翻訳と辞書
Words near each other
・ Antimafia Commission
・ Antimafia Pool
・ Antimagic square
・ Antimagnetic watch
・ Antimalarial medication
・ Antimaniax
・ Antimanoa
・ Antimargarita
・ Antimargarita bentarti
・ Antimargarita dulcis
・ Antimargarita maoria
・ Antimargarita powelli
・ Antimargarita smithiana
・ Antimaterialism
・ Antimatroid
Antimatter
・ Antimatter (album)
・ Antimatter (band)
・ Antimatter (disambiguation)
・ Antimatter comet
・ Antimatter gravity measurement
・ Antimatter rocket
・ Antimatter tests of Lorentz violation
・ Antimatter weapon
・ Antimatter-catalyzed nuclear pulse propulsion
・ Antimc
・ Antimelatoma
・ Antimelatoma buchanani
・ Antimelatoma buchanani maorum
・ Antimelatoma maoria


Dictionary Lists
翻訳と辞書 辞書検索 [ 開発暫定版 ]
スポンサード リンク

Antimatter : ウィキペディア英語版
Antimatter

In particle physics, antimatter is material composed of antiparticles, which have the same mass as particles of ordinary matter but opposite charges, as well as other particle properties such as lepton and baryon numbers and quantum spin. Collisions between particles and antiparticles lead to the annihilation of both, giving rise to variable proportions of intense photons (gamma rays), neutrinos, and less massive particle–antiparticle pairs. The total consequence of annihilation is a release of energy available for work, proportional to the total matter and antimatter mass, in accord with the mass–energy equivalence equation, .〔(Smidgen of Antimatter Surrounds Earth )〕
Antiparticles bind with each other to form antimatter, just as ordinary particles bind to form normal matter. For example, a positron (the antiparticle of the electron) and an antiproton (the antiparticle of the proton) can form an antihydrogen atom. Physical principles indicate that complex antimatter atomic nuclei are possible, as well as anti-atoms corresponding to the known chemical elements. Studies of cosmic rays have identified both positrons and antiprotons, presumably produced by collisions between particles of ordinary matter. Satellite-based searches of cosmic rays for antideuteron and antihelium particles have yielded nothing.
There is considerable speculation as to why the observable universe is composed almost entirely of ordinary matter, as opposed to a more even mixture of matter and antimatter. This asymmetry of matter and antimatter in the visible universe is one of the great unsolved problems in physics.〔David Tenenbaum, David, (One step closer: UW-Madison scientists help explain scarcity of anti-matter ), University of Wisconsin—Madison News, December 26, 2012〕 The process by which this inequality between particles and antiparticles developed is called baryogenesis.
Antimatter in the form of anti-atoms is one of the most difficult materials to produce. Antimatter in the form of individual anti-particles, however, is commonly produced by particle accelerators and in some types of radioactive decay. The nuclei of antihelium (both helium-3 and helium-4) have been artificially produced with difficulty. These are the most complex anti-nuclei so far observed.
==History of the concept==
The idea of negative matter appears in past theories of matter that have now been abandoned. Using the once popular vortex theory of gravity, the possibility of matter with negative gravity was discussed by William Hicks in the 1880s. Between the 1880s and the 1890s, Karl Pearson proposed the existence of "squirts" and sinks of the flow of aether. The squirts represented normal matter and the sinks represented negative matter. Pearson's theory required a fourth dimension for the aether to flow from and into.
The term antimatter was first used by Arthur Schuster in two rather whimsical letters to ''Nature'' in 1898, in which he coined the term. He hypothesized antiatoms, as well as whole antimatter solar systems, and discussed the possibility of matter and antimatter annihilating each other. Schuster's ideas were not a serious theoretical proposal, merely speculation, and like the previous ideas, differed from the modern concept of antimatter in that it possessed negative gravity.
The modern theory of antimatter began in 1928, with a paper by Paul Dirac. Dirac realised that his relativistic version of the Schrödinger wave equation for electrons predicted the possibility of antielectrons. These were discovered by Carl D. Anderson in 1932 and named positrons (a portmanteau of "positive electron"). Although Dirac did not himself use the term antimatter, its use follows on naturally enough from antielectrons, antiprotons, etc. A complete periodic table of antimatter was envisaged by Charles Janet in 1929.
The Feynman–Stueckelberg interpretation states that antimatter and antiparticles are regular particles traveling backward in time.〔Canetti, L., Drewes, M., and Shaposhnikov, M. (2012). Matter and antimatter in the universe. New J. Phys. 14 (9), 095012.〕

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Antimatter」の詳細全文を読む



スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース

Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.