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Flux compactification
Open accessAbstract
Recent work is reviewed in which compactifications of string and M theory are constructed in which all scalar fields (moduli) are massive, and supersymmetry is broken with a small positive cosmological constant, features needed to reproduce real world physics. In this work it is explained that there is a ``landscape'' of string/M theory vacua, perhaps containing many candidates for describing real world physics, and arguments are presented for and against this idea. Statistical surveys of the landscape are discussed, as well as the prospects for testable consequences of this picture, such as observable effects of moduli, constraints on early cosmology, and predictions for the scale of supersymmetry breaking.
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String theory supports an enormous landscape of metastable vacua.
“Indeed this view of cosmology is supported by the present understanding of string theory, which argues for the existence of an enormous landscape of such metastable vacua [5,6,7,8].”
From Observable effects of anisotropic bubble nucleation (2010) · cites this paper as [8]
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The cosmological constant problem
Weinberg, S. (1989) · Reviews of Modern Physics · doi:10.1103/revmodphys.61.1 · Cited by 7,341
Hartle, J. B., & Hawking, S. W. (1983) · Physical Review D · doi:10.1103/physrevd.28.2960 · Cited by 3,027
Heterotic and Type I string dynamics from eleven dimensions
Hořava, P., & Witten, E. (1996) · Nuclear Physics B · doi:10.1016/0550-3213(95)00621-4 · Cited by 1,984
Gravitational effects on and of vacuum decay
Coleman, S., & De Luccia, F. (1980) · Physical Review D · doi:10.1103/physrevd.21.3305 · Cited by 1,537
False vacuum inflation with Einstein gravity
Copeland, E. J., Liddle, A. R., Lyth, D. H., Stewart, E. D., & Wands, D. (1994) · Physical Review D · doi:10.1103/physrevd.49.6410 · Cited by 1,077
Birth of inflationary universes
Vilenkin, A. (1983) · Physical Review D · doi:10.1103/physrevd.27.2848 · Cited by 998
Supercooled phase transitions in the very early universe
Hawking, S. W., & Moss, I. L. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)90946-7 · Cited by 816
Further evidence for a variable fine-structure constant from Keck/HIRES QSO absorption spectra
Murphy, M. T., Webb, J. K., & Flambaum, V. V. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06970.x · Cited by 514
Is it possible to create a universe in the laboratory by quantum tunneling?
Farhi, E., Guth, A. H., & Guven, J. (1990) · Nuclear Physics B · doi:10.1016/0550-3213(90)90357-j · Cited by 292
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Research works printed but not linked: 362
- Aazami, A., 2006, J. Cosmol. Astropart. Phys., 013, 10.1088/1475-7516/2006/03/013 · DOI
