron. Soc. 489, 2247 (2019).
- N. Sabti, J. B. Muñoz, and D. Blas, Astrophys. J. Lett. 928, L20 (2022).
- T. Kobayashi, R. Murgia, A. De Simone, V. Iršič, and M. Viel, Phys. Rev. D 96, 123514 (2017).
- V. Iršič, H. Xiao, and M. McQuinn, Phys. Rev. D 101, 123518 (2020).
- M. Feix, J. Frank, A. Pargner, R. Reischke, B. M. Schäfer, and T. Schwetz, J. Cosmol. Astropart. Phys. 05 (2019) 021.
- M. Feix, S. Hagstotz, A. Pargner, R. Reischke, B. M. Schäfer, and T. Schwetz, J. Cosmol. Astropart. Phys. 11 (2020) 046.
- R. T. Co, D. Dunsky, N. Fernandez, A. Ghalsasi, L. J. Hall, K. Harigaya, and J. Shelton, J. High Energy Phys. 09 (2022) 116.
- G. Hütsi, M. Raidal, J. Urrutia, V. Vaskonen, and H. Veermäe, Phys. Rev. D 107, 043502 (2023).
- M. Gorghetto and E. Hardy, J. High Energy Phys. 05 (2023) 030.
- S. Bird, C.-F. Chang, Y. Cui, and D. Yang, Phys. Lett. B 858, 139062 (2024).
- H. Winch, K. K. Rogers, R. Hložek, and D. J. E. Marsh, Astrophys. J. 976, 40 (2024).
- J. Ellis, M. Fairbairn, J. Urrutia, and V. Vaskonen, Astron. Astrophys. 702, A109 (2025).
- N. Afshordi, P. McDonald, and D. N. Spergel, Astrophys. J. Lett. 594, L71 (2003).
- B. Carr and J. Silk, Mon. Not. R. Astron. Soc. 478, 3756 (2018).
- D. Inman and Y. Ali-Haïmoud, Phys. Rev. D 100, 083528 (2019).
- R. Murgia, G. Scelfo, M. Viel, and A. Raccanelli, Phys. Rev. Lett. 123, 071102 (2019).
- B. Liu and V. Bromm, Astrophys. J. Lett. 937, L30 (2022).
- Y. Gouttenoire, S. Trifinopoulos, G. Valogiannis, and M. Vanvlasselaer, Phys. Rev. D 109, 123002 (2024).
- N. K. Khan, A. Ray, G. Kulkarni, and B. Dasgupta, Phys. Rev. D 112, 123019 (2025).
- S. Hawking, Mon. Not. R. Astron. Soc. 152, 75 (1971).
- B. Carr, K. Kohri, Y. Sendouda, and J. Yokoyama, Rep. Prog. Phys. 84 (2021) 116902.
- R. Bean and J. Magueijo, Phys. Rev. D 66, 063505 (2002).
- M. Kawasaki, A. Kusenko, and T. T. Yanagida, Phys. Lett. B 711, 1 (2012).
- Y. Ali-Haïmoud and M. Kamionkowski, Phys. Rev. D 95, 043534 (2017).
- S. Clesse and J. García-Bellido, Phys. Dark Universe 15, 142 (2017).
- S. Clesse and J. García-Bellido, Phys. Dark Universe 22, 137 (2018).
- P. D. Serpico, V. Poulin, D. Inman, and K. Kohri, Phys. Rev. Res. 2, 023204 (2020).
- T. Nakama, T. Suyama, and J. Yokoyama, Phys. Rev. D 94, 103522 (2016).
- T. Nakama, B. Carr, and J. Silk, Phys. Rev. D 97, 043525 (2018).
- P. Meszaros, Astron. Astrophys. 37, 225 (1974), https://ui.adsabs.harvard.edu/abs/1974A%26A....37..225M.
- B. J. Carr, Astrophys. J. 201, 1 (1975).
- M. Sasaki, T. Suyama, T. Tanaka, and S. Yokoyama, Classical Quantum Gravity 35, 063001 (2018).
- V. Atal, A. Sanglas, and N. Triantafyllou, J. Cosmol. Astropart. Phys. 06 (2021) 022.
- P. F. Depta, K. Schmidt-Hoberg, P. Schwaller, and C. Tasillo, Phys. Rev. Res. 7, 013196 (2025).
- B. Carr, F. Kuhnel, and L. Visinelli, Mon. Not. R. Astron. Soc. 501, 2029 (2021).
- M. M. Ivanov, Phys. Rev. D 109, 023507 (2024).
- M. Garny, T. Konstandin, L. Sagunski, and S. Tulin, J. Cosmol. Astropart. Phys. 09 (2018) 011.
- M. Garny, T. Konstandin, L. Sagunski, and M. Viel, J. Cosmol. Astropart. Phys. 03 (2021) 049.
- S.-F. Chen, Z. Vlah, and M. White, J. Cosmol. Astropart. Phys. 05 (2021) 053.
- M. M. Ivanov, M. W. Toomey, and N. G. Karaçayl𝚤, Phys. Rev. Lett. 134, 091001 (2025).
- R. de Belsunce, S.-F. Chen, M. M. Ivanov, C. Ravoux, S. Chabanier, J. Sexton, and Z. Lukic, Phys. Rev. D 111, 063524 (2025).
- A. Chudaykin and M. M. Ivanov, Phys. Rev. D 111, 083515 (2025).
