From Friedrich-Alexander-Universität Erlangen-Nürnberg [FAU] (DE): “Are pulsars the source of galactic cosmic rays?”

From Friedrich-Alexander-Universität Erlangen-Nürnberg [FAU] (DE)

September 17, 2021

New FAU research group hopes to provide experimental evidence for cosmic rays using high energy gamma rays from the area around pulsars.

For Dr. Alison Mitchell, who is transferring to FAU from Swiss Federal Institute of Technology ETH Zürich [Eidgenössische Technische Hochschule Zürich)](CH), it would be a dream come true. From October, Dr. Mitchell and her Emmy Noether junior research group at the Erlangen Centre for Astroparticle Physics (DE) are to investigate the role pulsars play in creating galactic, high-energy cosmic rays. The project is set to run for six years, and has received nearly 1.5 million euros in funding.

The search for the origin of cosmic rays

Galactic cosmic rays are created within our galaxy, the Milky Way. They consist predominantly of charged particles, i.e. protons, ions, positrons and electrons that are accelerated under extreme conditions and arrive at the Earth laden with high energy. As photons-or light particles-are created during the acceleration process gamma rays can also provide clues to the nature of cosmic accelerators. The first step towards understanding this phenomenon was taken in 1912, when cosmic rays were discovered by the Austrian physicist Victor Franz Hess. Charged particles are deflected on their long journey to the Earth by interstellar magnetic fields. Research into the origin of cosmic rays therefore focuses on non-charged particles such as photons or neutrinos, as they come down to Earth directly and can give us clues as to their site of origin. Alison Mitchell is one of the leading scientists in the world for research into high-energy photons from space, known as gamma rays.

It is still not known where cosmic rays come from and whether they originate from one or several source populations. The most promising candidates include supernova remnants; the area around rotating neutron stars; or pulsars and black holes. “Many colleagues tend to favour supernova remnants but experiments have so far failed to provide unambiguous proof that this is the case,” explains Dr. Mitchell. The longer ago the stellar explosion took place, the lower the acceleration is expected to be. In addition, theoretical investigations have not yet succeeded in providing convincing evidence that particles in supernova remnants can be accelerated to the extremely high energy levels found in cosmic rays. Scientists are therefore looking for other explanations. Several research groups-for example in France; Poland and the USA-are working on theoretical models indicating that galactic cosmic rays originate in the area around pulsars.

It was only proven in 2019 that pulsar wind nebulas are capable of accelerating positrons and electrons to energy levels of 1015 electron volts. It follows that the main components of galactic cosmic rays, in other words protons and ions, may also originate from the area around a pulsar. In her work at FAU Dr. Mitchell now hopes to provide the anticipated experimental proof that protons are accelerated by pulsars and the area around them. ‘As far as I am aware, the extensive research programme we are planning is the only one of its kind in the world,’ she explains.

On the lookout with gigantic telescopes

As high-energy particles are hard to find using satellites, researchers are using the Earth’s atmosphere as a detector. Čerenkov telescopes intercept the faint glow that is emitted when a photon from the gamma rays collides with the Earth’s atmosphere. The five telescopes at the HESS observatory in Namibia accurately plot the direction of the gamma rays.

Alison Mitchell and other researchers from FAU are also involved in the major international project to build a ground-based observatory for gamma ray astronomy known as the Čerenkov Telescope Array (CTA).

Algorithms are to be used to improve the resolution of the telescopes. Currently, researchers are also working on new methods aimed at detecting gamma ray sources spread over a wider area. Mitchell believes that thanks to its leading position in the field of theoretical astrophysics and neutrino, X-ray and gamma ray astronomy, FAU offers a very broad range of possible avenues for her project. “It is extremely likely both supernovas and pulsars are responsible for galactic cosmic rays, but I believe that pulsars can accelerate particles to energies thousands of times higher than those attained by supernova remnants.”

See the full article here.


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Friedrich-Alexander-Universität Erlangen-Nürnberg, [FAU] (DE} is a public research university in the cities of Erlangen and Nuremberg in Bavaria, Germany. The name Friedrich–Alexander comes from the university’s first founder Friedrich, Margrave of Brandenburg-Bayreuth, and its benefactor Christian Frederick Charles Alexander, Margrave of Brandenburg-Ansbach.

FAU is the second largest state university in the state of Bavaria. It has 5 faculties, 24 departments/schools, 25 clinical departments, 21 autonomous departments, 579 professors, 3,457 members of research staff and roughly 14,300 employees.

In winter semester 2018/19 around 38,771 students (including 5,096 foreign students) enrolled in the university in 265 fields of study, with about 2/3 studying at the Erlangen campus and the remaining 1/3 at the Nuremberg campus. These statistics put FAU in the list of top 10 largest universities in Germany. In 2018, 7,390 students graduated from the university and 840 doctorates and 55 post-doctoral theses were registered. Moreover, FAU received 201 million Euro (2018) external funding in the same year, making it one of the strongest third-party funded universities in Germany.

FAU is also a member of DFG (Deutsche Forschungsgemeinschaft) and the Top Industrial Managers for Europe network.