Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
The quantity and quality of cosmic structure observations have greatly accelerated in recent years, and further leaps forward will be facilitated by imminent projects. These will enable us to map the evolution of dark and baryonic matter density fluctuations over cosmic history. The way that these f...
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| Veröffentlicht in: | Astroparticle physics 2014-03, Vol.63 |
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| creator | Huterer, Dragan Kirkby, David Bean, Rachel Connolly, Andrew Dawson, Kyle Dodelson, Scott Evrard, August Jain, Bhuvnesh Jarvis, Michael Linder, Eric Mandelbaum, Rachel May, Morgan Raccanelli, Alvise Reid, Beth Rozo, Eduardo Schmidt, Fabian Sehgal, Neelima Slosar, Anze Van Engelen, Alex Wu, Hao-Yi Zhao, Gongbo |
| description | The quantity and quality of cosmic structure observations have greatly accelerated in recent years, and further leaps forward will be facilitated by imminent projects. These will enable us to map the evolution of dark and baryonic matter density fluctuations over cosmic history. The way that these fluctuations vary over space and time is sensitive to several pieces of fundamental physics: the primordial perturbations generated by GUT-scale physics; neutrino masses and interactions; the nature of dark matter and dark energy. We focus on the last of these here: the ways that combining probes of growth with those of the cosmic expansion such as distance-redshift relations will pin down the mechanism driving the acceleration of the Universe. |
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| subjects | ASTRONOMY AND ASTROPHYSICS Cosmology Dark energy Large-scale structure |
| title | Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion |
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