| Location: | Home  CMB Presentation for ICNO Meeting 18-Mar-2020.pdf CMB Presentation for ICNO Meeting 18-Mar-2020.pdf Properties |
| Location: | Home CMB Presentation for ICNO Meeting 18-Mar-2020.pdf CMB Presentation for ICNO Meeting 18-Mar-2020.pdf Properties |
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| CMB Presentation for ICNO Meeting 18-Mar-2020.pdf | |
| Handle: | Version-104467 |
| Owner: | Hanson, Kael (User-71, kaeld:LDAP)DS |
| Wednesday, March 18, 2020 09:01:31 AM CDT | |
| Wednesday, March 18, 2020 09:44:30 AM CDT | |
| Modified By: | |
| - The CMB Probes Cosmology and Fundamental Physics 2 Inflation • Rule out and test simplest models of Inflation • Measure the Energy-scale of Inflation (~1016 GeV) Neutrinos • Detect or rule out the production of any new light relic particle species • Measure structure growth to detect the sum of the neutrino masses Dark Energy • Use CMB as back-light to measure evolution of structure via lensing and Sunyaev-Zel’dovich effect • Tests of gravity and the nature of dark energy The South Pole is the Best Place in the World to Observe the CMB South Pole Environment • High Altitude (~10,000 ft) ... | |
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| Appears In: | CMB Presentation for ICNO Meeting 18-Mar-2020.pdf |
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