uncharged hole

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• Timeline of black hole physics — Timeline of black hole physics* 1640 Ismael Bullialdus suggests an inverse square gravitational force law * 1684 Isaac Newton writes down his inverse square Law of universal gravitation * 1758 Rudjer Josip Boscovich develops his Theory of forces …   Wikipedia

• Schwarzschild black hole — noun An uncharged (q = 0), nonrotating (L = 0) black hole. See Also: Schwarzschild circumference, Schwarzschild metric, Schwarzschild radius …   Wiktionary

• Kerr black hole — noun An uncharged (q = 0), rotating (L ≠ 0) black hole …   Wiktionary

• radiation measurement — ▪ technology Introduction       technique for detecting the intensity and characteristics of ionizing radiation, such as alpha, beta, and gamma rays or neutrons, for the purpose of measurement.       The term ionizing radiation refers to those… …   Universalium

• Kerr metric — In general relativity, the Kerr metric (or Kerr vacuum) describes the geometry of spacetime around a rotating massive body. According to this metric, such rotating bodies should exhibit frame dragging, an unusual prediction of general relativity; …   Wikipedia

• Casimir effect — Casimir forces on parallel plates Casimir forces on parallel pl …   Wikipedia

• electricity — /i lek tris i tee, ee lek /, n. 1. See electric charge. 2. See electric current. 3. the science dealing with electric charges and currents. 4. a state or feeling of excitement, anticipation, tension, etc. [1640 50; ELECTRIC + ITY] * * *… …   Universalium

• Bagram torture and prisoner abuse — In 2005, The New York Times obtained a 2,000 page United States Army report concerning the homicides of two unarmed civilian Afghan prisoners by U.S. armed forces in 2002 at the Bagram Theater Internment Facility (also Bagram Collection Point or… …   Wikipedia

• Hawking radiation — is a thermal radiation with a black body spectrum predicted to be emitted by black holes due to quantum effects. It is named after the physicist Stephen Hawking, who provided a theoretical argument for its existence in 1974, and sometimes also… …   Wikipedia

• Properties and features of black holes — According to the No Hair theorem a black hole has only three independent physical properties: mass, charge and angular momentum. [citation|last=Heusler |first=M. |year=1998 |title=Stationary Black Holes: Uniqueness and Beyond |journal=Living Rev …   Wikipedia

• Holographic principle — Holographic Universe redirects here. For the album, see Holographic Universe (album). For the book by Michael Talbot, see The Holographic Universe. String theory …   Wikipedia