Cited by 154Relativity and Gravitational TheoryCosmology and Gravitation TheoriesPulsars and Gravitational Waves Research

Gravitation

Misner, C. W., Thorne, K. S., Wheeler, J. A., Chandrasekhar, S.·1974·Physics Today

Abstract

Share Icon Share Twitter Facebook Reddit LinkedIn Reprints and Permissions Cite Icon Cite Search Site Citation C. W. Misner, K. S. Thorne, J. A. Wheeler, S. Chandrasekhar; Gravitation. Physics Today 1 August 1974; 27 (8): 47–48. https://doi.org/10.1063/1.3128805 Download citation file: Ris (Zotero) Reference Manager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentPhysics Today Search Advanced Search

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Crossref · 10.1063/1.3128805

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  • According to the general theory of relativity, a precise clock located at a position with higher geopotential runs quicker than a precise clock located at a position with lower geopotential.

    “According to the GRT, a precise (atomic) clock located at the position P with higher geopotential runs quicker than a precise clock located at the position Q with lower geopotential [12,44,45].”
  • The energy-momentum tensor of the form with a time-like unit vector, energy density, and pressure tensor is classified as Hawking-Ellis type I and covers standard non-null classical matters in 3+1 dimensions.

    “This EMT is classified as the Hawking-Ellis type I[19], and it covers standard (non-null) classical matters in 3 + 1 dimensions[30].”

    From Is energy conserved in general relativity? (2025) · cites this paper as [19]

  • When the spatial separation of two clocks is much smaller than the typical length of background curvature of space-time, curvature effects can safely be neglected, as a consequence of the Einstein equivalence principle.

    “When the spatial separation of two clocks is much smaller than the typical length of background curvature of space-time, then curvature effects can safely be neglected. This is a consequence of the Einstein equivalence principle (see e.g. [14]).”

    From Chronometric Geodesy: Methods and Applications (2019) · cites this paper as [14]

  • Local energy is not well-defined in general relativity, and global definitions of mass require the space-time to possess an infinity.

    “Local energy is not well-defined in general relativity, and for global definitions of mass the space-time must possess an infinity [19,20].”

    From A covariant entropy conjecture (1999) · cites this paper as [20]

  • The mass inside the apparent horizon is exactly a quarter of the area of the apparent horizon.

    “This is exactly a quarter of the area of the apparent horizon.”

    From A covariant entropy conjecture (1999) · cites this paper as [20]

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Cited by 154

Authors
Misner, C. W., Thorne, K. S., Wheeler, J. A., & Chandrasekhar, S.
Affiliations
University of Chicago (US)
Venue
Physics Today
Published
1974-08-01
Volume
27
Issue
8
Pages
47-48
ISSN
  • 0031-9228 (ISSN-L)
  • 1945-0699
OpenAlex
W4253222338
Cited by
154
References
0
Citations by year
2026: 6 · 2025: 1 · 2024: 1 · 2023: 1 · 2022: 3 · 2021: 2 · 2020: 1 · 2018: 1 · 2016: 1 · 2015: 4 · 2014: 10 · 2013: 17 · 2012: 7
Type
book review
Language
en
Open access
closed
Locations
Physics Today (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
Keywords
gravity, general relativity

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