Important clues into cause and process of death of stars revealed by IIT Guwahati researchers


IIT Guwahati researchers find key clues about the death of stars! Working with researchers from Germany-based Max Planck Institute for Physics and US’ Northwestern University, researchers from the eminent Indian Institute of Technology (IIT), Guwahati, have found major clues to better understand the death of stars. Moreover, they have also been able to point out the problems that existing models had. The team of researchers has revealed that the clue to the death of these stars lies in tiny subatomic particles called neutrinos in the supernovae, and have said that all the three species of neutrinos are important, instead of commonly believed two. The research published in Physics Review Letters journal. In a statement issued by IIT Guwahati, lead researcher Dr Sovan Chakraborty carried out the research with research scholar Madhurima Chakraborty, along with Max Planck Institute’s postdoctoral fellow Dr Francesco Capozzi and Northwestern University postdoctoral fellow Dr Manibrata Sen. The researchers pointed out that so far, the existing models of supernovae predicted that antineutrinos as well as the neutrinos species mu and tau were very similar in their properties and clubbed them as one species, leading to simplified problem of the supernovae and neutrinos. This meant that most studies were being carried out with researchers assuming that all these neutrinos and antineutrinos were behaving in the same way when they were ejected from the dying star. The study has clearly demonstrated the relevance of all the three flavours of neutrinos, leading to an incomplete picture of fast flavour exchange if the presence of any species is ignored Dr Sovan said that in extremely dense supernovae core, neutrinos interact with each other, and they might interchange their flavours. This interchanging, however, can happen very rapidly and it can impact the process of the supernova because neutrinos of different species are emitted from the explosion with different angular distribution. The conversion of flavours is non-linear, Dr Sovan added, and the phenomenon is not confronted in any other sources of the neutrino except the supernovae. For the first time, the research team carried out nonlinear simulations of this rapid conversion between all three species of neutrinos. This was possible because new simulations of supernovae showed the presence of muons, leading to the production of asymmetry between antineutrinos and muon neutrinos, which was otherwise taken to be zero. This has implied three flavour effects. Dr Manibrata Sen was quoted by the statement as saying that the study of these three flavours has changed the results drastically as against the results of existing studies. This study, Sen said, can have huge implications for particle and astrophysics of supernovae neutrinos.

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