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Quantum effects near a point mass in (2 + 1)-dimensional gravity

Souradeep, Tarun, Sahni, Varun·1992·Physical Review D
DOI 10.1103/physrevd.46.1616
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Crossref · 10.1103/physrevd.46.1616

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  • δg_tt > 0, indicating gravitational attraction.

    “Notably, δg tt > 0, indicating gravitational attraction [32,33].”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [32]

  • A conformally coupled scalar field in Schwarzschild-(A)dS3 produces a Casimir effect with negative energy density such that, upon solving the semi-classical Einstein equations, the linear order change to the tt-component of the metric in static patch coordinates goes like δg_tt = 2L_P F(M)/r.

    “For example, a conformally coupled scalar field in Schwarzschild-(A)dS 3 produces a Casimir effect with negative energy density such that, upon solving the semi-classical Einstein equations (1.1), the linear order change to the tt-component of the metric in static patch coordinates goes like [32,33] δg tt = 2L P F (M ) r , (1.3)”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [32]

  • Quantum backreaction effects alter the geometry such that the black hole horizon appears to hide the conical singularity.

    “Again, quantum backreaction effects alter the geometry such that the black hole horizon appears to hide the conical singularity [32].”

    From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [32]

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Research works printed but not linked: 51

  1. D. Kramer, 1980, Exact Solutions of Einstein's Field Equations
  2. S. Deser, 1990, Fields, Strings and Gravity
  3. S. Deser, 1982, Ann. Phys. (N.Y.), 140, 372, 10.1016/0003-4916(82)90164-6 · DOI
  4. M. E. Ortiz, 1991, Nucl. Phys., B363, 185, 10.1016/0550-3213(91)90240-X · DOI
  5. N. J. Cornish, 1991, Phys. Rev. D, 43, 2555, 10.1103/PhysRevD.43.2555 · DOI · Paper page
  6. A. Vilenkin, 1985, Phys. Rep., 121, 263, 10.1016/0370-1573(85)90033-X · DOI
  7. G. 't Hooft, 1988, Commun. Math. Phys., 117, 685, 10.1007/BF01218392 · DOI
  8. S. Deser, 1988, Commun. Math. Phys., 118, 495, 10.1007/BF01466729 · DOI
  9. A. Cappelli, 1992, Nucl. Phys., B369, 669, 10.1016/0550-3213(92)90282-G · DOI
  10. T. M. Helliwell, 1986, Phys. Rev. D, 34, 1918, 10.1103/PhysRevD.34.1918 · DOI
  11. B. Linet, 1986, Phys. Rev. D, 33, 1833, 10.1103/PhysRevD.33.1833 · DOI
  12. B. Linet, 1987, Phys. Rev. D, 35, 536, 10.1103/PhysRevD.35.536 · DOI
  13. A. G. Smith, 1990, The Formation and Evolution of Cosmic Strings
  14. J. S. Dowker, 1977, J. Phys. A, 10, 115, 10.1088/0305-4470/10/1/023 · DOI
  15. J. S. Dowker, 1987, Class. Quantum Grav., 4, L157, 10.1088/0264-9381/4/5/001 · DOI
  16. J. S. Dowker, 1987, Phys Rev. D, 36, 3095, 10.1103/PhysRevD.36.3095 · DOI
  17. J. S. Dowker, 1990, The Formation and Evolution of Cosmic Strings
  18. P. C. W. Davies, 1987, Class. Quantum Grav., 5, 1, 10.1088/0264-9381/5/1/009 · DOI
