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July 14, 2025

Neutrinos could have a secret life: Study suggests they may interact secretly during massive star collapse

Left Panel: When neutrinos scatter with themselves via standard model interactions the collapsing core of the massive star is relatively cold, and the neutrinos are mostly all electron flavor. In this scenario we may get a supernova explosion leaving, usually, a neutron star remnant. Right Panel: If neutrinos have "secret" interactions with themselves, then electron neutrinos can be converted to all flavors. This leads to rapid heating, the "melting" of nuclei, and the rapid conversion of most protons to neutrons. We might get a black hole instead of a neutron star remnant. It is not yet clear if we get a supernova explosion. Credit: George Fuller lab / UC San Diego
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Left Panel: When neutrinos scatter with themselves via standard model interactions the collapsing core of the massive star is relatively cold, and the neutrinos are mostly all electron flavor. In this scenario we may get a supernova explosion leaving, usually, a neutron star remnant. Right Panel: If neutrinos have "secret" interactions with themselves, then electron neutrinos can be converted to all flavors. This leads to rapid heating, the "melting" of nuclei, and the rapid conversion of most protons to neutrons. We might get a black hole instead of a neutron star remnant. It is not yet clear if we get a supernova explosion. Credit: George Fuller lab / UC San Diego

Neutrinos are cosmic tricksters, paradoxically hardly there but lethal to stars significantly more massive than the sun.

These come in three known "flavors": electron, muon and tau. Whatever the flavor, neutrinos are notoriously slippery, and much about their properties remains mysterious. It is almost impossible to collide neutrinos with each other in the lab, so it is not known if neutrinos interact with each other according to the , or if there are much-speculated "secret" interactions only among neutrinos.

Now a team of researchers from the Network for Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS), including several from UC San Diego, have shown, through theoretical calculations, how collapsing can act as a "neutrino collider." Neutrinos steal from these stars, forcing them to contract and causing their electrons to move near light speed. This drives the stars to instability and collapse.

The study, in Âé¶¹ÒùÔºical Review Letters, was led by UC San Diego researchers Anna M. Suliga, Julien Froustey, Lukáš Gráf, Kyle Kehrer and George Fuller, as well as collaborators from other institutions.

Eventually, the collapsing star's density becomes so high that the neutrinos are trapped and collide with each other. With purely standard model interactions, the neutrinos will be mostly electron-flavored, the matter will be relatively "cold," and the collapse will likely leave a neutron star remnant. However, secret interactions that change neutrino flavor radically alter this scenario, producing neutrinos of all flavors and leading to a mostly neutron "hot" core that may lead to a black hole remnant.

Fermi National Accelerator Lab's upcoming Deep Underground Neutrino Experiment (DUNE) might be able to test these ideas, as might future observations of the or from collapsing stars.

More information: Anna M. Suliga et al, Nonconservation of Lepton Numbers in the Neutrino Sector Could Change the Prospects for Core Collapse Supernova Explosions, Âé¶¹ÒùÔºical Review Letters (2025).

Journal information: Âé¶¹ÒùÔºical Review Letters

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Theoretical calculations indicate that during the collapse of massive stars, high neutrino densities could enable secret interactions beyond the Standard Model. Such interactions may alter neutrino flavor distributions, resulting in hotter, neutron-rich cores and increasing the likelihood of black hole formation instead of neutron stars. Future experiments like DUNE may test these predictions.

This summary was automatically generated using LLM.