INFN-LNF Laboratori Nazionali di Frascati
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11:30
Mini-Workshop: Theoretical implications on the first results of the Desi experiment
Danilo Babusci (Istituto Nazionale di Fisica Nucleare)
Federico Mescia (Istituto Nazionale di Fisica Nucleare)
Our leading model of the universe is known as Lambda CDM. It includes both a weakly interacting type of matter (cold dark matter, or CDM) and dark energy (Lambda). Both matter and dark energy shape how the universe expands – but in opposing ways. Matter and dark matter slow the expansion down, while dark energy …
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