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Gravitational waveforms from periodic orbits around a dyonic ModMax black hole

  • Mirzabek Alloqulov*
  • , Sanjar Shaymatov
  • , Bobomurat Ahmedov
  • , Tao Zhu
  • *Corresponding author for this work
  • School of Physics, Harbin Institute of Technology
  • University of Tashkent for Applied Sciences
  • New Uzbekistan University
  • Tashkent Institute of Irrigation and Agricultural Mechanization Engineers
  • Academy of Sciences of the Republic of Uzbekistan
  • Tashkent State Technical University
  • Western Caspian University
  • National University of Uzbekistan named after Mirzo Ulugbek
  • Zhejiang University of Technology

Research output: Contribution to journalArticlepeer-review

Abstract

In this work, we study the gravitational waveforms from the periodic orbits of a massive particle around a dyonic ModMax black hole. We begin with a brief analysis of the spacetime and then examine how its parameters influence the dynamics of a massive neutral particle using the Lagrangian formalism. In particular, we compute the characteristics of marginally bound orbits and innermost stable circular orbits. Our results show that the values of these quantities increase with the black hole charge Q and the screening parameter γ. We then plot various periodic orbits, characterized by the integers (z,w,v). Finally, we present the gravitational waveforms associated with extreme mass ratio inspirals, consisting of a stellar-mass compact object orbiting a supermassive black hole.

Original languageEnglish
Article number259
JournalEuropean Physical Journal C
Volume86
Issue number3
DOIs
StatePublished - Mar 2026
Externally publishedYes

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