Fear Street - Prom Queen (2025) (Hindi + English) Dual Audio Hollywood Movie HD ESub
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Published 五月 30, 2025
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Types of Black Holes
1. Stellar-Mass Black Holes
Formed from the collapse of massive stars (typically over 20 times the mass of the Sun).
Mass ranges from about 3 to 50 solar masses.
Common in binary star systems and are the sources of many gravitational wave detections.
2. Supermassive Black Holes
Found at the centers of galaxies, including our own Milky Way.
Mass ranges from millions to billions of solar masses.
Example: Sagittarius A* is the supermassive black hole at the center of the Milky Way (~4 million solar masses).
3. Intermediate-Mass Black Holes
Hypothetical class with masses between 100 and 100,000 solar masses.
Harder to detect but may form through the merging of stellar black holes or in dense star clusters.
4. Primordial Black Holes
Theoretical black holes formed shortly after the Big Bang.
Could range in mass from tiny to massive.
Some theories propose they might contribute to dark matter.
Name: Fear Street - Prom Queen (2025) (Hindi + English) Dual Audio Hollywood Movie HD ESub
Genre: Horror | Thriller
Anatomy of a Black Hole
1. Singularity
The core where matter is crushed into infinite density.
Current physics breaks down here; quantum gravity theories are needed.
2. Event Horizon
The boundary beyond which nothing can escape.
Not a physical surface—more like a mathematical limit.
3. Accretion Disk
A swirling disk of gas and dust falling into the black hole.
Emits immense radiation (X-rays, gamma rays) as material heats up due to friction and gravitational forces.
4. Jets
Some black holes, especially supermassive ones, eject powerful jets of particles from their poles.
Duration: 1 hours 30 minutes
Release Date: 2025
Observing the Invisible
Despite their name, black holes are not entirely invisible. Astronomers detect them through their effects on nearby matter and light:
Gravitational Waves: Detected when black holes collide (e.g., by LIGO and Virgo).
X-ray Emissions: From hot gas in the accretion disk.
Stellar Motion: Observing stars orbiting an invisible massive object.
Direct Imaging: As in the EHT's 2019 image, capturing the "shadow" of the event horizon.
Language: Hindi + English
Starcast: India Fowler, Suzanna Son, Fina Strazza, Chris Klein, David Iacono, Ella Rubin, Ariana Greenblatt, Lili Taylor, Katherine Waterston, Dale Whibley, Damian Romeo, Rebecca Ablack, Joanne Boland, Eden Summer Gilmore.
Black Holes and the Laws of Physics
1. General Relativity
Describes the macroscopic properties of black holes—how they curve spacetime and influence their surroundings.
2. Quantum Mechanics
Black holes challenge quantum theory, especially concerning the information paradox: if information is lost in a black hole, it contradicts quantum laws stating information must be preserved.
3. Hawking Radiation
In 1974, Stephen Hawking proposed that black holes emit radiation due to quantum effects near the event horizon, causing them to slowly evaporate. This bridged quantum mechanics and general relativity, but raised new questions about black hole thermodynamics and entropy.
Size: 400mb 1Gb 2.2Gb HD
Description: As students at Shadyside High are preparing for the 1988 prom, the are fighting to get support to be voted Prom Queen. As an unusual nominee emerges in the race, some of the other candidates begin to vanish without a trace.
Black Holes and the Universe
1. Galactic Architects
Supermassive black holes may play a critical role in galaxy formation and evolution, regulating star formation through their energy output.
2. Cosmic Timekeepers
Merging black holes help astronomers measure the rate of expansion of the universe through gravitational wave observations.
3. Dark Matter Candidates
While not a leading theory, some hypothesize that primordial black holes could account for some portion of dark matter.
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Mysteries and Theories
1. Wormholes
Black holes may be connected to hypothetical wormholes—tunnels through spacetime that could, in theory, allow faster-than-light travel or time travel.
2. White Holes
A speculative "opposite" of black holes, white holes could emit matter and energy but not allow anything to enter.
3. Black Hole Entropy and the Holographic Principle
Physicists like Gerard 't Hooft and Leonard Susskind suggest that information falling into a black hole is encoded on its surface, not lost—supporting the holographic theory of the universe.
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