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MORE ABOUT ME

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In January 2022, I was selected for Asigmo GmbH's Data Science bootcamp (300+ hrs) as an Asigmo Data Science Fellow.

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In October 2017, I joined the University of Amsterdam's Anton Pannekoek Research Institute (API) as a post-doctoral researcher in Prof. Sera Markoff's research group. Here my research work focused on semi-analytically modeling of jets from black holes.

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I obtained my PhD (Physics) from Oregon State University in 2017, under the supervision of Prof. Davide Lazzati. During my PhD I studied Gamma-ray bursts (GRBs) and Active Galactic Nuclei (AGNs). You can read more about these fascinating objects below.

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Surprisingly, besides doing astrophysics and thinking about the universe I also enjoy doing other things in life! These include and are not limited to reading (not only astro stuff!), racket sports, working out (weight training, cross-fit, HIIT), and hiking.

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Oh, and by the way, I hail from New Delhi, India.

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MORE ABOUT MY RESEARCH

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Jets are funnel shaped ultra-fast (they almost travel as fast as light) ejections of matter. It is natural to ask how black holes, which don't even allow light to escape, are somehow failing to not just trap matter but somehow propelling it to speeds almost as fast as light! This is the question that my work in Amsterdam focused upon. I investigated how strong gravity (General Relativity or GR) guides the interaction between matter/plasma and magnetic fields (Magnetohydrodynamics), in short GRMHD. Employing GRMHD, I developed a semi-analytical model to describe how jets can be launched from the vicinity of black holes.

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Gamma Ray Bursts (GRBs for short) are one of the most powerful explosions in the universe. Mankind now regularly detects them in space as extremely energetic bursts of gamma rays. These explosions are believed to be associated with the formation of a dense, compact object and with the ejection of matter at extremely fast speeds. The ejected stuff is called an outflow (or a jet) as it flows outward from the compact object.

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AGNs are extremely luminous core of galaxies, believed to harbor a super-massive black hole (imagine a black hole having the same mass as millions of our suns!) at their center. Many of these giant black holes have been seen spewing copious amounts of matter outwards (just like an outflow), also, at really fast speeds.  

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My PhD research explored how light (or to be specific, electromagnetic radiation) can accelerate outflows to extremely high speeds. It involved a lot of theoretical work, coding, and simulations - it was hard but really fun! 

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RESEARCH INTERESTS

EDUCATION

January - April 2022 

Asigmo GmbH

Data Science Fellow

General Relativistic Magnetohydrodynamics (GRMHD)

Self--similar solutions to equations of GRMHD

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Gamma-ray Bursts (Prompt Emission, Jets)

The origin of prompt emission of gamma-rays from GRBs

2011 - 2014

North Carolina State University

Graduate Student

Radiative Acceleration and Radiative Processes

2005 - 2010

Birla Institute of Technology and Science, Pilani

B.E. (Hons) Electrical and Electronics Engineering and MSc. (Hons) Physics

Active Galactic Nuclei (Emissions, Jets)

Spine-sheath structured jets

2014 - 2017

Oregon State University

Graduate Student

Machine Learning, AI

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