- A. He, M. M. Ivanov, S. Bird, R. An, and V. Gluscevic, Phys. Rev. D 112, 063540 (2025).
- R. de Belsunce, M. M. Ivanov, J. M. Sullivan, K. Akitsu, and S.-F. Chen, Phys. Rev. Lett. 136, 101001 (2026).
- R. de Belsunce, J. M. Sullivan, and P. McDonald, Phys. Rev. D 113, 063550 (2026).
- V. Desjacques, D. Jeong, and F. Schmidt, Phys. Rep. 733, 1 (2018).
- M. M. Ivanov, M. Simonović, and M. Zaldarriaga, J. Cosmol. Astropart. Phys. 05 (2020) 042.
- M. M. Ivanov, Effective Field Theory for Large-Scale Structure (Springer, Singapore, 2023).
- B. J. Carr and S. W. Hawking, Mon. Not. R. Astron. Soc. 168, 399 (1974).
- V. De Luca, V. Desjacques, G. Franciolini, and A. Riotto, J. Cosmol. Astropart. Phys. 11 (2020) 028.
- M. Viel, G. D. Becker, J. S. Bolton, and M. G. Haehnelt, Phys. Rev. D 88, 043502 (2013).
- M. Esposito, V. Iršič, M. Costanzi, S. Borgani, A. Saro, and M. Viel, Mon. Not. R. Astron. Soc. 515, 857 (2022).
- See Supplemental Material at http://link.aps.org/supplemental/10.1103/8g8z-bmxd for data combination, EFT modeling details, best-fit comparisons, and a discussion of isocurvature bias.
- A. Barreira, G. Cabass, D. Nelson, and F. Schmidt, J. Cosmol. Astropart. Phys. 02 (2020) 005.
- B. Villasenor, B. Robertson, P. Madau, and E. Schneider, Phys. Rev. D 108, 023502 (2023).
- P. Montero-Camacho, C. M. Hirata, P. Martini, and K. Honscheid, Mon. Not. R. Astron. Soc. 487, 1047 (2019).
- N. Kaiser, Mon. Not. R. Astron. Soc. 227, 1 (1987).
- S. Chabanier, C. Ravoux, L. Latrille, J. Sexton, É. Armengaud, J. Bautista, T. Dumerchat, and Z. Lukić, Mon. Not. R. Astron. Soc. 534, 2674 (2024).
- B. Hadzhiyska, R. de Belsunce, A. Cuceu, J. Guy, M. M. Ivanov, H. Coquinot, and A. Font-Ribera, Mon. Not. R. Astron. Soc. 540, 1960 (2025).
- T. Brinckmann and J. Lesgourgues, Phys. Dark Universe 24, 100260 (2019).
- B. Audren, J. Lesgourgues, K. Benabed, and S. Prunet, J. Cosmol. Astropart. Phys. 02 (2013) 001.
- A. Chudaykin, M. M. Ivanov, O. H. E. Philcox, and M. Simonović, Phys. Rev. D 102, 063533 (2020).
- S. Chabanier et al. (eBOSS Collaboration), J. Cosmol. Astropart. Phys. 07 (2019) 017.
- A. G. Adame et al. (DESI Collaboration), J. Cosmol. Astropart. Phys. 07 (2025) 028.
- A. Chudaykin, M. M. Ivanov, and O. H. E. Philcox, Phys. Rev. D 113, 063502 (2026).
Notice that the CMB spectral -distortion bounds can be relaxed by introducing non-Gaussianities in the probability distribution of the primordial curvature perturbations [37].
- Y. Inoue and A. Kusenko, J. Cosmol. Astropart. Phys. 10 (2017) 034.
- P. N. Wilkinson, D. R. Henstock, I. W. A. Browne, A. G. Polatidis, P. Augusto, A. C. S. Readhead, T. J. Pearson, W. Xu, G. B. Taylor, and R. C. Vermeulen, Phys. Rev. Lett. 86, 584 (2001).
- B. J. Carr and M. Sakellariadou, Astrophys. J. 516, 195 (1999).
- N. Sabti, J. B. Muñoz, and M. Kamionkowski, Phys. Rev. Lett. 132, 061002 (2024).
- K. Kohri, T. Nakama, and T. Suyama, Phys. Rev. D 90, 083514 (2014).
- M. Levi, C. Bebek, T. Beers, R. Blum, R. Cahn, D. Eisenstein, B. Flaugher, K. Honscheid, R. Kron, O. Lahav, P. McDonald, N. Roe, and D. Schlegel (Representing the DESI Collaboration), arXiv:1308.0847.
- R. Besuner et al. (Spec-S5 Collaboration), arXiv:2503.07923.
- R. Laureijs et al. (EUCLID Collaboration), arXiv:1110.3193.
- A. Abate et al. (LSST Dark Energy Science Collaboration), arXiv:1211.0310.
- J. B. Muñoz, C. Dvorkin, and F.-Y. Cyr-Racine, Phys. Rev. D 101, 063526 (2020).
- I. Labbé, P. van Dokkum, E. Nelson, R. Bezanson, K. A. Suess, J. Leja, G. Brammer, K. Whitaker, E. Mathews, M. Stefanon, and B. Wang, Nature (London) 616, 266 (2023).
- M. Xiao et al., Nature (London) 635, 311 (2024).