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Dr Marko Pavlović
marko@matf.bg.ac.rs

Research Assistant
Department of Astronomy
Faculty of Mathematics
University of Belgrade
Studentski trg 16, 11000 Belgrade
Phone: +381 11-2027-827

Curriculum Vitae
ResearchGate, Scopus, ORCID,
Google Scholar, Publications: ADS, arXiv

GitHub



I defended my PhD at the Department of Astronomy, University of Belgrade, under the supervision of Dr Dejan Urošević. My PhD thesis was "Modeling the radio-evolution of supernova remnants by using hydrodynamic simulations and non-linear diffusive shock acceleration". Before that, I obtained both my MSc (2011) and BSc (2010) in astrophysics, from University of Belgrade. I am a Research Assistant at the Department of Astronomy, University of Belgrade and a proud member of Supernova Remnants Group from Belgrade, supported by the Ministry of Education and Science of the Republic of Serbia through the project 176005 Emission nebulae: structure and evolution (PI Dr. Dejan Urošević).

I am interested in supernova remnants and different aspects of cosmic ray acceleration. My work is mostly based on numerical modeling. I am particularly interested in the following topics:

  • Supernova remnants (SNRs)
  • High energy astrophysics
  • Cosmic rays
  • Statistics and Monte Carlo methods
  • MHD and PIC simulations
  • High performance computing

  • Recent Publications:

  • "Searching for an interstellar medium association for HESS J1534 − 571", Maxted, N. I., Braiding, C., Wong, G. F., Rowell, G. P., Burton, M. G., Filipović, M. D., Voisin F., Urošević, D., Vukotić, B., Pavlović, M. Z., Sano, H., Fukui, Y., Mon. Not. R. Astron. Soc., 480, 134 (2018)

  • " A Multi-Frequency Study of the Milky Way-like Spiral Galaxy NGC 6744", Yew, M., Filipović, M. D., Roper, Q., Collier, J. D., Crawford, E. J., Jarrett, T. H., Tothill, N. F. H., O'Brien, A. N., Pavlović, M. Z., Pannuti, T. G., Galvin, T. J., Kapińska, A. D., Cluver, M. E., Banfield, J. K., Schlegel, E. M., Maxted, M., Grieve, K. R., Publ. Astron. Soc. Aust., 35, e015 (2018)

  • "On the foundation of equipartition in supernova remnants", Urošević, D., Pavlović, M. Z., Arbutina, B., Astrophys. J., 855, 59 (2018)

  • "Radio evolution of supernova remnants including non-linear particle acceleration: insights from hydrodynamic simulations", Pavlović, M. Z., Urošević, D., Arbutina, B., Orlando, S., Maxted, N., Filipović, M., Astrophys. J., 852, 84 (2018)

  • "Hydrodynamical and radio evolution of young supernova remnant G1.9+0.3 based on the model of diffusive shock acceleration", Pavlović, M. Z., Mon. Not. R. Astron. Soc., 468, 1616 (2017)

  • "Statistical Analysis of Supernova Remnants in the Large Magellanic Cloud", Bozzetto, L. M., Filipović, M. D., Vukotić, B., Pavlović, M. Z., Urošević, D., Kavanagh, P. J., Arbutina, B., Maggi, P., Sasaki, M., Haberl, F., Crawford, E. J., Roper, Q., Grieve, K., Points, S. D., Astrophys. J. Suppl. Ser., 230, 2 (2017)

  • "Radio evolution of supernova remnants including non-linear particle acceleration", Pavlović, M. Z., Supernova Remnants: An Odyssey in Space after Stellar Death, Proceedings of the Conference held 6-11 June 2016, in Chania, Greece. Online at http://snr2016.astro.noa.gr, 102