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Observational probes of dark energy/modified gravity

<!--HTML--><p>The discovery of the accelerated expansion of the Universe has come relatively late in our study of the cosmos, but in showing that gravity can act repulsively, it has opened up many new questions about the nature of gravity and what the Universe might contain. Is the accel...

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Autor principal: Koyama, Kazuya
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:http://cds.cern.ch/record/2806721
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author Koyama, Kazuya
author_facet Koyama, Kazuya
author_sort Koyama, Kazuya
collection CERN
description <!--HTML--><p>The discovery of the accelerated expansion of the Universe has come relatively late in our study of the cosmos, but in showing that gravity can act repulsively, it has opened up many new questions about the nature of gravity and what the Universe might contain. Is the acceleration being driven by dark energy?&nbsp; Or is general relativity itself in error, requiring a modification at large scales to account for the late acceleration? Structure formation in our Universe can be different even if the geometry of the homogeneous and isotropic universe is the same in these two classes of models, offering a possibility to distinguish between them observationally. I will discuss cosmological tests of dark energy and modified gravity models using latest cosmological observations.</p> <p>&nbsp;</p> <p>The video of the presentation will be available shortly after the event.&nbsp;</p> <div>&nbsp;</div> <div>&nbsp;</div>
id cern-2806721
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2022
record_format invenio
spelling cern-28067212022-11-02T22:04:06Zhttp://cds.cern.ch/record/2806721engKoyama, KazuyaObservational probes of dark energy/modified gravityObservational probes of dark energy/modified gravityEuCAPT Virtual Colloquium<!--HTML--><p>The discovery of the accelerated expansion of the Universe has come relatively late in our study of the cosmos, but in showing that gravity can act repulsively, it has opened up many new questions about the nature of gravity and what the Universe might contain. Is the acceleration being driven by dark energy?&nbsp; Or is general relativity itself in error, requiring a modification at large scales to account for the late acceleration? Structure formation in our Universe can be different even if the geometry of the homogeneous and isotropic universe is the same in these two classes of models, offering a possibility to distinguish between them observationally. I will discuss cosmological tests of dark energy and modified gravity models using latest cosmological observations.</p> <p>&nbsp;</p> <p>The video of the presentation will be available shortly after the event.&nbsp;</p> <div>&nbsp;</div> <div>&nbsp;</div>oai:cds.cern.ch:28067212022
spellingShingle EuCAPT Virtual Colloquium
Koyama, Kazuya
Observational probes of dark energy/modified gravity
title Observational probes of dark energy/modified gravity
title_full Observational probes of dark energy/modified gravity
title_fullStr Observational probes of dark energy/modified gravity
title_full_unstemmed Observational probes of dark energy/modified gravity
title_short Observational probes of dark energy/modified gravity
title_sort observational probes of dark energy/modified gravity
topic EuCAPT Virtual Colloquium
url http://cds.cern.ch/record/2806721
work_keys_str_mv AT koyamakazuya observationalprobesofdarkenergymodifiedgravity