The DOI matches its Crossref record, with a small difference in title or year; 9 of the 9 references it cites were found in a registry or an index.
Black holes in the Brans-Dicke: Theory of gravitation
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In the citing paper
“There is an obvious analogy with the second law of thermodynamics in the law that, classically, the area of the event horizon can never decrease and that when two black holes collide and merge together, the area of the final event horizon is greater than the sum of the areas of the two original horizons [7, 12].”
From Particle creation by black holes (1975) · cites this paper as [7]
In the citing paper
“As the mass of the black hole decreased, the area of the event horizon would have to go down, thus violating the law that, classically, the area cannot decrease [7, 12].”
From Particle creation by black holes (1975) · cites this paper as [7]
In the citing paper
“It is now generally believed that, according to classical theory, a gravitational collapse will produce a black hole which will settle down rapidly to a stationary axisymmetric equilibrium state characterized by its mass, angular momentum and electric charge [7, 13].”
From Particle creation by black holes (1975) · cites this paper as [7]
In the citing paper
“From the classical singularity theorems [3-6], one would expect such high curvatures to occur in collapsing stars and, in the past, at the beginning of the present espe se e oone o on oet e ne o e e osones of high curvature to be hidden from us by an event horizon [7].”
From Particle creation by black holes (1975) · cites this paper as [7]
In the citing paper
“The decrease in area of the event horizon is caused by a violation of the weak energy condition [5–7, 12] which arises from the indeterminacy of particle number and energy density in a curved space-time.”
From Particle creation by black holes (1975) · cites this paper as [7]
In the citing paper
“A wave packet of a classical Boson field will obey the weak energy condition: the local energy density for any observer is non-negative. It follows from this [7, 12] that the change in area dA induced by the wave-packet will be non-negative.”
From Particle creation by black holes (1975) · cites this paper as [7]
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Metadata
- Authors
- Hawking, S. W.
- Affiliations
- University of Cambridge (GB)
- Corresponding author
- Hawking, S. W.
- ORCID
- Hawking, S. W.
- Venue
- Communications in Mathematical Physics
- Published
- 1972-06
- Volume
- 25
- Issue
- 2
- Pages
- 167-171
- ISSN
- 0010-3616 (ISSN-L)
- 1432-0916
- OpenAlex
- W2044258715
- Cited by
- 433
- References
- 9
- Citations by year
- 2026: 13 · 2025: 25 · 2024: 26 · 2023: 21 · 2022: 21 · 2021: 25 · 2020: 30 · 2019: 32 · 2018: 43 · 2017: 14 · 2016: 24 · 2015: 17 · 2014: 19 · 2013: 13 · 2012: 4
- FWCI
- 2.68
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Communications in Mathematical Physics (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Keywords
- Brans-Dicke theory, black holes, Einstein field equations, scalar-tensor gravity, black hole collisions, stellar collapse
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