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Hubble trouble or Hubble bubble?
The recent analysis of low-redshift supernovae (SN) has increased the apparent tension between the value of $H_0$ estimated from low and high redshift observations such as the cosmic microwave background (CMB) radiation. At the same time other observations have provided evidence of the existence of...
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| Lenguaje: | eng |
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2016
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| Acceso en línea: | https://dx.doi.org/10.1142/S021827181850102X http://cds.cern.ch/record/2215645 |