- Abbott, L. F., 1985, Phys. Lett., 150, 427, 10.1016/0370-2693(85)90459-9 · DOI · Paper page
- Acharya, B. S., 2005, J. High Energy Phys., 056, 10.1088/1126-6708/2005/06/056 · DOI
- 10.1103/PhysRevD.47.426 · DOI
- 10.1016/0550-3213(84)90058-0 · DOI
- 10.1016/0550-3213(85)90408-0 · DOI
- 10.1016/S0370-1573(99)00083-6 · DOI
- Aldazabal, G., 2006, J. High Energy Phys., 070, 10.1088/1126-6708/2006/05/070 · DOI
- Alexander, S. H. S., 2002, Phys. Rev. D, 65, 023507, 10.1103/PhysRevD.65.023507 · DOI
- 10.1103/PhysRevD.70.123505 · DOI · Paper page
- Allanach, B. C., 2005, J. High Energy Phys., 030, 10.1088/1126-6708/2005/05/030 · DOI
- 10.1103/PhysRevB.55.1142 · DOI · Paper page
- 10.1016/0370-2693(86)91524-8 · DOI
- 10.1016/S0550-3213(02)00090-1 · DOI
- Andrianopoli, L., 2002, J. High Energy Phys., 010, 10.1088/1126-6708/2002/07/010 · DOI
- Andrianopoli, L., 2002, Nucl. Phys. B, 640, 46, 10.1016/S0550-3213(02)00563-1 · DOI
- Andrianopoli, L., 2003, J. High Energy Phys., 044, 10.1088/1126-6708/2003/03/044 · DOI
- 10.1016/j.physletb.2003.12.074 · DOI
- Angelantonj, C., 2003, J. High Energy Phys., 015, 10.1088/1126-6708/2003/10/015 · DOI
- 10.1016/0550-3213(87)90372-5 · DOI
- Appelquist, E. T., 1987, Frontiers in Physics
- 10.1103/PhysRevLett.90.221302 · DOI
- Arkani-Hamed, N., 2005, J. High Energy Phys., 073, 10.1088/1126-6708/2005/06/073 · DOI
- 10.1016/S0370-2693(98)00466-3 · DOI · Paper page
- 10.1016/j.nuclphysb.2004.12.026 · DOI
- Ashok, S., 2004, J. High Energy Phys., 060, 10.1088/1126-6708/2004/01/060 · DOI
- Aspinwall, P. S., 2005, J. High Energy Phys., 001, 10.1088/1126-6708/2005/10/001 · DOI
- 10.1016/0550-3213(96)00058-2 · DOI
- Babich, D., 2004, J. Cosmol. Astropart. Phys., 009, 10.1088/1475-7516/2004/08/009 · DOI
- Bachas, E. C., 2002, Unity from Duality: Gravity, Gauge Theory, and Strings
- Balasubramanian, V., 2004, J. High Energy Phys., 085, 10.1088/1126-6708/2004/11/085 · DOI
- Balasubramanian, V., 2005, J. High Energy Phys., 007, 10.1088/1126-6708/2005/03/007 · DOI
- 10.1103/PhysRevLett.52.1461 · DOI
- 10.1016/0550-3213(85)90020-3 · DOI · Paper page
- 10.1103/PhysRevLett.88.131301 · DOI
- Banks, T., 2003, J. Cosmol. Astropart. Phys., 001, 10.1088/1475-7516/2003/06/001 · DOI
- Banks, T., 2004, J. High Energy Phys., 058, 10.1088/1126-6708/2004/08/058 · DOI
- 10.1016/0370-2693(91)90561-4 · DOI
- 10.1016/0550-3213(88)90551-2 · DOI
- 10.1103/PhysRevD.49.779 · DOI
- Barrow, J., 1988, The Anthropic Cosmological Principle
- Beasley, C., 2002, J. High Energy Phys., 46, 10.1088/1126-6708/2002/07/046 · DOI
- 10.1016/0550-3213(96)00367-7 · DOI · Paper page
- Becker, K., 2003, J. High Energy Phys., 007, 10.1088/1126-6708/2003/04/007 · DOI
- 10.1016/S0550-3213(03)00495-4 · DOI
- 10.1016/j.nuclphysb.2006.05.034 · DOI
- 10.1016/j.nuclphysb.2003.11.029 · DOI
- Becker, K., 2002, J. High Energy Phys., 060, 10.1088/1126-6708/2002/06/060 · DOI