  19. V. P. Frolov, 1986, Phys. Rev. D, 34, 2840, 10.1103/PhysRevB.34.2840 · DOI
  20. L. Parker, 1987, Phys. Rev. Lett., 59, 1369, 10.1103/PhysRevLett.59.1369 · DOI
  21. V. Sahni, 1988, Mod. Phys. Lett. A, 3, 1425, 10.1142/S0217732388001719 · DOI
  22. W. A. Hiscock, 1987, Phys. Lett. B, 188, 317, 10.1016/0370-2693(87)91388-8 · DOI
  23. I. H. Russell, 1989, Class. Quantum Grav., 6, 1343, 10.1088/0264-9381/6/10/005 · DOI
  24. A. Sarmiento, 1988, Phys. Rev. D, 38, 1331, 10.1103/PhysRevD.38.1331 · DOI
  25. I. S. Gradshteyn, 1980, Tables of Integrals, Series and Products
  26. B. S. DeWitt, 1975, Phys. Rep., 19C, 295, 10.1016/0370-1573(75)90051-4 · DOI
  27. S. M. Christensen, 1976, Phys. Rev. D, 14, 2490, 10.1103/PhysRevD.14.2490 · DOI
  28. L. D. Landau, 1975, The Classical Theory of Fields
  29. J. D. Barrow, 1986, Class. Quantum Grav., 3, 551, 10.1088/0264-9381/3/4/010 · DOI · Paper page
  30. N. J. Cornish, 1991, Phys. Rev. D, 43, 2555, 10.1103/PhysRevD.43.2555 · DOI · Paper page
  31. 1970, Handbook of Mathematical Functions
  32. T. S. Bunch, 1978, Proc. R. Soc. London, A360, 117, 10.1098/rspa.1978.0060 · DOI
  33. B. Allen, 1987, Phys. Rev. D, 35, 3771, 10.1103/PhysRevD.35.3771 · DOI
  34. W. G. Unruh, 1976, Phys. Rev. D, 14, 870, 10.1103/PhysRevD.14.870 · DOI · Paper page
  35. B. S. DeWitt, 1979, General Relativity
  36. S. Takagi, 1986, Prog. Theor. Phys. Suppl., 88, 1, 10.1143/PTPS.88.1 · DOI
  37. C. J. Isham, 1978, Proc. R. Soc. London, A362, 383, 10.1098/rspa.1978.0140 · DOI
  38. C. J. Isham, 1978, Proc. R. Soc. London, A364, 591, 10.1098/rspa.1978.0219 · DOI
  39. L. H. Ford, 1980, Phys. Rev. D, 21, 949, 10.1103/PhysRevD.21.949 · DOI
  40. T. S. Bunch, 1978, J. Phys. A, 11, 1315, 10.1088/0305-4470/11/7/018 · DOI
  41. N. Sanchez, 1986, Nucl. Phys., B266, 487, 10.1016/0550-3213(86)90102-1 · DOI
  42. C. Teitleboim, 1984, Quantum Theory of Gravity
  43. R. Jackiw, Quantum Theory of Gravity
  44. N. J. Cornish, 1991, Phys. Rev. D, 43, 2555, 10.1103/PhysRevD.43.2555 · DOI · Paper page
  45. J. Gegenberg, 1988, Phys. Rev. D, 37, 3463, 10.1103/PhysRevD.37.3463 · DOI
  46. S. Deser, 1984, Ann. Phys. (N.Y.), 152, 220, 10.1016/0003-4916(84)90085-X · DOI · Paper page
  47. D. Deutch, 1979, Phys. Rev. D, 20, 3063, 10.1103/PhysRevD.20.3063 · DOI
  48. P. Candelas, 1975, Phys. Rev. D, 12, 965, 10.1103/PhysRevD.12.965 · DOI
  49. J. S. Dowker, 1976, Phys. Rev. D, 13, 3224, 10.1103/PhysRevD.13.3224 · DOI
  50. B. Ratra, 1985, Phys. Rev. D, 31, 1931, 10.1103/PhysRevD.31.1931 · DOI
  51. J. Garriga, 1992, Phys. Rev. D, 45, 3469, 10.1103/PhysRevD.45.3469 · DOI

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Metadata

Authors
Souradeep, T., & Sahni, V.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
1992-08-15
Volume
46
Issue
4
Pages
1616-1633
ISSN
0556-2821
DOI
10.1103/physrevd.46.1616
Cited by
68
References
1
Language
en
Licence
link.aps.org/licenses/aps-default-license (vor)

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