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G. Mamatsashvili

15 papers hereh-index 13374 citations21 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author8
  • last author1

Across the 14 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP7
  • astro-ph.HE4
  • astro-ph2
  • astro-ph.SR2
same name
  • G. Mamatsashvili — 24 papers, h 9
  • G. Mamatsashvili — 6 papers, h 7
  • G. Mamatsashvili — 2 papers
  • G. Mamatsashvili — 2 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20072024
most citedStability of self-gravitating discs under irradiation

84 citations · 425 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2024

Evolution of current and pressure driven instabilities in relativistic jets

M. Musso, G. Bodo, G. Mamatsashvili +2

Instabilities in relativistic magnetized jets are thought to be deeply connected to their energy dissipation properties and to the consequent acceleration of the non-thermal emitti…

astro-ph.HE2021

Current driven kink instabilities in relativistic jets: dissipation properties

G. Bodo, G. Mamatsashvili, P. Rossi +1

We analyze the evolution of current driven kink instabilities of a highly magnetized relativistic plasma column, focusing in particular on its dissipation properties. The instabili…

astro-ph.HE2016★ 29 cited

Linear stability analysis of magnetized jets: the rotating case

G. Bodo, G. Mamatsashvili, P. Rossi +1

We perform a linear stability analysis of magnetized rotating cylindrical jet flows in the approximation of zero thermal pressure. We focus our analysis on the effect of rotation o…

astro-ph.HE2013★ 68 cited

Linear stability analysis of magnetized relativistic jets: the nonrotating case

G. Bodo, G. Mamatsashvili, P. Rossi +1

We perform a linear analysis of the stability of a magnetized relativistic non-rotating cylindrical flow in the aproximation of zero thermal pressure, considering only the m = 1 mo…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.