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SUMMARY:DE models with combined H0⋅rd from BAO and CMB dataset and frien
 ds
DTSTART;VALUE=DATE-TIME:20230601T135000Z
DTEND;VALUE=DATE-TIME:20230601T141500Z
DTSTAMP;VALUE=DATE-TIME:20260907T155213Z
UID:indico-contribution-971@cern.ch
DESCRIPTION:Speakers: Denitsa STAICOVA ()\nIt has been theorized that Dyna
 mical Dark Energy (DDE) could be a possible solution to the Hubble tension
 . To avoid the degeneracy between the Hubble parameter H0 and the sound ho
 rizon scale rd\, we use their multiplication as one parameter c/(H0rd). To
  the BAO points we add the SNIa Pantehon dataset and GRB dataset and the p
 oints from the CMB priors. We use different DE parametrizations to constra
 in the cosmological parameters and we compare the results based on statist
 ical measures. We compare the results with the ones obtained by marginaliz
 ing over the H0⋅rd by redefining the likelihood in a BAO and SNIa datase
 ts.\n\nhttps://indico.unina.it/event/70/contributions/971/
LOCATION:Lisbon
URL:https://indico.unina.it/event/70/contributions/971/
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