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How and Why Stars Die? New Study on 'Flavours' in Supernova Unlocks New Clues

IANS

Last Updated: December 23, 2020, 11:35 IST

News18 representational image.

News18 representational image.

Contrary to the past practice of simplifying studies by studying one flavour while ignoring the other two, the researchers in the new study created a non-linear simulation of a 'fast conversion' when three neutrino flavours are present, where a fast conversion is marked by neutrinos interacting and changing flavours.

Researchers from Northwestern University (NU) have found that by studying all three “flavours” involved in a supernova, they have unlocked more clues as to how and why stars die.

Contrary to the past practice of simplifying studies by studying one flavour while ignoring the other two, the researchers in the new study created a non-linear simulation of a “fast conversion” when three neutrino flavours are present, where a fast conversion is marked by neutrinos interacting and changing flavours.

They removed the assumption that the three flavours of neutrinos, muon, electron and tau neutrinos, have the same angular distribution, giving them each a different distribution.

A two-flavour setup of the same concept looks at electron neutrinos and “x” neutrinos, in which x can be either muon or tau neutrinos and where differences between the two are insignificant.

When an enormous number of neutrinos are sent careening during the massive explosion of a core-collapse supernova, they begin to oscillate. Interactions between neutrinos change the properties and behaviours of the whole system, creating a coupled relationship.

Therefore, when neutrino density is high, a fraction of neutrinos interchange flavours. When different flavours are emitted in different directions deep within a star, conversions occur rapidly and are called “fast conversions.”

Interestingly, the research found that as the number of neutrinos grows, so do their conversion rates, regardless of mass, reports Xinhua news agency.

“We are trying to convince the community that when you take these fast conversions into account, you have to use all three flavours to understand it,” said senior author Manibrata Sen, a postdoctoral researcher currently based at NU under the Network for Neutrinos, Nuclear Astrophysics and Symmetries program at University of California – Berkeley.

“A proper understanding of fast oscillations can actually hold the key to why some stars explode from supernovas.”

In the next step, the researchers hope to make their results more generic by including spatial dimensions in addition to components of momentum and time.

The study has been published in the journal Physical Review Letters.

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first published:December 23, 2020, 11:28 IST
last updated:December 23, 2020, 11:35 IST