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[[Image:Blackhole3.jpg|right|thumb|A black hole at the center of a [[galaxy]], NASA image]]
[[Image:Blackhole3.jpg|right|thumb|A black hole at the center of a [[galaxy]], NASA image]]


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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. <ref>Wood, C. (2019). [https://www.livescience.com/65700-big-bang-theory.html The Big Bang Theory: How the Universe Began], Live Science.</ref> The framework of the Big Bang Theory and nuclear physics was later constructed into the cosmic interpretations of the theoretical celestial object.
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. <ref>Wood, C. (2019). [https://www.livescience.com/65700-big-bang-theory.html The Big Bang Theory: How the Universe Began], Live Science.</ref> 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, primordial black hole and the normative black hole. Primordial black holes are thought to be created not soon after the Big Bang, and the normative black holes 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|singularity]], it must have a mass greater than 3.4 times that of the Sun.
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|singularity]], it must have a mass greater than 3.4 times that of the Sun.


== Characteristics ==
== Characteristics ==


Quite a few features have been attributed to black holes in observational astronomy, among which include its Bolometric luminosity, denoted by L<sub>Bol</sub>, 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 [[infinity|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.
Quite a few features have been attributed to black holes in observational astronomy, among which include its Bolometric luminosity, denoted by L<sub>Bol</sub>, absolute magnitude, the widely known event horizon and [[singularity]], Hawking radiation and Hawking points, and active galactic nuclei, etc.  <ref>Daly, R. A. (2020). [https://sites.psu.edu/rdaly/476-2/ New Methods of Measuring Black Hole Spin and Accretion Disk Properties], Caltech Tea Talk, The Pennsylvania State University.</ref> 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 [[infinity|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 ===
=== 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. <ref>Herman, R. L. (2021). [http://people.uncw.edu/hermanr/BlackHoles/Kerr_Metric_II.pdf#:~:text=The%20Kerr%20solution%20di%0Bers%20from%20theSchwarzschild%20in%20that,free%20to%20change%20direction%20inr%3B%20by%20pass%20thesingularity. Notes on the Kerr Metric], PHY 490 The Physics of Black Holes, University of North Carolina Wilmington.</ref> The ergoregions are composed the outer ergosphere and inner ergosphere, beyond which are the ring singularity and singularity. <ref>Sutter, P. (2022). [https://www.livescience.com/are-black-holes-wormholes Are black holes wormholes?], Live Science.</ref>
Kerr's exact solutions of general relativity postulate that rotating black holes, namely Kerr and Kerr-Newman black holes, have two event horizons. Beyond the outer event horizon are the inner event horizon and ergoregions. <ref>Herman, R. L. (2021). [http://people.uncw.edu/hermanr/BlackHoles/Kerr_Metric_II.pdf#:~:text=The%20Kerr%20solution%20di%0Bers%20from%20theSchwarzschild%20in%20that,free%20to%20change%20direction%20inr%3B%20by%20pass%20thesingularity. Notes on the Kerr Metric], PHY 490 The Physics of Black Holes, University of North Carolina Wilmington.</ref> The ergoregions are composed of the outer ergosphere and inner ergosphere, beyond which are the ring singularity and singularity. <ref>Sutter, P. (2022). [https://www.livescience.com/are-black-holes-wormholes Are black holes wormholes?], Live Science.</ref>
 
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. <ref>Bardeen, J. M., Carter, B., and Hawking, S. W. (1973). The four laws of black hole mechanics. ''Communications in Mathematical Physics, 31''(2): 161-170. DOI: [http://doi.org/10.1007/BF01645742 10.1007/BF01645742]</ref> 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) located in the [[United States of America|U.S.]] became feasible. <ref>Chu, J. (2021). [https://news.mit.edu/2021/hawkings-black-hole-theorem-confirm-0701 Physicists observationally confirm Hawking’s black hole theorem for the first time], MIT News.</ref>
 
