The Unsettled Number: Hubble’s Tension

One of main sources of uncertainty in modern cosmology is the present rate of the universe’s expansion, H<sub>0</sub>, called the Hubble constant. Once again, different observational techniques bring about different results, causing new “Hubble tension”. In the present work, we review th...

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Main Authors: Jorge L. Cervantes-Cota, Salvador Galindo-Uribarri, George F. Smoot
Format: Article
Language:English
Published: MDPI AG 2023-11-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/9/12/501
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author Jorge L. Cervantes-Cota
Salvador Galindo-Uribarri
George F. Smoot
author_facet Jorge L. Cervantes-Cota
Salvador Galindo-Uribarri
George F. Smoot
author_sort Jorge L. Cervantes-Cota
collection DOAJ
description One of main sources of uncertainty in modern cosmology is the present rate of the universe’s expansion, H<sub>0</sub>, called the Hubble constant. Once again, different observational techniques bring about different results, causing new “Hubble tension”. In the present work, we review the historical roots of the Hubble constant from the beginning of the twentieth century, when modern cosmology originated, to the present. We develop the arguments that gave rise to the importance of measuring the expansion of the Universe and its discovery, and we describe the different pioneering works attempting to measure it. There has been a long dispute on this matter, even in the present epoch, which is marked by high-tech instrumentation and, therefore, in smaller uncertainties in the relevant parameters. It is, again, currently necessary to conduct a careful and critical revision of the different methods before one invokes new physics to solve the so-called Hubble tension.
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spelling doaj.art-3d3cfa0a02db49ac9d4ccfbf7d4a55dd2023-12-22T14:46:34ZengMDPI AGUniverse2218-19972023-11-0191250110.3390/universe9120501The Unsettled Number: Hubble’s TensionJorge L. Cervantes-Cota0Salvador Galindo-Uribarri1George F. Smoot2Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac C.P. 52750, Mexico State, MexicoDepartment of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac C.P. 52750, Mexico State, MexicoDonostia International Physics Center (DIPC), Basque Country, E-48080 San Sebastian, SpainOne of main sources of uncertainty in modern cosmology is the present rate of the universe’s expansion, H<sub>0</sub>, called the Hubble constant. Once again, different observational techniques bring about different results, causing new “Hubble tension”. In the present work, we review the historical roots of the Hubble constant from the beginning of the twentieth century, when modern cosmology originated, to the present. We develop the arguments that gave rise to the importance of measuring the expansion of the Universe and its discovery, and we describe the different pioneering works attempting to measure it. There has been a long dispute on this matter, even in the present epoch, which is marked by high-tech instrumentation and, therefore, in smaller uncertainties in the relevant parameters. It is, again, currently necessary to conduct a careful and critical revision of the different methods before one invokes new physics to solve the so-called Hubble tension.https://www.mdpi.com/2218-1997/9/12/501Hubble constantHubble tensionobservational cosmologyhistory of physics
spellingShingle Jorge L. Cervantes-Cota
Salvador Galindo-Uribarri
George F. Smoot
The Unsettled Number: Hubble’s Tension
Universe
Hubble constant
Hubble tension
observational cosmology
history of physics
title The Unsettled Number: Hubble’s Tension
title_full The Unsettled Number: Hubble’s Tension
title_fullStr The Unsettled Number: Hubble’s Tension
title_full_unstemmed The Unsettled Number: Hubble’s Tension
title_short The Unsettled Number: Hubble’s Tension
title_sort unsettled number hubble s tension
topic Hubble constant
Hubble tension
observational cosmology
history of physics
url https://www.mdpi.com/2218-1997/9/12/501
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