Gaură neagră (Romanian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Gaură neagră" in Romanian language version.

refsWebsite
Global rank Romanian rank
2nd place
3rd place
18th place
27th place
1st place
1st place
69th place
132nd place
4th place
4th place
3rd place
6th place
75th place
56th place
1,553rd place
1,008th place
8,860th place
4,229th place
low place
low place
857th place
479th place
234th place
260th place
low place
9,940th place
670th place
1,710th place
low place
low place
5th place
11th place
3,410th place
2,799th place
310th place
1,271st place
7th place
25th place
887th place
815th place
179th place
36th place
344th place
184th place
8,316th place
5,256th place
low place
low place
1,959th place
2,088th place
3,538th place
3,279th place
3,034th place
2,281st place
low place
low place

arxiv.org

books.google.com

boston.com

archive.boston.com

caltech.edu

theory.caltech.edu

cam.ac.uk

ast.cam.ac.uk

damtp.cam.ac.uk

cern.ch

cds.cern.ch

doi.org

doi.org

dx.doi.org

  • Particle emission rates from a black hole: Massless particles from an uncharged, nonrotating hole, Don N. Page, Physical Review D 13 (1976), pp. 198–206. doi:10.1103/PhysRevD.13.198. See in particular equation (27).

einstein-online.info

eso.org

eurekalert.org

harvard.edu

adsabs.harvard.edu

cfa.harvard.edu

hawking.org.uk

imamu.edu.sa

ligo.org

ligo.org

  • „Detection of gravitational waves”. LIGO. Accesat în . 

dcc.ligo.org

nasa.gov

imagine.gsfc.nasa.gov

nasa.gov

science.nasa.gov

jpl.nasa.gov

nationalgeographic.com

news.nationalgeographic.com

nature.com

nih.gov

ncbi.nlm.nih.gov

nytimes.com

sciencemag.org

sciencenews.org

  • Siegfried, Tom (). „50 years later, it's hard to say who named black holes” (în engleză). Science News. Arhivat din originalul de la . Accesat în . It seems that the “black hole” label was also bandied about in January 1964 in Cleveland at a meeting of the American Association for the Advancement of Science. Science News Letter reporter Ann Ewing reported from that meeting, describing how an intense gravitational field could cause a star to collapse in on itself. “Such a star then forms a ‘black hole’ in the universe,” Ewing wrote 

skyandtelescope.com

spacetelescope.org

stanford.edu

plato.stanford.edu

ucr.edu

math.ucr.edu

web.archive.org

wikipedia.org

en.wikipedia.org

  • Kip Thorne comments on this quote on pp. 134–135 Arhivat în , la Wayback Machine. of his book Black Holes and Time Warps, writing that "The first conclusion was the Newtonian version of light not escaping; the second was a semi-accurate, relativistic description; and the third was typical Eddingtonian hyperbole ... when a star is as small as the critical circumference, the curvature is strong but not infinite, and space is definitely not wrapped around the star. Eddington may have known this, but his description made a good story, and it captured in a whimsical way the spirit of Schwarzschild's spacetime curvature."

worldcat.org