Acceleration and Propagation of Cosmic Rays in High-Metallicity Astrophysical Environments
Ana Laura Müller
Acceleration and Propagation of Cosmic Rays in High-Metallicity Astrophysical Environments
Ana Laura Müller
Paperback
|
Engels
€ 118,95
- Vanaf €15,- geen verzendkosten.
- 30 dagen ruiltermijn voor fysieke producten
Omschrijving
On one hand, the hypothesis of accelerating particles with energies above 10¹⁸ eV in starburst superwinds is carefully revisited, taking into account the constraints imposed by the most recent electromagnetic observations.
Ana Laura Müller received her Licentiate degree in Astronomy from the Universidad Nacional de La Plata (UNLP). Afterwards, she started her doctoral research focusing on the origin of ultra-high-energy cosmic rays under the supervision of Prof. Dr. Gustavo E. Romero and Prof. Dr. Dr. Johannes Blümer, as well as the advice of Dr. Markus Roth. She graduated from the Double Doctoral degree program in Astrophysics (DDAp), offered jointly by the Karlsruher Institut für Technologie (KIT) and the Universidad Nacional de San Martín (UNSAM). Currently, she is working as a postdoctoral fellow at the Institute of Physics of the Czech Academy of Sciences (CAS) in Prague on a project led by Dr. Anabella Araudo to investigate the production of cosmic rays in jets of active galactic nuclei.
Ana Laura Müller received her Licentiate degree in Astronomy from the Universidad Nacional de La Plata (UNLP). Afterwards, she started her doctoral research focusing on the origin of ultra-high-energy cosmic rays under the supervision of Prof. Dr. Gustavo E. Romero and Prof. Dr. Dr. Johannes Blümer, as well as the advice of Dr. Markus Roth. She graduated from the Double Doctoral degree program in Astrophysics (DDAp), offered jointly by the Karlsruher Institut für Technologie (KIT) and the Universidad Nacional de San Martín (UNSAM). Currently, she is working as a postdoctoral fellow at the Institute of Physics of the Czech Academy of Sciences (CAS) in Prague on a project led by Dr. Anabella Araudo to investigate the production of cosmic rays in jets of active galactic nuclei.