Category Archives: Notes

Working notes, informal derivations, calculations, and intermediate results. These posts are exploratory in nature and reflect ongoing thought rather than polished exposition.

Why MHD Works in Weakly Collisional Astrophysical Plasmas

Here is a number that should bother you. In the solar wind near the Earth’s orbit the proton density is about $5$ per cubic centimetre and the temperature is around $10^{5}$ K. Work out how far a proton travels before … Continue reading →

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From the Equivalence Principle to Curved Geometry of Spacetime

Newtonian mechanics contains two masses with no obvious reason to be related. One appears in the law of gravitation, $$\mathbf{F}=-\frac{GMm_g}{r^{2}}\hat{\mathbf r},$$ where $m_g$ measures how strongly a body couples to a gravitational field. The other appears in the second law, … Continue reading →

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Why $R_{\mu\nu}=0$ does not imply $R_{\mu\nu\rho\sigma}=0$

Almost everyone makes this mistake once, and it’s a good one to make. You learn the Einstein field equations. You learn that in vacuum, with no matter and no energy and no cosmological constant, they collapse down to something very … Continue reading →

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The rubber sheet gets the geometry right and the mechanism wrong!

You have seen this demonstration. Somebody stretches a rubber sheet over a frame, drops a bowling ball in the middle, and the sheet sags. Then they roll a marble across it and the marble curves toward the bowling ball, maybe … Continue reading →

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A Scientist Before “Scientist”

Mary Somerville is so difficult to put into words that it’s funny. To be honest, who was she? Although you would be correct in calling her a mathematician, you would then be required to clarify the astronomy. The word “astronomer” … 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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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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Inspiral-merger-ringdown consistency tests and the reconstruction of Kerr geometry

One of the more conceptually interesting developments in gravitational wave astronomy is the inspiral-merger-ringdown (IMR) consistency test. At a heuristic level, the idea is rather simple: different sectors of a binary black hole coalescence should reconstruct the same final spacetime … Continue reading →

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A Consistency Test for Kerr Black Holes via Orbital Motion, Ringdown, and Imaging

Kerr Trisector Closure (KTC) is a consistency test for the Kerr hypothesis that tries to stay honest about what is actually being inferred from data. The guiding principle is simple: if the exterior spacetime of an astrophysical, stationary, uncharged black … Continue reading →

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