ব্ল্যাক হোল Black hole and Supermassive Black hole explained in bangla with animation Ep 49

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This video about black hole and supermassive black hole.
Video chapter:
00:00 - intro about black hole
01:08 - what is black hole
01:51 - first concept of black hole
02:56 - how create black hole
04:03 - how we detect black hole
07:18 - black hole accretion disk
08:45 - black hole jets
09:31 - quasar
11:45 - Is the center of the Milky Way a black hole
14:13 - black hole size comparison
14:42 - how create supermassive black hole
15:49 - eddington limit
16:42 - james webb telescope
17:01 - LIGO (Laser Interferometer Gravitational-wave Observatory)
18:46 - first signal of gravitational waves
19:45 - can we create a black hole on earth
20:29 - future of black holes

A black hole is a region of spacetime where gravity is so strong that nothing—no particles or even electromagnetic radiation such as light—can escape from it.The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.The boundary of no escape is called the event horizon. Although it has an enormous effect on the fate and circumstances of an object crossing it, according to general relativity it has no locally detectable features.In many ways, a black hole acts like an ideal black body, as it reflects no light.Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe directly.

Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace.The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, and its interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were long considered a mathematical curiosity; it was not until the 1960s that theoretical work showed they were a generic prediction of general relativity. The discovery of neutron stars by Jocelyn Bell Burnell in 1967 sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality. The first black hole known as such was Cygnus X-1, identified by several researchers independently in 1971.

Black holes of stellar mass form when very massive stars collapse at the end of their life cycle. After a black hole has formed, it can continue to grow by absorbing mass from its surroundings. By absorbing other stars and merging with other black holes, supermassive black holes of millions of solar masses (M☉) may form. There is consensus that supermassive black holes exist in the centers of most galaxies.

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