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Big Bang Nucleosynthesis, Cosmic Microwave Background Anisotropies and Dark Energy (2001)
| Content Provider | CiteSeerX |
|---|---|
| Author | Signore, M. Puy, D. |
| Abstract | Abstract. Over the last decade, cosmological observations have attained a level of precision which allows for very detailed comparison with theoretical predictions. We are beginning to learn the answers to some fundamental questions, using information contained in Cosmic Microwave Background Anisotropy (CMBA) data. In this talk, we briefly review some studies of the current and prospected constraints imposed by CMBA measurements on the neutrino physics and on the dark energy. As it was already announced by Scott [1], we present some possible new physics from the Cosmic Microwave Background (CMB). 1 |
| File Format | |
| Publisher Date | 2001-01-01 |
| Access Restriction | Open |
| Subject Keyword | Big Bang Nucleosynthesis Neutrino Physic Cosmological Observation Last Decade Theoretical Prediction Possible New Physic Cosmic Microwave Background Prospected Constraint Cmba Measurement Fundamental Question Cosmic Microwave Background Anisotropy Dark Energy Detailed Comparison |
| Content Type | Text |
| Resource Type | Article |
