Author Archives: Aronno Mirdha

About Aronno Mirdha

I am a theoretical physics student working on general relativity and black hole physics. My research builds statistical tools for testing whether independent observations of the same black hole, from gravitational waves to shadow imaging to stellar dynamics, all agree on a single underlying geometry.

So, what is a vector?

In my first year of undergraduate physics, one of my professors walked into the lecture hall, placed his notes on the desk, looked around the room, and asked a question that, at first, seemed almost too easy. “What is a … Continue reading →

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Deriving the Euler–Lagrange Equation for Particles, Fields, and Curved Spacetime

A good way to understand the laws of motion is not to memorize a separate equation for each situation, but to notice there is really only one trick, and every equation of motion is what falls out when you apply … Continue reading →

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So what are tensors, really?

I want to start with a confession. When I first heard the word “tensor,” I assumed it was one of those words that exists to make physicists sound clever. Something you learn in graduate school, surrounded by people who already … Continue reading →

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On physics, visibility, and why I stayed

I remember being in high school and telling people I wanted to study physics. The response was almost always the same. Not discouragement exactly, more like mild concern, the kind adults give you when they think you are about to … Continue reading →

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The mathematics behind a “wormhole”

Let me tell you something that will sound ridiculous at first. Take a piece of paper. Draw a dot on the left and a dot on the right. The shortest path between them, if you are a little ant walking … Continue reading →

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How many solutions of Einstein’s equations are there?

How many solutions does the most beautiful equation in physics have? More than you’d think… probably infinitely many, and most of them will never have names. Continue reading →

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On the Consistency of Published M87* Mass Measurements

A useful way to test a black hole spacetime is not only to ask whether one observational method agrees with Kerr, but to ask whether several independent methods agree with each other. In the case of M87*, this question is … Continue reading →

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Some remarks on quasinormal modes for Euler–Heisenberg black holes in a PFDM background

One of the recurring themes in black hole perturbation theory is that many apparently complicated dynamical questions eventually reduce to a rather geometric spectral problem. One begins with a black hole spacetime, perturbs it slightly, separates variables, and discovers that … Continue reading →

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Aristotle on Motion

Aristotle divided motion into two classes: natural motion and violent motion. These ideas are not really part of modern physics anymore, but they are important because they were among the first serious attempts to explain motion logically rather than through … Continue reading →

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Recent notes on covariance-weighted consistency tests for Kerr parameter estimates

A recurring issue in strong-field tests of General Relativity is the question of how one should compare parameter estimates inferred from genuinely independent observational sectors. In the case of stationary black hole spacetimes, the Kerr hypothesis predicts that all sufficiently … Continue reading →

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