Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Letter
  • Open Access

Thermonuclear diversity and the Hubble tension

Richard S. Miller*

  • *Contact author: Richard.S.Miller@jhuapl.edu

Phys. Rev. D 111, L081305 – Published 23 April, 2025

DOI: https://doi.org/10.1103/PhysRevD.111.L081305

Abstract

Homogeneity is the hallmark of standard candle-based cosmology investigations. Thermonuclear supernovae (Type-Ia, SNeIa) violate this essential requirement if they develop along multiple evolutionary pathways. In this work, the impact of thermonuclear diversity on cosmological parameter constraints is quantified using Pantheon+, one of the largest ensembles of SNeIa compiled to probe cosmology to date. Evidence of diversity is encoded in supernova light curves. Pantheon+ is shown to be diverse, with features indicative of multiple thermonuclear subclasses. Diversity driven systematic effects have been quantified on a supernova-by-supernova basis; event selections based on light curve derived metrics were subsequently used to characterize diversity dependent trends and limit their impact. A diversity mitigated estimate of the Hubble-Lemaître parameter, H0=67.9±0.8  km s−1 Mpc−1 (68% C.L.), was obtained by reanalyzing Pantheon+. The Hubble tension, an apparent disparity between early and late Universe determinations of H0, is eased from ∼5σ to <1σ after accounting for the diverse thermonuclear scenarios that govern SNeIa. Diversity mitigated subsets of Pantheon+ also show a ∼3.4σ preference for a flat w0waCDM cosmology with dark energy equation of state parameters (w0,wa)=(−1.084±0.180,−2.066±0.675). A strategy for precise SNeIa-derived cosmological inferences, dominated by statistical rather than systematic uncertainties, is also presented.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (70)

