Using neutrino oscillations to measure <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e701" altimg="si7.svg"><mml:msub><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msub></mml:math>
نویسندگان
چکیده
The tension between late and early universe probes of today’s expansion rate, the Hubble parameter H 0 , remains a challenge for standard model cosmology ? CDM. There are many theoretical proposals to remove tension, with work still needed on that front. However, by looking at new one can get insights might ease tension. Here, we argue neutrino oscillations could be such probe. We expand previous study full three-flavor within CDM paradigm. show how oscillation probabilities evolve differently redshift different values mass hierarchies. also point out this affects fluxes which, from their measurements telescopes, would determine which value is probed technique, thus establishing aforementioned aim.
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ژورنال
عنوان ژورنال: Physics of the Dark Universe
سال: 2022
ISSN: ['2212-6864']
DOI: https://doi.org/10.1016/j.dark.2022.101063