Search: onr:"swepub:oai:DiVA.org:su-227679" >
Leveraging SN Ia sp...
Leveraging SN Ia spectroscopic similarity to improve the measurement of H0
-
Murakami, Yukei S. (author)
-
Riess, Adam G. (author)
-
Stahl, Benjamin E. (author)
-
show more...
-
- Kenworthy, William D'Arcy, 1995- (author)
- Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
-
Pluck, Dahne-More A. (author)
-
Macoretta, Antonella (author)
-
Brout, Dillon (author)
-
Jones, David O. (author)
-
Scolnic, Dan M. (author)
-
Filippenko, Alexei V. (author)
-
show less...
-
(creator_code:org_t)
- 2023
- 2023
- English.
-
In: Journal of Cosmology and Astroparticle Physics. - 1475-7516. ; 2023:11
- Related links:
-
https://doi.org/10.1...
-
show more...
-
https://urn.kb.se/re...
-
https://doi.org/10.1...
-
show less...
Abstract
Subject headings
Close
- Recent studies suggest spectroscopic differences explain a fraction of the variation in Type Ia supernova (SN Ia) luminosities after light-curve/color standardization. In this work, (i) we empirically characterize the variations of standardized SN Ia luminosities, and (ii) we use a spectroscopically inferred parameter, SIP, to improve the precision of SNe Ia along the distance ladder and the determination of the Hubble constant (H0). First, we show that thePantheon+ covariance model modestly overestimates the uncertainty of standardized magnitudes by ∼ 7%, in the parameter space used by the SH0ES Team to measure H0; accounting for this alone yields H0 = 73.01 ± 0.92 km s-1 Mpc-1. Furthermore, accounting for spectroscopic similarity between SNe Ia on the distance ladder reduces their relative scatter to ∼ 0.12 mag per object (compared to ∼ 0.14 mag previously). Combining these two findings in the model of SN covariance, we find an overall 14% reduction (to ± 0.85 km s-1 Mpc-1) of the uncertainty in the Hubble constant and a modest increase in its value. Including a budget for systematic uncertainties itemized by Riess et al. (2022a), we report an updated local Hubble constant with ∼ 1.2% uncertainty, H0 = 73.29 ± 0.90 km s-1 Mpc-1. We conclude that spectroscopic differences among photometrically standardized SNe Ia do not explain the "Hubble tension". Rather, accounting for such differences increases its significance, as the discrepancy against ΛCDM calibrated by the Planck 2018 measurement rises to 5.7σ.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- cosmological parameters from CMBR
- cosmological parameters from distance ladder
- supernova type Ia - standard candles
Publication and Content Type
- ref (subject category)
- art (subject category)
Find in a library
To the university's database
- By the author/editor
-
Murakami, Yukei ...
-
Riess, Adam G.
-
Stahl, Benjamin ...
-
Kenworthy, Willi ...
-
Pluck, Dahne-Mor ...
-
Macoretta, Anton ...
-
show more...
-
Brout, Dillon
-
Jones, David O.
-
Scolnic, Dan M.
-
Filippenko, Alex ...
-
show less...
- About the subject
-
- NATURAL SCIENCES
-
NATURAL SCIENCES
-
and Physical Science ...
-
and Astronomy Astrop ...
- Articles in the publication
-
Journal of Cosmo ...
- By the university
-
Stockholm University