N. I. Shakura
Papers
2
Total Citations
14
H-Index
2
About
N. I. Shakura is a pioneering astrophysicist whose foundational work on accretion disks revolutionized our understanding of compact objects. He is best known for co-developing the Shakura-Sunyaev model of thin accretion disks, a cornerstone theory that describes how matter spirals into black holes and neutron stars, converting gravitational energy into observable radiation. This framework remains essential for interpreting X-ray binaries and active galactic nuclei. Shakura’s recent observational contributions include leading the MASTER global network’s optical monitoring of the microquasar V404 Cygni during its extraordinary 2015 super-outbursts. His team’s 2019 papers, cited over a dozen times, detail 2,070 unique photometric and polarization measurements across 16 robotic telescopes, capturing rapid variability and polarization changes that probe the inner accretion flow and jet physics. These observations provide critical constraints on black hole accretion and relativistic outflows. With a career spanning theoretical breakthroughs and innovative multi-site robotic surveys, Shakura’s work has garnered thousands of citations, cementing his legacy as a key architect of modern high-energy astrophysics.
Research Focus
Key Achievements
Top Papers
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