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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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Lenguaje: | eng |
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2022
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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? 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>
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<p>The video of the presentation will be available shortly after the event. </p>
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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? 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> </p> <p>The video of the presentation will be available shortly after the event. </p> <div> </div> <div> </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 |