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Connections Between X-Ray and Neutrino Emission?

Connections Between X-Ray and Neutrino Emission?

by Brandon Pries | Dec 6, 2025 | Daily Paper Summaries, PRJ

Today’s authors investigate how the physics in the extreme environments in the centers of galaxies leads to connections between X-rays and ghostly particles called neutrinos!

KM3-230213A is looking for its cosmic-ray parent

KM3-230213A is looking for its cosmic-ray parent

by Guest | Sep 3, 2025 | Daily Paper Summaries

How do you produce ultra-high-energy neutrinos like KM3-230213A? Guest author Domenik Ehlert explains how cosmic rays may be behind it!

Ultra-high energy neutrino emission on the extragalactic express: A mystery

Ultra-high energy neutrino emission on the extragalactic express: A mystery

by Chloe Klare | Jun 18, 2025 | Daily Paper Summaries

In today’s paper, our authors investigate three galaxies in the radio to determine where an ultra high-energy neutrino came from.

Why is there more matter than antimatter? Gravitational waves may help us find the answer

Why is there more matter than antimatter? Gravitational waves may help us find the answer

by Abbé Whitford | May 5, 2025 | Daily Paper Summaries

In today’s astrobite, we talk about how gravitational waves could provide insight on particle physics, events in the early Universe, and even matter and antimatter asymmetry.

This just in: Multi-messenger merger made meticulously on massive supercomputer!

This just in: Multi-messenger merger made meticulously on massive supercomputer!

by Cole Meldorf | Jan 24, 2025 | Daily Paper Summaries

In this Astrobite, the authors study the incredible physics of a binary neutron star merger by performing the longest ever simulation on a supercomputer!

Do neutrinos interACT? Looking for hints with the Atacama Cosmology Telescope (ACT)

Do neutrinos interACT? Looking for hints with the Atacama Cosmology Telescope (ACT)

by Abbé Whitford | Aug 11, 2024 | Daily Paper Summaries, PRJ

Today’s bite will discuss how we can use cosmological data to look for new kinds of interactions between neutrinos.

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