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• W2605804845 abstract "Intensity interferometry is a technique that has been used to measure the size of sources ranging from the quark-gluon plasma formed in heavy ion collisions to the radii of stars. We investigate using the same technique to measure proto-neutron star (PNS) radii with the neutrino signal received from a core-collapse supernovae. Using a full wave-packet analysis, including the neutrino mass for the first time, we derive criteria where the effect can be expected to provide the desired signal, and find that neutrinos from the next Galactic supernova should contain extractable PNS radius information." @default.
• W2605804845 created "2017-04-28" @default.
• W2605804845 creator A5000485742 @default.
• W2605804845 creator A5082981947 @default.
• W2605804845 date "2017-08-01" @default.
• W2605804845 modified "2023-10-13" @default.
• W2605804845 title "Neutrino Intensity Interferometry: Measuring Protoneutron Star Radii During Core-Collapse Supernovae" @default.
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• W2605804845 doi "https://doi.org/10.1103/physrevlett.119.051101" @default.
• W2605804845 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/28949708" @default.
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