  1. A. G. Riess et al., Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116, 1009 (1998).
  2. S. Perlmutter et al., Measurements of Ω and Λ from 42 high-redshift supernovae, Astrophys. J. 517, 565 (1999).
  3. A. Goobar and B. Leibundgut, Supernova cosmology: Legacy and future, Annu. Rev. Nucl. Part. Sci. 61, 251 (2011).
  4. K. Nomoto, F. K. Thielemann, and K. Yokoi, Accreting white dwarf models for type I supern. III. Carbon deflagration supernovae, Astrophys. J. 286, 644 (1984).
  5. P. Höflich, Physics of type Ia supernovae, Nucl. Phys. A777, 579 (2006).
  6. W. Hillebrandt and J. C. Niemeyer, Type IA supernova explosion models, Annu. Rev. Astron. Astrophys. 38, 191 (2000).
  7. D. Maoz, F. Mannucci, and G. Nelemans, Observational clues to the progenitors of type Ia supernovae, Annu. Rev. Astron. Astrophys. 52, 107 (2014).
  8. National Research Council, New Worlds, New Horizons in Astronomy and Astrophysics (The National Academies Press, Washington, DC, 2010).
  9. National Academies of Sciences, Engineering, and Medicine, Pathways to Discovery in Astronomy and Astrophysics for the 2020s (The National Academies Press, Washington, DC, 2023).
  10. M. M. Phillips, The absolute magnitudes of type IA supernovae, Astrophys. J. Lett. 413, L105 (1993).
  11. J. Guy et al., SALT2: Using distant supernovae to improve the use of type Ia supernovae as distance indicators, Astron. Astrophys. 466, 11 (2007).
  12. W. L. Freedman, Measurements of the Hubble constant: Tensions in perspective, Astrophys. J. 919, 16 (2021).
  13. E. Di Valentino, O. Mena, S. Pan, L. Visinelli, W. Yang, A. Melchiorri, D. F. Mota, A. G. Riess, and J. Silk, In the realm of the Hubble tension-A review of solutions, Classical Quantum Gravity 38, 153001 (2021).
  14. M. Kamionkowski and A. G. Riess, The Hubble tension and early dark energy, Annu. Rev. Nucl. Part. Sci. 73, 153 (2023).
  15. E. Abdalla et al., Cosmology intertwined: A review of the particle physicsastrophysics, and cosmology associated with the cosmological tensions and anomalies, J. High Energy Astrophys. 34, 49 (2022).
  16. L. Perivolaropoulos and F. Skara, Challenges for ΛCDM: An update, New Astron. Rev. 95, 101659 (2022).
  17. N. Aghanim et al., Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641, A6 (2020).
  18. D. Brout et al., The Pantheon+ analysis: Cosmological constraints, Astrophys. J. 938, 110 (2022).
  19. L.-S. The and A. Burrows, Expectations for the hard x-ray continuum and gamma-ray line fluxes from the type Ia supernova SN 2014J in M82, Astrophys. J. 786, 141 (2014).
  20. I. R. Seitenzahl and D. M. Townsley, Nucleosynthesis in thermonuclear supernovae, in Handbook of Supernovae, edited by A. W. Alsabti and P. Murdin (Springer International Publishing, Cham, Switzerland, 2017), p. 1955.
  21. D. D. Clayton, S. A. Colgate, and G. J. Fishman, Gamma-ray lines from young supernova remnants, Astrophys. J. 155, 75 (1969).
  22. S. A. Sim and P. A. Mazzali, On the γ-ray emission of type Ia supernovae, Mon. Not. R. Astron. Soc. 385, 1681 (2008).
  23. F. H. Panther, I. R. Seitenzahl, A. J. Ruiter, T. Siegert, S. Sim, and R. M. Crocker, Prospects of direct detection of V48 gamma-rays from thermonuclear supernovae, Mon. Not. R. Astron. Soc. 508, 1590 (2021).
  24. A. Summa, A. Ulyanov, M. Kromer, S. Boyer, F. K. Röpke, S. A. Sim, I. R. Seitenzahl, M. Fink, K. Mannheim, R. Pakmor, F. Ciaraldi-Schoolmann, R. Diehl, K. Maeda, and W. Hillebrandt, Gamma-ray diagnostics of type Ia supernovae. Predictions of observables from three-dimensional modeling, Astron. Astrophys. 554, A67 (2013).
  25. R. Diehl, T. Siegert, W. Hillebrandt, S. A. Grebenev, J. Greiner, M. Krause, M. Kromer, K. Maeda, F. Röpke, and S. Taubenberger, Early Ni56 decay gamma rays from SN2014J suggest an unusual explosion, Science 345, 1162 (2014).
