It seems that the role of active black holes in the production of high-energy neutrinos has been confirmed. Physicists have traced ghost particles to the heart of a galaxy for the second time.

We can use the neutrinos' properties to understand their home environments with this finding.

A beautiful barred spiral located around 47 million light-years away, known as the SquidGalaxy, is a well- studied object.

Scientists have counted tens of neutrinos coming from its direction.

There was a single TeV particle tracked to an extragalactic source that was traced to a blazar some 3.8 billion light-years away.

The new collection of data was obtained over the course of a decade.

It is possible to single out a source. Francis Halzen of the University of Wisconsin-Madison is the principal investigator of IceCube.

It's not yet enough to answer all our questions, but they are the next big step towards the realization of neutrino astronomy.

Neutrinos are small particles produced by radioactive decay.

They are among the most abundant particles in the universe. Right now they are streaming through you. It's difficult to detect them because they barely interact with anything.

Normal matter in the universe may be smoke and shadows. They are called ghost particles because of this.

They're so potentially useful to study because of this very property. They travel in a straight line because they aren't affected by the Universe.

Powerful jets generated in the extreme environment around a black hole are examples of processes that produce high-energy neutrinos.

We need to find the neutrinos to learn about these factories. When the neutrinos interact with atoms, photodetectors look for a shower of light produced.

The IceCube observatory with the Milky Way overhead.
The IceCube Lab at night, with the Milky Way visible overhead. (Martin Wolf/IceCube/NSF)

This is how a tight, international collaboration, carefully analyzing 10 years' worth of data collected by the observatory, was able to identify 80 high-energy neutrinos in the 1.5 to 15 TeV range.

We have already noted that the galaxy is an active one. The black hole at the center of the barred spiral is consuming matter at a rapid rate from the surrounding space.

The black hole is surrounded by a large disk of dust and gas. The gravity of the torus and disk causes insane amounts of heat and light.

Some of the material doesn't end up in the black hole. Scientists think that some of it gets accelerated along the black hole's magnetic field lines to the poles, where it is launched into space in the form of powerful jets ofplasma that punch through space almost at light speed.

If the jet is pointed in our direction, TXS 0506+056 is a blazar, and analysis shows its 300 TeV neutrino was produced in the jet.

The jet doesn't point in our direction. A lot of the high-energy light from the active galactic nucleus is obscured by dense dust. It's possible that the neutrinos could be used to investigate a black hole.

According to a physicist at Michigan State University, recent models of the black hole environments suggest that gas, dust, and radiation should block the gamma rays.

Our understanding of the environments around black holes will be improved by this detection.

According to the team, the discovery suggests that active galactic nuclei make a significant contribution to the neutrino population.

They say that the discovery is a breakthrough for astronomy and that it could become one of the cornerstones of the field in the future.

An ambitious project to expand our understanding of the Universe was started several years ago by the National Science Foundation.

This new and exciting field that promises insights into the undiscovered power of massive black holes, and other fundamental properties of the universe, is just the beginning of this new and exciting field.

The research has appeared in a journal.