| MG14 | Rome 12 - 18 July, 2015 |
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Session: |
CM2-3 - (CM2) Cosmology with the Cosmic Microwave Background: Implications of Planck and Other Experiments in Temperature and Polarization (CM3) Galaxy Clusters as probes for Cosmology and Dark Matter |
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Chairperson: |
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Day: |
Friday, July 17 |
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Room: |
FMRasetti - Second floor - Physics-Marconi (VEF) - CU013 |
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| Arrived | Accept | N. | Hour | Time | Talk Type | Speaker | Talk Title | Talk view |
| √ | Yes |
1 |
14:30 | 20' | Oral abstract | |||
| √ | Yes |
2 |
14:50 | 10' | Oral abstract |
Cosmic Polarization Rotation: a GR test using astrophysical measurements |
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| √ | Yes |
3 |
15:00 | 20' | Oral abstract | |||
| √ | Yes |
4 |
15:20 | 20' | Oral abstract |
Deciphering the Early Universe: Connecting Theory with Observations |
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| √ | Yes |
5 |
15:40 | 10' | Oral abstract | |||
| √ | Yes |
6 |
15:50 | 10' | Oral abstract |
Features in the spectrum of primordial perturbations, constraints from CMB and SDSS data. |
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COFFEE BREAK |
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| √ | Yes |
7 |
16:30 | 20' | Oral abstract |
Cosmology with Square Kilometre Array and Synergies with CMB observations |
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| √ | Yes |
8 |
16:50 | 10' | Oral abstract |
Square Kilometre Array and Cosmic Microwave Background spectral distortions |
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| √ | Yes |
9 |
17:00 | 30' | Oral abstract | |||
| √ | Yes |
10 |
17:30 | 30' | Oral abstract |  |
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