  26. E. Churazov, R. Sunyaev, J. Isern, J. Knödlseder, P. Jean, F. Lebrun, N. Chugai, S. Grebenev, E. Bravo, S. Sazonov, and M. Renaud, Cobalt-56γ-ray emission lines from the type Ia supernova 2014J, Nature (London) 512, 406 (2014).
  27. E. Churazov, R. Sunyaev, J. Isern, I. Bikmaev, E. Bravo, N. Chugai, S. Grebenev, P. Jean, J. Knödlseder, F. Lebrun, and E. Kuulkers, Gamma-rays from type Ia supernova SN2014J, Astrophys. J. 812, 62 (2015).
  28. J. Isern et al., Gamma-ray emission from SN2014J near maximum optical light, Astron. Astrophys. 588, A67 (2016).
  29. S. A. Colgate and C. McKee, Early supernova luminosity, Astrophys. J. 157, 623 (1969).
  30. K. S. Mandel, D. M. Scolnic, H. Shariff, R. J. Foley, and R. P. Kirshner, The type Ia supernova color-magnitude relation and host galaxy dust: A simple hierarchical Bayesian model, Astrophys. J. 842, 93 (2017).
  31. P. Clark, K. Maguire, M. Bulla, L. Galbany, M. Sullivan, J. P. Anderson, and S. J. Smartt, Probing the progenitors of type Ia supernovae using circumstellar material interaction signatures, Mon. Not. R. Astron. Soc. 507, 4367 (2021).
  32. W. D. Arnett, On the theory of type I supernovae, Astrophys. J. Lett. 230, L37 (1979).
  33. W. D. Arnett, Type I supernovae. I—Analytic solutions for the early part of the light curve, Astrophys. J. 253, 785 (1982).
  34. W. D. Arnett, D. Branch, and J. C. Wheeler, Hubble’s constant and exploding carbon-oxygen white dwarf models for type I supernovae, Nature (London) 314, 337 (1985).
  35. A. Khokhlov, E. Mueller, and P. Hoeflich, Light curves of type IA supernova models with different explosion mechanisms, Astron. Astrophys. 270, 223 (1993), https://articles.adsabs.harvard.edu/pdf/1993A%26A...270..223K.
  36. M. Stritzinger, P. A. Mazzali, J. Sollerman, and S. Benetti, Consistent estimates of Ni56 yields for type Ia supernovae, Astron. Astrophys. 460, 793 (2006).
  37. S. Blondin, L. Dessart, D. J. Hillier, and A. M. Khokhlov, One-dimensional delayed-detonation models of type Ia supernovae: Confrontation to observations at bolometric maximum, Mon. Not. R. Astron. Soc. 429, 2127 (2013).
  38. R. Scalzo et al., Type Ia supernova bolometric light curves and ejected mass estimates from the nearby supernova factory, Mon. Not. R. Astron. Soc. 440, 1498 (2014).
  39. S. Dhawan, B. Leibundgut, J. Spyromilio, and S. Blondin, A reddening-free method to estimate the Ni56 mass of type Ia supernovae, Astron. Astrophys. 588, A84 (2016).
  40. P. Hoeflich, E. Y. Hsiao, C. Ashall, C. R. Burns, T. R. Diamond, M. M. Phillips, D. Sand, M. D. Stritzinger, N. Suntzeff, C. Contreras, K. Krisciunas, N. Morrell, and L. Wang, Light and color curve properties of type Ia supernovae: Theory versus observations, Astrophys. J. 846, 58 (2017).
  41. T. Sukhbold, Properties of type-Ia supernova light curves, Astrophys. J. 874, 62 (2019).
  42. D. K. Khatami and D. N. Kasen, Physics of luminous transient light curves: A new relation between peak time and luminosity, Astrophys. J. 878, 56 (2019).
  43. D. Brout, G. Taylor, D. Scolnic, C. M. Wood, B. M. Rose, M. Vincenzi, A. Dwomoh, C. Lidman, A. Riess, N. Ali, H. Qu, and M. Dai, The Pantheon+ analysis: SuperCal-fragilistic cross calibration, retrained SALT2 light-curve model, and calibration systematic uncertainty, Astrophys. J. 938, 111 (2022).
  44. D. Scolnic Brown et al., The Pantheon+ analysis: The full data set and light-curve release, Astrophys. J. 938, 113 (2022).
  45. https://github.com/PantheonPlusSH0ES/DataRelease
  46. J. P. Norris, J. T. Bonnell, D. Kazanas, J. D. Scargle, J. Hakkila, and T. W. Giblin, Long-lag, wide-pulse gamma-ray bursts, Astrophys. J. 627, 324 (2005).
  47. R. J. Nemiroff, Extension of an exponential light-curve gamma-ray burst pulse model across energy bands, Mon. Not. R. Astron. Soc. 419, 1650 (2012).
