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Do we care about the distance to the CMB? Clarifying the impact of second-order lensing
It has recently been shown that second-order corrections to the background distance-redshift relation can build up significantly at large redshifts, due to an aggregation of gravitational lensing events. This shifts the expectation value of the distance to the CMB by 1%. In this paper we show that t...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2015
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2015/06/050 http://cds.cern.ch/record/2004544 |
_version_ | 1780946121707749376 |
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author | Bonvin, Camille Clarkson, Chris Durrer, Ruth Maartens, Roy Umeh, Obinna |
author_facet | Bonvin, Camille Clarkson, Chris Durrer, Ruth Maartens, Roy Umeh, Obinna |
author_sort | Bonvin, Camille |
collection | CERN |
description | It has recently been shown that second-order corrections to the background distance-redshift relation can build up significantly at large redshifts, due to an aggregation of gravitational lensing events. This shifts the expectation value of the distance to the CMB by 1%. In this paper we show that this shift is already properly accounted for in standard CMB analyses. We clarify the role that the distance to the CMB plays in the presence of second-order lensing corrections. |
id | cern-2004544 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
spelling | cern-20045442023-10-04T21:42:52Zdoi:10.1088/1475-7516/2015/06/050http://cds.cern.ch/record/2004544engBonvin, CamilleClarkson, ChrisDurrer, RuthMaartens, RoyUmeh, ObinnaDo we care about the distance to the CMB? Clarifying the impact of second-order lensingAstrophysics and AstronomyIt has recently been shown that second-order corrections to the background distance-redshift relation can build up significantly at large redshifts, due to an aggregation of gravitational lensing events. This shifts the expectation value of the distance to the CMB by 1%. In this paper we show that this shift is already properly accounted for in standard CMB analyses. We clarify the role that the distance to the CMB plays in the presence of second-order lensing corrections.It has recently been shown that second-order corrections to the background distance-redshift relation can build up significantly at large redshifts, due to an aggregation of gravitational lensing events. This shifts the expectation value of the distance to the CMB by 1%. In this paper we show that this shift is already properly accounted for in standard CMB analyses. We clarify the role that the area distance to the CMB plays in the presence of second-order lensing corrections.It has recently been shown that second-order corrections to the background distance-redshift relation can build up significantly at large redshifts, due to an aggregation of gravitational lensing events. This shifts the expectation value of the distance to the CMB by 1%. In this paper we show that this shift is already properly accounted for in standard CMB analyses. We clarify the role that the area distance to the CMB plays in the presence of second-order lensing corrections.arXiv:1503.07831CERN-PH-TH-2015-062CERN-PH-TH-2015-062oai:cds.cern.ch:20045442015-03-26 |
spellingShingle | Astrophysics and Astronomy Bonvin, Camille Clarkson, Chris Durrer, Ruth Maartens, Roy Umeh, Obinna Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title | Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title_full | Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title_fullStr | Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title_full_unstemmed | Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title_short | Do we care about the distance to the CMB? Clarifying the impact of second-order lensing |
title_sort | do we care about the distance to the cmb? clarifying the impact of second-order lensing |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1088/1475-7516/2015/06/050 http://cds.cern.ch/record/2004544 |
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