=== Observation of Black Holes ===
 
The concentration of mass by black holes with their basic properties has made [[Gravitational lens|gravitational lensing]] the optimal technique for black hole observation. <ref>[https://hubblesite.org/contents/articles/gravitational-lensing Gravitational Lensing], Space Telescope Science Institute.</ref> A multitude of spectra has been adopted in the surveys, and observation by [[Gravitational wave|gravitational wave]] detection with interferometry has been the recent development since 2015, apart from Virgo in Italy. <ref>[https://www.ligo.caltech.edu/page/what-is-ligo What is LIGO?], LIGO Caltech.</ref> Like all other astronomical observations, the ideal site for detection is beyond the earth's atmosphere. The preferences of eliminating detection biases from the atmospheric environment have categorized telescopes into ground-based and space-based. Placing telescopes in the aerospace mounted on high altitude planes has also been adopted. <ref name="history">Walker, H. J. (2000). A brief history of infrared astronomy. ''Astronomy & Geophysics, 41''(5): 5.10–5.13. DOI: [https://doi.org/10.1046/j.1468-4004.2000.41510.x 10.1046/j.1468-4004.2000.41510.x]</ref>
 
==== Observational Signatures ====


According to [[quantum mechanics]], the location of the matter within a black hole is [[quantum uncertainty|uncertain]]. Additionally, a phenomenon called Hawking radiation predicts that black holes can "leak" a very small amount of mass. So theoretically, black holes are not truly "black" due to emitted radiation. Black holes have a surface temperature defined by their mass. The larger the [[mass]] of a black hole, the larger the diameter, and the lower the amount of energy which escapes, thus the lower the temperature, and the longer the time it takes for the black hole to "evaporate".
While black hole mergers are easier to detect than isolated black holes, black holes with spins are easier to detect than those without, especially Schwarzchild black holes. <ref>Daly, R. A. (2021). [https://sites.psu.edu/rdaly/losoncy-lecture-ruth-daly-april-9-2021/ Public Lecture – 9<sup>th</sup> Annual Losoncy Lecture – Black Holes in Galaxies across the Universe], Penn State University, Berks Campus.</ref> Black hole observations typically involve accretion disk, event horizon, long tail of stars, black hole shadows, black hole seeds, etc. <ref>Torbet, G. (2023). [https://www.digitaltrends.com/space/black-hole-tail-star-formation/#:~:text=The%20lonely%20black%20hole%20has%20been%20traveling%20space,as%20long%20as%20the%20Milky%20Way%20is%20wide. Unique black hole is trailed by 200,000 light-year-long tail of stars], Digital Trends Media Group.</ref> <ref>Ricarte, A. & Natarajan, P. (2018). The observational signatures of supermassive black hole seeds. ''Monthly Notices of the Royal Astronomical Society, 481''(3): 3278-3292. DOI: [https://doi.org/10.1093/mnras/sty2448 10.1093/mnras/sty2448]</ref> <ref>The Nature of Reality (2015). [https://www.pbs.org/wgbh/nova/article/the-shadow-of-a-black-hole/ The Shadow of a Black Hole], Public Broadcasting Service.</ref>


=== Detection and Observation of Black Holes ===
==== Observational Histories ====


Methods of detecting and observing black holes include imaging using radio telescopes and also gravitational wave detection.
The first black hole ever discovered was Cygnus X-1 in 1964. Cygnus X-1 is located within the Milky Way in the constellation of Cygnus, the Swan. <ref>Choi, C. Q. (2021). [https://www.space.com/first-discovered-black-hole-larger-than-thought Scientists revisit the 1st black hole they ever discovered and realize it's bigger than they thought]. Space.com.</ref> While early detections mainly utilized the X-ray and gamma-ray emitted from the believed accretion activities, infrared astronomy developed in 1967 when the Mauna Kea Observatories site for astronomy was founded 4200 m above sea-level on an extinct volcano in Hawaii. <ref name="history" />


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.
== References ==


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.
<references />

Latest revision as of 07:30, 31 July 2023

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. [1] The term black hole for the then-theoretical celestial object was coined later by John Wheeler. [2] 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: [3]

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. [4] 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 LBol, absolute magnitude, the widely known event horizon and singularity, Hawking radiation and Hawking points, and active galactic nuclei, etc. [5] 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, namely Kerr and Kerr-Newman black holes, have two event horizons. Beyond the outer event horizon are the inner event horizon and ergoregions. [6] The ergoregions are composed of the outer ergosphere and inner ergosphere, beyond which are the ring singularity and singularity. [7]