- 10.1016/j.nuclphysb.2004.06.019 · DOI
- Behrndt, K., 2005, Phys. Rev. Lett., 95, 021601, 10.1103/PhysRevLett.95.021601 · DOI
- Behrndt, K., 2005, Nucl. Phys. B, 708, 45, 10.1016/j.nuclphysb.2004.12.004 · DOI
- 10.1016/j.nuclphysb.2005.05.020 · DOI
- 10.1016/j.nuclphysb.2006.04.018 · DOI
- 10.1016/j.nuclphysb.2006.05.003 · DOI
- Berg, M., 2005, J. High Energy Phys., 030, 10.1088/1126-6708/2005/11/030 · DOI
- 10.1103/PhysRevLett.96.021601 · DOI
- Berger, M., 1955, Bull. Soc. Math. France, 83, 279, 10.24033/bsmf.1464 · DOI
- 10.1016/0550-3213(95)00367-2 · DOI
- 10.1016/S0550-3213(96)00452-X · DOI
- 10.1103/PhysRevD.34.3069 · DOI
- Blanco-Pillado, J. J., 2004, J. High Energy Phys., 063, 10.1088/1126-6708/2004/11/063 · DOI
- 10.1146/annurev.nucl.55.090704.151541 · DOI
- 10.1016/j.nuclphysb.2005.02.005 · DOI
- 10.1016/S0550-3213(03)00392-4 · DOI
- Bousso, R., 2000, J. High Energy Phys., 006, 10.1088/1126-6708/2000/06/006 · DOI · Paper page
- 10.1103/PhysRevLett.92.181601 · DOI
- Bovy, J., 2005, J. High Energy Phys., 056, 10.1088/1126-6708/2005/08/056 · DOI
- 10.1016/0550-3213(89)90037-0 · DOI
- 10.1016/j.physletb.2006.06.074 · DOI
- 10.1016/0370-2693(87)91190-7 · DOI
- 10.1016/0550-3213(88)90559-7 · DOI
- 10.1103/PhysRevD.68.023517 · DOI
- Burgess, C. P., 2006, J. High Energy Phys., 044, 10.1088/1126-6708/2006/06/044 · DOI
- Burgess, C. P., 2003, J. High Energy Phys., 056
- Burgess, C. P., 2002, J. High Energy Phys., 052, 10.1088/1126-6708/2002/03/052 · DOI
- Burgess, C. P., 2001, J. High Energy Phys., 047, 10.1088/1126-6708/2001/07/047 · DOI
- 10.1016/0370-2693(87)90769-6 · DOI
- 10.1016/0370-2693(88)90602-8 · DOI
- 10.1103/PhysRevD.16.1762 · DOI · Paper page
- Camara, P. G., 2005, J. High Energy Phys., 013, 10.1088/1126-6708/2005/09/013 · DOI
- 10.1016/j.nuclphysb.2004.04.013 · DOI
- 10.1016/j.nuclphysb.2004.11.035 · DOI
- 10.1016/0550-3213(91)90122-E · DOI
- 10.1016/0550-3213(91)90292-6 · DOI
- 10.1016/0550-3213(95)00189-Y · DOI
- 10.1016/0550-3213(85)90602-9 · DOI
- 10.1016/0550-3213(90)90577-Z · DOI
- Carroll, S. M., 2001, Living Rev. Relativ., 4, 1, 10.12942/lrr-2001-1 · DOI · Paper page
- Cascales, J. F. G., 2004, J. High Energy Phys., 031, 10.1088/1126-6708/2004/02/031 · DOI
- Cascales, J. F. G., 2005, J. High Energy Phys., 047, 10.1088/1126-6708/2005/11/047 · DOI
- Cascales, J. F. G., 2003, J. High Energy Phys., 011, 10.1088/1126-6708/2003/05/011 · DOI
- 10.1016/S0550-3213(00)00267-4 · DOI
- Chen, X., 2005, J. High Energy Phys., 045, 10.1088/1126-6708/2005/08/045 · DOI
- Chen, X., 2005, Phys. Rev. D, 71, 063506, 10.1103/PhysRevD.71.063506 · DOI
- 10.1142/S0217751X06029351 · DOI
- 10.1016/j.nuclphysb.2005.04.032 · DOI
- Choi, K., 2004, J. High Energy Phys., 076, 10.1088/1126-6708/2004/11/076 · DOI
- 10.1016/j.physletb.2005.11.078 · DOI
- Choi, K., 2005, J. High Energy Phys., 039, 10.1088/1126-6708/2005/09/039 · DOI
