Categories: neutrinos

Almost all High-Energy Neutrinos Come From Quasars

Buried under the ice at the South Pole is a neutrino observatory called IceCube. Every now and then IceCube will detect a particularly high-energy neutrino from space. Some of them are so high energy we aren’t entirely sure what causes them. But a new article points to quasars as the culprit.

Quasars are distant supermassive black holes. During the early universe, many of these black holes were extremely active. The hot material surrounding these black holes can emit everything from x-rays to powerful bursts of radio light. In this new work, the team analyzed 7 years of data from IceCube and found an interesting correlation between quasars and high-energy neutrinos.

Map comparing quasar locations to probable neutrino sources. Credit: Plavin, et al

The data showed that most of the high-energy neutrinos originated from the centers of quasars. Their detection often occurs around the time that a quasar undergoes a strong radio burst. Since neutrinos travel at nearly the speed of light, photons and neutrinos reach Earth and nearly the same time. This suggests that the quasar radio bursts are producing neutrinos.

To explain this, the team proposed a rough model. Strong radio quasar bursts occur when hot, ionized gas near the black hole flows through strong magnetic fields. The charged particles are accelerated, causing them to emit radio light. But a rapid flow of dense plasma also causes nuclei and electrons to collide with each other. The high-energy collision of protons can create pions, which emit gamma rays and neutrinos when they decay.

How quasars might create high-energy neutrinos. Credit: Plavin, et al

This is only a rough model. To study their idea further, the team will gather more radio observations of quasars, as well as data from a neutrino telescope known as the Baikal Gigaton Volume Detector. Together this will allow them to study the central regions of quasars in detail.

Reference: Plavin, A. V., et al. “Directional Association of TeV to PeV Astrophysical Neutrinos with Radio Blazars.” The Astrophysical Journal 908.2 (2021): 157.

Brian Koberlein

Brian Koberlein is an astrophysicist and science writer with the National Radio Astronomy Observatory. He writes about astronomy and astrophysics on his blog. You can follow him on YouTube, and on Twitter @BrianKoberlein.

Recent Posts

Scientists Develop Technique to Create 3D Models of Cosmic Structures

For decades, astronomers have used powerful instruments to capture images of the cosmos in various…

3 hours ago

The Best Way to Find Planet Nine Might Be Hundreds of Tiny Telescopes

Although the outer Solar System is mostly empty, there are icy objects drifting within the…

4 hours ago

It Takes Very Special Conditions to Create This Bizarre Stellar Spectacle

A stellar odd couple 700 light-years away is creating a chaotically beautiful display of colourful,…

4 hours ago

A New Look a the Most Ancient Light in the Universe

About 370,000 years after the Big Bang, the Universe had cooled down so light could…

6 hours ago

Space Tourism: The Good, The Bad, The Meh

Space tourism here is here to stay, and will likely remain a permanent fixture of…

11 hours ago

New Study Examines Cosmic Expansion, Leading to a New Drake Equation

In 1960, in preparation for the first SETI conference, Cornell astronomer Frank Drake formulated an…

1 day ago