Black hole

A black hole at the center of a galaxy, NASA image

The theory of black holes was conceived by Karl Schwarzschild during World War II. The term black hole for the then-theoretical celestial object was coined later by John Wheeler. Black holes are thought to have the escape velocity faster than the speed of light, which means not even light can escape their gravitational fields. Currently, most astronomical scientists have reached the consensus that black holes exist at the center of every galaxy.

Physical Properties

Black holes can only be described by their spin, charge, and angular momentum, with other attributes derived from the basic properties. They are thought in classical cosmology, i.e. the Big Bang model, to be the result of collapsing matter following the explosion of large stars into supernovae. Therefore, the mass of a black hole is often depicted in terms of solar mass, denoted by m_⊙.ּּ

With their basic physical properties, four types of black holes have been proposed by theoretical physicists, with each type named in honor of them:

Types of Black Hole

Name	Charge	Spin
Schwarzchild black hole	No	No
Kerr black hole	No	Yes
Kerr-Newman black hole	Yes	Yes
Reissner-Nordström black hole	Yes	No

The Big Bang Interpretations

The idea of the universe starting out from an atom originated from the Belgian physicist contemporary to Einstein's time, George Lemaître. On March 28, 1949, the English astronomer Fred Hoyle popularized the phrase the "Big Bang" during a defense. The framework of the Big Bang Theory and nuclear physics was later constructed into the cosmic interpretations of the theoretical celestial object.

Two types of black holes are categorized in the Bang Bang model according to the origins, primordial black hole and the normative black hole from stellar remnants. Primordial black holes are thought to be created not soon after the Big Bang, and the black holes from stellar remnants are thought to be created after a star exhausted its capacities for nuclear fusion. It is estimated that for a star to be capable of compaction into a singularity, it must have a mass greater than 3.4 times that of the Sun.

Characteristics

Quite a few features have been attributed to black holes in observational astronomy, among which include its Bolometric luminosity, denoted by L_Bol, absolute magnitude, the widely known event horizon and singularity, Hawking radiation and Hawking points, and active galactic nuclei, etc. The stellar remnant belief of black hole postulates that the event horizon is the threshold in space where the gravitational force surpasses the velocity of light, and relativity theory postulates the singularity being a point of infinite spacetime curvature. To an outside observer, objects falling into a black hole will take an infinite amount of time to reach the event horizon. The amount of time as measured by the object falling into the black hole, however, can be very short.

Metrics in the Quantum Realm

Kerr's exact solutions of general relativity postulate that rotating black holes have two event horizons, namely Kerr and Kerr-Newman black holes. Beyond the outer event horizon are the inner event horizon and ergoregions. The ergoregions are composed of the outer ergosphere and inner ergosphere, beyond which are the ring singularity and singularity.

The astronomical developments in black hole detection started the quantization. James M. Bardeen, Brandon D. Carter, and Stephen W. Hawking formulated four laws concerning black hole thermodynamics for the foundation of cryogenic technology applied in quantum sensing. Even though Hawking proposed black hole evaporation theories before, contradictions emerged with the observational confirmation of Hawking's surface area law by Isi and his colleagues, after gravitational wave detection by Laser Interferometer Gravitational-Wave Observatory (LIGO) became feasible.

Detection and Observation of Black Holes

Methods of detecting and observing black holes include imaging using radio telescopes and also gravitational wave detection.

In 2015, the two LIGO (Laser Interferometer Gravitational-Wave Observatory) detectors in the USA made the first-ever detection of gravitational waves, which were emitted by two colliding black holes that were approximately 29 and 36 times as massive as the Sun. Since then, the Virgo detector in Italy has also contributed to gravitational wave detection.

In 2019, a direct image of a black hole was made using the Event Horizon Telescope, which is actually a worldwide network of radio telescopes. This black hole is 6.5 billion times more massive than the Sun and located 55 million light-years away in the galaxy M87.