- 10.1103/PhysRevD.15.2929 · DOI · Paper page
- 10.1016/0550-3213(88)90097-1 · DOI · Paper page
- Conlon, J. P., 2004, J. High Energy Phys., 039, 10.1088/1126-6708/2004/10/039 · DOI
- Conlon, J. P., 2006, J. High Energy Phys., 029, 10.1088/1126-6708/2006/06/029 · DOI
- Conlon, J. P., 2005, J. High Energy Phys., 007, 10.1088/1126-6708/2005/08/007 · DOI
- Copeland, E. J., 2004, J. High Energy Phys., 013, 10.1088/1126-6708/2004/06/013 · DOI
- Cremmer, E., 1983, Phys. Lett., 133B, 61, 10.1016/0370-2693(83)90106-5 · DOI · Paper page
- 10.1016/0550-3213(76)90286-8 · DOI
- 10.1016/S0550-3213(01)00533-8 · DOI
- 10.1016/S0550-3213(01)00285-1 · DOI
- 10.1103/PhysRevD.71.106008 · DOI
- 10.1016/j.physletb.2005.01.053 · DOI
- Dabholkar, A., 2003, J. High Energy Phys., 054, 10.1088/1126-6708/2003/09/054 · DOI
- Dabholkar, A., 2006, J. High Energy Phys., 009, 10.1088/1126-6708/2006/05/009 · DOI
- Dall’Agata, G., 2001, J. High Energy Phys., 005, 10.1088/1126-6708/2001/11/005 · DOI
- Dall’Agata, G., 2004, Nucl. Phys. B, 695, 243, 10.1016/j.nuclphysb.2004.06.037 · DOI
- Dall’Agata, G., 2004, Class. Quantum Grav., 21, S1479, 10.1088/0264-9381/21/10/021 · DOI
- 10.1103/PhysRevD.65.126002 · DOI
- Dasgupta, K., 1999, J. High Energy Phys., 023, 10.1088/1126-6708/1999/08/023 · DOI
- D’Auria, R., 2003, J. High Energy Phys., 045, 10.1088/1126-6708/2003/06/045 · DOI
- 10.1016/S0370-2693(03)00191-6 · DOI
- 10.1088/1367-2630/4/1/371 · DOI
- 10.1016/j.physletb.2005.09.027 · DOI
- 10.1016/0370-2693(93)91538-X · DOI
- Denef, F., 2004, J. High Energy Phys., 072, 10.1088/1126-6708/2004/05/072 · DOI
- Denef, F., 2005, J. High Energy Phys., 061, 10.1088/1126-6708/2005/03/061 · DOI
- Denef, F., 2004, J. High Energy Phys., 034, 10.1088/1126-6708/2004/06/034 · DOI
- Derendinger, J. P., 2005, Fortschr. Phys., 53, 926, 10.1002/prop.200410242 · DOI
- Derendinger, J.-P., 2005, Nucl. Phys. B, 715, 211, 10.1016/j.nuclphysb.2005.02.038 · DOI
- 10.1016/0550-3213(87)90267-7 · DOI
- DeWolfe, O., 2005, J. High Energy Phys., 066
- 10.1103/PhysRevD.67.066008 · DOI
- DeWolfe, O., 2005, J. High Energy Phys., 037, 10.1088/1126-6708/2005/02/037 · DOI
- DeWolfe, O., 2005, J. High Energy Phys., 066
- DeWolfe, O., 2004, J. High Energy Phys., 017, 10.1088/1126-6708/2004/05/017 · DOI
- Diaconescu, D.-E., 2006, J. High Energy Phys., 020, 10.1088/1126-6708/2006/02/020 · DOI
- 10.1103/PhysRevD.73.106010 · DOI
- 10.1103/PhysRevD.72.026005 · DOI
- 10.1016/j.nuclphysb.2004.12.032 · DOI
- 10.1016/0550-3213(81)90522-8 · DOI
- 10.1016/0370-2693(96)00390-5 · DOI
- Dine, M., 2005, J. High Energy Phys., 014, 10.1088/1126-6708/2005/07/014 · DOI
- Dine, M., 2006, J. High Energy Phys., 129, 10.1088/1126-6708/2006/01/129 · DOI
- 10.1016/0550-3213(86)90619-X · DOI
- 10.1016/0550-3213(90)90057-K · DOI
- 10.1016/0550-3213(87)90572-4 · DOI
- Donagi, R., 2005, J. High Energy Phys., 070, 10.1088/1126-6708/2005/06/070 · DOI