  48. D. Scolnic et al., Supernova siblings: Assessing the consistency of properties of type Ia supernovae that share the same parent galaxies, Astrophys. J. Lett. 896, L13 (2020).
  49. P. Astier et al., The supernova legacy Survey: Measurement of ΩM, ΩΛ and w from the first year data set, Astron. Astrophys. 447, 31 (2006).
  50. A. Conley et al., Supernova constraints and systematic uncertainties from the first three years of the supernova legacy survey, Astrophys. J. Suppl. Ser. 192, 1 (2011).
  51. T. M. C. Abbott et al. (DES Collaboration), The Dark Energy Survey: Cosmology results with ∼1500 new high-redshift type Ia supernovae using the full 5-year dataset, Astrophys. J. Lett. 973, L14 (2024).
  52. R. Tripp, A two-parameter luminosity correction for type IA supernovae, Astron. Astrophys. 331, 815 (1998).
  53. A. G. Riess et al., A comprehensive measurement of the local value of the Hubble constant with 1  km s−1 Mpc−1 uncertainty from the Hubble Space Telescope and the SH0ES Team, Astrophys. J. Lett. 934, L7 (2022).
  54. P. J. E. Peebles, Principles of Physical Cosmology (Princeton University Press, Princeton, NJ, 1993).
  55. D. W. Hogg, Distance measures in cosmology, arXiv:astro-ph/9905116.
  56. M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter, Int. J. Mod. Phys. D 10, 213 (2001).
  57. E. V. Linder, Exploring the expansion history of the universe, Phys. Rev. Lett. 90, 091301 (2003).
  58. W. J. Handley, M. P. Hobson, and A. N. Lasenby, POLYCHORD: Next-generation nested sampling, Mon. Not. R. Astron. Soc. 453, 4384 (2015).
  59. J. Zuntz, M. Paterno, E. Jennings, D. Rudd, A. Manzotti, S. Dodelson, S. Bridle, S. Sehrish, and J. Kowalkowski, cosmosis: Modular cosmological parameter estimation, Astron. Comput. 12, 45 (2015).
  60. A. G. Adame et al. (DESI Collaboration), DESI 2024 VI: Cosmological constraints from the measurements of baryon acoustic oscillations, J. Cosmol. Astropart. Phys. 02 (2025) 021.
  61. J. P. Blakeslee, J. B. Jensen, C.-P. Ma, P. A. Milne, and J. E. Greene, The Hubble constant from infrared surface brightness fluctuation distances, Astrophys. J. 911, 65 (2021).
  62. W. L. Freedman, B. F. Madore, I. S. Jang, T. J. Hoyt, A. J. Lee, and K. A. Owens, Status report on the Chicago-Carnegie Hubble Program (CCHP): Three independent astrophysical determinations of the Hubble constant using the James Webb Space Telescope, arXiv:2408.06153.
  63. P. L. Kelly et al., Constraints on the Hubble constant from supernova Refsdal’s reappearance, Science 380, abh1322 (2023).
  64. W. L. Freedman et al., The Carnegie-Chicago Hubble Program. VIII. An independent determination of the Hubble constant based on the tip of the red giant branch, Astrophys. J. 882, 34 (2019).
  65. W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee, A. Monson, J. Neeley, and J. Rich, Calibration of the tip of the red giant branch, Astrophys. J. 891, 57 (2020).
  66. J. Carron, M. Mirmelstein, and A. Lewis, CMB lensing from Planck PR4 maps, J. Cosmol. Astropart. Phys. 09 (2022) 039.
  67. M. S. Madhavacheril et al., The Atacama Cosmology Telescope: DR6 gravitational lensing map and cosmological parameters, Astrophys. J. 962, 113 (2024).
  68. F. J. Qu et al., The Atacama Cosmology Telescope: A measurement of the DR6 CMB lensing power spectrum and its implications for structure growth, Astrophys. J. 962, 112 (2024).
  69. N. MacCrann et al., The Atacama Cosmology Telescope: Mitigating the impact of extragalactic foregrounds for the DR6 cosmic microwave background lensing analysis, Astrophys. J. 966, 138 (2024).
  70. P. A. Abell et al. (LSST Science Collaboration), LSST science book, version 2.0, arXiv:0912.0201.

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation