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Titre	Black Holes: The Membrane Paradigm
Qualité	Sonic 44.1 kHz
Fichier	black-holes-the-memb_yqIwu.epub
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Libéré	1 year 10 months 12 days ago
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Des pages	116 Pages
Une longueur de temps	50 min 15 seconds

Black Holes: The Membrane Paradigm

Catégorie: Histoire, Tourisme et voyages
Auteur: Janet W. Hardy
Éditeur: Adrian Tchaikovsky, Louise Bay
Publié: 2019-12-25
Écrivain: Keri E. Iyall Smith
Langue: Chinois, Latin, Tchèque, Arabe, Russe
Format: pdf, eBook Kindle

黑洞 - 維基百科，自由的百科全書 -  · Black holes : the membrane paradigm. New Haven. ISBN 0-300-03769-4. OCLC 13759977. ^ Preskill, J. Black holes and information: A crisis in quantum physics (PDF). Caltech Theory Seminar. 21 October 1994 [2020-02-01]. （原始內容 (PDF) 存檔於2008-05-18）. ^ Hawking & Ellis 1973，Appendix B

Black hole - Wikipedia - 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

블랙홀 - 위키백과, 우리 모두의 백과사전 - 블랙홀(영어: Black hole) 은 항성이 진화의 최종단계에서 폭발후 수축되어 생성된 것으로 추측되는, 강력한 밀도와 중력으로 입자나 전자기 복사, 빛을 포함한 그 무엇도 빠져나올 수 없는 시공간 영역이다. 일반 상대성이론은 충분히 밀집된 질량이 시공을 뒤틀어 블랙홀을 형성할 수 있음을 예측한다

黑洞 - 维基百科，自由的百科全书 - 黑洞（英語： black hole ）是時空展現出極端強大的引力，以致於所有粒子、甚至光这样的電磁輻射都不能逃逸的區域 。廣義相對論預測，足夠緊密的質量可以扭曲時空，形成黑洞 ；不可能從該區域逃離的邊界稱為事件視界（英語： event horizon ）。雖然，事件視界對穿越它的物體的命運和情況有巨大

Mechanistic Insights into Gasdermin Pore Formation and -  · Subsequent studies further showed that GSDMD-NTD can oligomerize and form pores with an inner diameter of 12–20 nm on the membrane.22, 25, 59, 60, 61 Extensive GSDMD pore formation on the plasma membrane triggers rapid pyroptotic cell death by disrupting osmotic pressure.62, 63 In vitro lipid-binding assays demonstrated that GSDMD-NTD selectively binds acidic phospholipids such as

List of black holes - Wikipedia - This list of black holes (and stars considered probable candidates) is organized by mass (including black holes of undetermined mass); some items in this list are galaxies or star clusters that are believed to be organized around a black hole. Messier and New General Catalogue designations are …

Singularities and Black Holes (Stanford Encyclopedia of -  · Black holes, however, raise several additional conceptual problems and questions on their own. When quantum effects are taken into account, black holes, although they are nothing more than regions of spacetime, appear to become thermodynamical entities, with a temperature and an entropy. This seems to point to a deep and hitherto unsuspected connection among our three most …

Kara delik - Vikipedi - Kara delik, astrofizikte, çekim alanı her türlü maddesel oluşumun ve ışınımın kendisinden kaçmasına izin vermeyecek derecede güçlü olan, kütlesi büyük bir kozmik cisimdir. Kara delik, uzayda belirli nicelikteki maddenin bir noktaya toplanması ile meydana gelen bir nesnedir de denilebilir. Bu tür nesneler ışık yaymadıklarından kara olarak nitelenirler

Buco nero - Wikipedia - In astrofisica un buco nero è un corpo celeste con un campo gravitazionale così intenso da non lasciare sfuggire né la materia, né la radiazione elettromagnetica, ovvero, da un punto di vista relativistico, una regione dello spaziotempo con una curvatura talmente grande che nulla dal suo interno può uscirne, nemmeno la luce essendo la velocità di fuga superiore a c

Buraco negro – Wikipédia, a enciclopédia livre - Buraco negro é uma região do espaço-tempo em que o campo gravitacional é tão intenso que nada — nenhuma partícula ou radiação eletromagnética como a luz — pode escapar dela. [6] A teoria da relatividade geral prevê que uma massa suficientemente compacta pode deformar o espaço-tempo para formar um buraco negro. [7] [8] O limite da região da qual não é possível escapar é

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