A collaboration between the neutrino detector and a space telescope led to the identification of a source producing cosmic rays for the first time

The source is an active black hole at the center of a galaxy 3.7 billion light-years away * Prof. Dafna Guetta from the physics department at the Academic College of Engineering in Brauda, ​​who is participating in the project, says that the discovery solved a question in the field of astrophysics that was still open to this day

Neutrinos, the ghost particles that barely make contact with normal matter, have previously been observed to come from supernovae (exploding stars) and the Sun. Now the giant IceCube detector at the South Pole has discovered that even blazars, galaxies with a massive black hole at their center, produce neutrino particles with an intensity millions of times stronger than that of supernovae and stars.

About 3.7 billion years ago, when the Earth was still in its infancy, radiation erupted from a black hole billion times more massive than the Sun in a jet that made its way and met the Earth on September 22, 2017.

This is the first time a neutrino source has been discovered in over 30 years. Moreover, this is the first time scientists have been able to observe high-energy neutrinos associated with a specific astrophysical event. The observation was published in the journal Nature last week.

Neutrino particles (from Italian: "little neutron") are elementary particles, without an electric charge and with a minimal mass that move at a speed very close to the speed of light and can usually pass through normal matter without interference. This feature allows astronomers and astrophysicists to obtain information from places that cannot be directly measured with other tools. On the other hand, this property of the neutrinos makes it very difficult to detect them, which is why they are also called "ghost particles". Indeed, as mentioned, until recently the origin of the neutrinos was never identified.
One such neutrino particle known as IceCube-170922A, discovered as mentioned on September 22, 2017 in the ice cap in Antarctica, sent the IceCube researchers, among them Prof. Daphne Guetta from the Department of Physics at the Academic College of Engineering in Rouda, on a frantic search for its origin in the universe. The answer was found by NASA's Fermi Gamma-ray Space Telescope, which detected gamma radiation from the same source as the neutrino - a blazar-type supermassive black hole whose jet of radiation is directed towards Earth 3.7 billion light-years away. Earth is at the center of an active galaxy.

The IceCube project was established at the exact point of the South Pole to monitor neutrino activity and consists of a square kilometer of sophisticated optical detectors located at a depth of a kilometer in the Antarctic ice sheet. Already in 2013, IceCube's detectors detected cosmic neutrinos with high energies for the first time and an alert was sent to observatories around the world in order to identify the source of the flux that is hitting the Earth, but without success. Now that the origin of IceCube-170922A has been discovered, a reanalysis of the neutrinos' trajectories discovered in 2013 has been carried out and it has been found that they also originate from the same cosmic particle accelerator, located in the heart of a distant galaxy.

Prof. Guetta previously had a permanent position at the University of Rome. In 2011 she moved to Israel for family reasons, and was accepted to the academic college in Rauda.
"Since the beginning of my career, I have been researching high-energy neutrino particles. I started the research with Prof. Eli Waxman from the Weizmann Institute and then continued alone, and occasionally I also research together with him and Prof. Ehud Bacher from the Technion, but today most of her research is done in collaboration with project researchers Ice Cube".

"The power of the neutrino is a million times higher than the power of the most powerful particle accelerator in the world. Imagine what can be done if we succeed in discovering how nature produces such energy." Prof. Guetta explains.
"The neutrino particles have very high energies of trillions of electron volts, thousands to millions of times higher than those of the supernova event, of the nuclear reactions in the sun or of the most powerful particle accelerators on Earth. "For over a century since the discovery of cosmic radiation, researchers have tried to discover its origin Without success, for this purpose they established the IceCube project. After the discovery, we know of one source of neutrinos, which also indicates the presence of protons in that source, and this is an indication that there is material with mass - something physical, not just a magnetic field and electrons.

"We know that high-energy cosmic radiation exists. For years, experiments were conducted to locate the source of cosmic radiation, but they failed to locate the sources. Cosmic radiation consists of protons with a charge. Because they have a charge, we lose our direction. Because they are magnetic, and because they have mass, they sometimes do not reach up to us
Neutrino particles, on the other hand, have no mass and no charge, so it is possible to reconstruct their origin and also understand the processes that caused the explosion. Until today there was a dispute as to whether they are dispersed equally in all directions or whether they are concentrated in a jet that happens to be facing us. Since the discovery of a high-energy neutrino flux in 2013, experimenters have been trying to locate events in which both energetic neutrino particles and gamma rays are recorded, and this is what happened this time. Both the Fermi Space Telescope, which detects gamma-ray bursts, and IceCube located the source.

An open question in astrophysics

Prof. Guetta explains that the source of the radiation is an active nucleus of a galaxy, meaning that the black hole devours matter from its surroundings, some of it enters the black hole and is swallowed up inside it, but some of the matter comes out as a jet of radiation that we see both in the gamma range and as neutrinos.

"Until today we did not know what the jet was made of. Astrophysicists had many theories on the subject. There are those who say that the jet is made only of a magnetic field and electrons and others, including me, argued that the jet must be composed of baryonic matter (ordinary AB matter). Neutrinos are byproducts of Protons, so what was emitted from the distant galaxy and reached us originates from kinetic energy, and not just electromagnetic radiation."

"This is a new era in astronomy, the discovery gives a new dimension to the study of the universe" says Prof. Guetta. "The discovery of additional sources of neutrinos will actually allow the creation of a map of cosmic ray accelerators and advanced research on their activity, which is why this discovery is so important to science. This is a new era in astronomy. The discovery gives a new dimension to the study of the universe," concludes Prof. Guetta.

News about the discovery on The Conversation website

A new window to The Conversation universe

More of the topic in Hayadan:

• Neutrinos with ice
• Particles from space deep in the ice (Report on the discovery from 2013)
• An Unfolding Mystery: One Hundred Years of the Discovery of Cosmic Radiation
• A universe of particles