Spaghettification: The Stretching Power of Black Holes
Spaghettification is the dramatic effect of tidal forces near a black hole, where objects are stretched lengthwise and compressed sideways
Reissner–Nordström Black Hole: Charged but Motionless
The Reissner–Nordström black hole is a solution to Einstein’s field equations that describes a charged, non-rotating black hole. Unlike the
Kerr Metric: The Geometry of a Spinning Black Hole
The Kerr metric is a solution to Einstein’s field equations in general relativity that describes the spacetime geometry around a
Penrose Process: Tapping Energy from a Rotating Black Hole
The Penrose process is a theoretical method for extracting energy from a rotating (Kerr) black hole. It takes advantage of
The Twisting Edge: The Ergosphere
The ergosphere is a fascinating region located just outside the event horizon of a rotating black hole (also known as
Boundary of No Return: The Event Horizon
The event horizon is a critical surface surrounding a black hole that marks the point of no return. Once any
AdS/CFT Correspondence: Bridging Gravity and Quantum Fields
The AdS/CFT correspondence is a groundbreaking idea in theoretical physics that connects two seemingly different frameworks: a gravitational theory in
Holographic Principle: Information Encoded on Boundaries
The holographic principle is a radical idea from theoretical physics proposing that all the information contained within a volume of
Dirac Materials: Electrons Mimicking Relativistic Particles
Dirac materials are a class of solids in which the electrons behave as if they are relativistic, massless particles described
Weyl Semimetals: Exotic Quantum Behavior from Topology
Weyl semimetals are materials where the electronic structure hosts special points known as Weyl nodes, where conduction and valence bands