Einstein Field Equations

The Paschen-Back effect occurs in the presence of a very strong magnetic field, where the Zeeman splitting energy becomes much larger than the fine-structure (spin-orbit) interaction energy. In this regime, the coupling between orbital (\(\vec{L}\)) and spin (\(\vec{S}\)) angular momentum is broken. They precess independently around the strong external magnetic field, simplifying the spectral pattern.

A key prediction of general relativity is that time passes at different rates in different gravitational potentials. A clock in a stronger gravitational field (closer to a massive object) will tick slower than a clock in a weaker field. This effect, known as gravitational time dilation, has been experimentally verified and is a crucial factor in modern technology like GPS.

General relativity predicts that the path of light is bent by gravity. When light from a distant source passes a massive object like a galaxy or a star, its path is deflected. This phenomenon, known as gravitational lensing, can magnify, distort, or create multiple images of the background source, acting like a cosmic telescope for observing the distant universe.

Redox (reduction-oxidation) reactions involve a transfer of electrons between chemical species. One species undergoes oxidation (loses electrons), while another undergoes reduction (gains electrons). These two processes always occur simultaneously. The species that loses electrons is the reducing agent, and the one that gains electrons is the oxidizing agent. This fundamental concept underpins electrochemistry and many biological processes.

The equivalence principle is a cornerstone of general relativity. It posits that the effects of a uniform gravitational field are indistinguishable from the effects of uniform acceleration. This means that an observer in a windowless, free-falling elevator experiences weightlessness, just like an observer in deep space, far from any gravitational source, forming the conceptual basis for gravity as a geometric phenomenon.

The von Mises yield criterion predicts that yielding of a ductile material begins when the second deviatoric stress invariant, \(J_2\), reaches a critical value. It is often expressed in terms of the von Mises stress, \(\sigma_v\), a scalar value that must be less than the material's yield strength, \(\sigma_y\). Yielding occurs when \(\sigma_v = \sigma_y\).

General relativity provided the first accurate explanation for the anomalous precession of Mercury's perihelion. Newtonian gravity could not fully account for the slow, gradual shift in the orientation of Mercury's elliptical orbit. Einstein's theory correctly predicted the missing 43 arcseconds per century, attributing it to the curvature of spacetime around the Sun, a major early triumph for the theory.

A black hole is a region of spacetime where gravity is so strong that nothing—no particles or even light—can escape. The boundary of this region is called the event horizon. Predicted by general relativity as a solution to the field equations, a black hole is the result of the complete gravitational collapse of a massive star.

General relativity predicts that a massive, rotating object should 'drag' the fabric of spacetime around with it, a phenomenon known as frame-dragging or the Lense-Thirring effect. This means a gyroscope orbiting the rotating body will precess, not because of any applied torque, but because spacetime itself is being twisted by the body's rotation.

Complex redox reactions can be balanced using the half-reaction method. The overall reaction is split into two separate half-reactions: one for oxidation and one for reduction. Each half-reaction is balanced for atoms and charge independently, often by adding H+, OH-, and H2O in aqueous solutions. Finally, the electron counts are equalized and the half-reactions are combined.