Cited by 22

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

The supersymmetric Casimir effect and quantum creation of the universe with nontrivial topology (II)

Goncharov, Yu.P., Bytsenko, A.A.·1986·Physics Letters B

Overview

Integrity signals

Registry

Crossref · 10.1016/0370-2693(86)90644-1

Cites

2 of 2 references verified0 citation errors · 0 not checkable

Statistics

Recomputing p-values needs the paper’s full text.

Verification

Claims the paper makes

We couldn’t retrieve this paper’s full text, so its claims and self-check weren’t run. The registry and citation checks still apply.

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • If the initial size of the universe was O(1), then at t >> 1 each particle within one cosmological time would run all over the torus many times, appearing in all parts with nearly equal probability; this chaotic mixing leads to rapid homogenization.

    “If the initial size of the universe was O(1), then at the time t ≫ 1 each particle (or a gravitational perturbation of metric) within one cosmological time would run all over the torus many times, appearing in all of its parts with nearly equal probability.This effect, called “chaotic mixing,” should lead to a rapid homogenization of the universe [5,6].”
  • Chaotic mixing can be very efficient in a compact hyperbolic universe.

    “Chaotic mixing can be very efficient in a compact hyperbolic universe (i.e. in a compactified version of an open universe) [5,6].”
  • With a specific fine-tuning of inflationary potential [12], the inflationary stage can be made sufficiently short, in which case remnants of the original anisotropy of the universe may become observable [6].

    “However, with a specific fine-tuning of inflationary potential [12], the inflationary stage can be made sufficiently short, in which case the remnants of the original anisotropy of the universe may become observable [6].”

Citations

Cites

Flagged first, then by citations

Research works printed but not linked: 33

  1. Goncharov, 1985, Phys. Lett., 160B, 385, 10.1016/0370-2693(85)90006-1 · DOI · Paper page
  2. Nilles, 1984, Phys. Rep., 110, 1, 10.1016/0370-1573(84)90008-5 · DOI
  3. Cremmer, 1978, Phys. Lett., 79B, 231, 10.1016/0370-2693(78)90230-7 · DOI
  4. 1979, Nucl. Phys., B147, 105
  5. Ellis, 1983, Nucl. Phys., B224, 427, 10.1016/0550-3213(83)90384-X · DOI
  6. Fayet, 1984, Phys. Lett., 142B, 263, 10.1016/0370-2693(84)91195-X · DOI
  7. Fayet, 1985, Phys. Lett., 153B, 397, 10.1016/0370-2693(85)90480-0 · DOI
  8. 1984, Nucl. Phys., B246, 89
  9. Enqvist, 1985, Phys. Lett., 157B, 43, 10.1016/0370-2693(85)91208-0 · DOI
  10. De Aguila, 1985, Nucl. Phys., B250, 225, 10.1016/0550-3213(85)90480-8 · DOI
  11. Ellis, 1984, Nucl. Phys., B241, 406, 10.1016/0550-3213(84)90054-3 · DOI
  12. Ellis, 1984, Nucl. Phys., B247, 373, 10.1016/0550-3213(84)90555-8 · DOI
  13. Starobinsky, 1980, Phys. Lett., 91B, 99, 10.1016/0370-2693(80)90670-X · DOI · Paper page
  14. Dowker, 1978, J. Phys., A11, 2255
  15. Dowker, 1979, J. Phys., A12, 2545
  16. De Witt, 1979, Physica, 96A, 197, 10.1016/0378-4371(79)90207-3 · DOI
  17. Bagger, 1983, Nucl. Phys., B222, 1, 10.1016/0550-3213(83)90605-3 · DOI
  18. van Nieuwenhuizen, 1981, Phys. Rep., 68, 189, 10.1016/0370-1573(81)90157-5 · DOI
  19. Chokalingham, 1980, J. Phys., A13, 2723
  20. Goncharov, 1982, Phys. Lett., 91A, 153, 10.1016/0375-9601(82)90820-9 · DOI
  21. Goncharov, 1982, Phys. Lett., 119B, 403, 10.1016/0370-2693(82)90700-6 · DOI
  22. Goncharov, 1983, Phys. Lett., 133B, 433, 10.1016/0370-2693(83)90822-5 · DOI
  23. Goncharov, 1984, Phys. Lett., 147B, 269, 10.1016/0370-2693(84)90114-X · DOI
  24. Goncharov, 1985, Phys. Lett., 163B, 155, 10.1016/0370-2693(85)90211-4 · DOI
  25. Goncharov, 1985, Class. Quantum Grav., 2, 179, 10.1088/0264-9381/2/2/011 · DOI
  26. Goncharov, 1985, Phys. Lett., 165B, 49, 10.1016/0370-2693(85)90688-4 · DOI
  27. Unwin, 1980, J. Phys., A13, 313
  28. Zucker, 1975, J. Phys., A8, 1734
  29. Ferrara, 1976, Phys. Rev. Lett., 37, 1669, 10.1103/PhysRevLett.37.1669 · DOI
  30. Ferrara, 1977, Phys. Lett., 66B, 35, 10.1016/0370-2693(77)90607-4 · DOI
  31. Das, 1977, Phys. Rev., D15, 2805
  32. Cremmer, 1977, Nucl. Phys., B127, 259, 10.1016/0550-3213(77)90214-0 · DOI
  33. Gates, 1984, Nucl. Phys., B238, 99, 10.1016/0550-3213(84)90468-1 · DOI

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Metadata

Authors
Goncharov, Y. P., & Bytsenko, A. A.
Venue
Physics Letters B
Publisher
Elsevier BV
Published
1986-03
Volume
169
Issue
2-3
Pages
171-176
ISSN
0370-2693
Cited by
22
References
2
Language
en

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

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