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. [8] 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) located in the U.S. became feasible. [9]

Observation of Black Holes

The concentration of mass by black holes with their basic properties has made gravitational lensing the optimal technique for black hole observation. [10] A multitude of spectra has been adopted in the surveys, and observation by gravitational wave detection with interferometry has been the recent development since 2015, apart from Virgo in Italy. [11] Like all other astronomical observations, the ideal site for detection is beyond the earth's atmosphere. The preferences of eliminating detection biases from the atmospheric environment have categorized telescopes into ground-based and space-based. Placing telescopes in the aerospace mounted on high altitude planes has also been adopted. [12]

Observational Signatures

While black hole mergers are easier to detect than isolated black holes, black holes with spins are easier to detect than those without, especially Schwarzchild black holes. [13] Black hole observations typically involve accretion disk, event horizon, long tail of stars, black hole shadows, black hole seeds, etc. [14] [15] [16]

Observational Histories

The first black hole ever discovered was Cygnus X-1 in 1964. Cygnus X-1 is located within the Milky Way in the constellation of Cygnus, the Swan. [17] While early detections mainly utilized the X-ray and gamma-ray emitted from the believed accretion activities, infrared astronomy developed in 1967 when the Mauna Kea Observatories site for astronomy was founded 4200 m above sea-level on an extinct volcano in Hawaii. [12]

References

  1. ↑ Schnittman, J. (2019). A brief history of black holes, Astronomy magazine.
  2. ↑ Overbye, D. (2008). John A. Wheeler, Physicist Who Coined the Term ‘Black Hole,’ Is Dead at 96, New York Times.
  3. ↑ Pachankis, Y. I. (2022). Neutron Number Asymmetry in Proton Decay Momentum, Journal of Agricultural, Earth & Environmental Sciences, 1(1): 1-9. Bibcode: 2022JAEES...1....1P
  4. ↑ Wood, C. (2019). The Big Bang Theory: How the Universe Began, Live Science.
  5. ↑ Daly, R. A. (2020). New Methods of Measuring Black Hole Spin and Accretion Disk Properties, Caltech Tea Talk, The Pennsylvania State University.
  6. ↑ Herman, R. L. (2021). Notes on the Kerr Metric, PHY 490 The Physics of Black Holes, University of North Carolina Wilmington.
  7. ↑ Sutter, P. (2022). Are black holes wormholes?, Live Science.
  8. ↑ Bardeen, J. M., Carter, B., and Hawking, S. W. (1973). The four laws of black hole mechanics. Communications in Mathematical Physics, 31(2): 161-170. DOI: 10.1007/BF01645742
  9. ↑ Chu, J. (2021). Physicists observationally confirm Hawking’s black hole theorem for the first time, MIT News.
  10. ↑ Gravitational Lensing, Space Telescope Science Institute.
  11. ↑ What is LIGO?, LIGO Caltech.
  12. ↑ 12.0 12.1 Walker, H. J. (2000). A brief history of infrared astronomy. Astronomy & Geophysics, 41(5): 5.10–5.13. DOI: 10.1046/j.1468-4004.2000.41510.x
  13. ↑ Daly, R. A. (2021). Public Lecture – 9th Annual Losoncy Lecture – Black Holes in Galaxies across the Universe, Penn State University, Berks Campus.
  14. ↑ Torbet, G. (2023). Unique black hole is trailed by 200,000 light-year-long tail of stars, Digital Trends Media Group.
  15. ↑ Ricarte, A. & Natarajan, P. (2018). The observational signatures of supermassive black hole seeds. Monthly Notices of the Royal Astronomical Society, 481(3): 3278-3292. DOI: 10.1093/mnras/sty2448
  16. ↑ The Nature of Reality (2015). The Shadow of a Black Hole, Public Broadcasting Service.
  17. ↑ Choi, C. Q. (2021). Scientists revisit the 1st black hole they ever discovered and realize it's bigger than they thought. Space.com.
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