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| cmb [2014/06/30 12:35] – valeria | cmb [2014/06/30 17:01] – valeria |
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| The most [[http://arxiv.org/abs/1303.5076|recent CMB data]] were delivered by the ESA mission [[http://sci.esa.int/planck|Planck]]: the all-sky image realized by the Planck satellite is the most precise picture of the early Universe and the results confirm that the Universe is in agreement with Lambda-CDM model. Our group is involved in the Planck Mission and collaborates [[http://arxiv.org/abs/1303.5076|in cosmological parameter estimation]]. | The most [[http://arxiv.org/abs/1303.5076|recent CMB data]] were delivered by the ESA mission [[http://sci.esa.int/planck|Planck]]: the all-sky image realized by the Planck satellite is the most precise picture of the early Universe and the results confirm that the Universe is in agreement with Lambda-CDM model. Our group is involved in the Planck Mission and collaborates [[http://arxiv.org/abs/1303.5076|in cosmological parameter estimation]]. |
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| The CMB is a very powerful observable which can be used to rule out or to validate the cosmological models and test fundamental physics. The ITP Cosmology group employed it for instance to test [[http://arxiv.org/abs/1202.1476|varying fundamental constants]], [[http://inspirehep.net/record/1215575|early dark energy]], [[http://inspirehep.net/record/1122522|coupled dark energy]], etc. | The CMB is a very powerful observable which can be used to rule out or to validate the cosmological models and test fundamental physics. The ITP Cosmology group employed it for instance to test [[http://arxiv.org/abs/1202.1476|varying fundamental constants]], [[http://inspirehep.net/record/1215575|early dark energy]], [[http://inspirehep.net/record/1122522|coupled dark energy]], |
| | speed of gravitational waves and lensing B modes in [[http://inspirehep.net/record/1298254|Hordenski models]] etc. |
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