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How Can CMB Help Constraining Dark Energy?
Licia Verde (ICREA & ICE (IEEC-CSIC))

Cosmic Microwave Background observations have been fundamental in defining the "standard cosmological model". It is however other probes (e.g., Baryon acoustic oscillations, weak lensing, Supernovae, clusters) that are considered the next frontier in dark energy studies. I will discuss how the CMB, alone or in combination with other probes, can help constraining dark energy.



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