- 10.1103/PhysRevD.69.106012 · DOI
- 10.1103/PhysRevD.73.113002 · DOI
- Douglas, M. R., 2003, J. High Energy Phys., 046, 10.1088/1126-6708/2003/05/046 · DOI · Paper page
- Douglas, M. R., 2004, C. R. Phys., 5, 965, 10.1016/j.crhy.2004.09.008 · DOI
- 10.1007/s00220-004-1228-y · DOI
- 10.1007/s00220-006-0003-7 · DOI
- Douglas, M. R., 2004, J. High Energy Phys., 014, 10.1088/1126-6708/2004/06/014 · DOI
- 10.1142/S0217751X96002583 · DOI
- Dvali, G., 2004, Phys. Rev. D, 70, 063501, 10.1103/PhysRevD.70.063501 · DOI
- Dvali, G., 2004, J. Cosmol. Astropart. Phys., 010, 10.1088/1475-7516/2004/03/010 · DOI
- 10.1016/S0370-2693(99)00132-X · DOI
- Easther, R., 2005, J. Cosmol. Astropart. Phys., 009
- Easther, R., 2006, J. Cosmol. Astropart. Phys., 018, 10.1088/1475-7516/2006/05/018 · DOI
- Eguchi, T., 2006, J. High Energy Phys., 100, 10.1088/1126-6708/2006/01/100 · DOI
- Ellis, J. R., 1984, Phys. Lett., 134, 429, 10.1016/0370-2693(84)91378-9 · DOI
- 10.1016/S0550-3213(01)00097-9 · DOI
- 10.1016/S0370-2693(02)02626-6 · DOI
- 10.1002/prop.200310153 · DOI
- 10.1007/s00220-004-1221-5 · DOI
- Firouzjahi, H., 2004, J. High Energy Phys., 060, 10.1088/1126-6708/2004/09/060 · DOI
- Fischler, W., 2001, J. High Energy Phys., 003, 10.1088/1126-6708/2001/07/003 · DOI · Paper page
- 10.1016/j.nuclphysb.2004.11.005 · DOI
- Flournoy, A., 2006, J. High Energy Phys., 166, 10.1088/1126-6708/2006/01/166 · DOI
- Font, A., 2005, J. High Energy Phys., 040, 10.1088/1126-6708/2005/03/040 · DOI
- Franco, S., 2005, J. High Energy Phys., 028, 10.1088/1126-6708/2005/09/028 · DOI
- Franco, S., 2006, J. High Energy Phys., 031, 10.1088/1126-6708/2006/06/031 · DOI
- 10.1103/PhysRevD.13.3214 · DOI
- 10.1103/PhysRevLett.65.3233 · DOI
- Freund, P. G. O., 1980, Phys. Lett., 97, 233, 10.1016/0370-2693(80)90590-0 · DOI
- 10.1103/PhysRevD.68.046008 · DOI
- Frey, A. R., 2006, J. High Energy Phys., 021, 10.1088/1126-6708/2006/08/021 · DOI
- 10.1103/PhysRevD.65.126009 · DOI
- Garcia-Bellido, J., 2002, J. High Energy Phys., 036, 10.1088/1126-6708/2002/01/036 · DOI
- Garcia del Moral, M. P., 2006, J. High Energy Phys., 022
- Garcia-Etxebarria, I., 2006, J. High Energy Phys., 069, 10.1088/1126-6708/2006/08/069 · DOI
- 10.1016/0370-2693(87)90938-5 · DOI
- 10.1103/PhysRevD.74.066007 · DOI
- 10.1103/PhysRevD.68.026006 · DOI
- 10.1103/PhysRevD.66.106006 · DOI
- 10.1103/PhysRevD.73.126003 · DOI
- 10.1103/PhysRevD.54.1667 · DOI
- Giryavets, A., 2004, J. High Energy Phys., 002, 10.1088/1126-6708/2004/08/002 · DOI
- Giryavets, A., 2004, J. High Energy Phys., 003, 10.1088/1126-6708/2004/04/003 · DOI
- Giudice, G., 1998, Perspectives on Supersymmetry
- Giudice, G. F., 1998, J. High Energy Phys., 027, 10.1088/1126-6708/1998/12/027 · DOI
- 10.1016/S0370-1573(99)00042-3 · DOI
- 10.1016/j.nuclphysb.2004.08.001 · DOI
- Gmeiner, F., 2006, Fortschr. Phys., 54, 391, 10.1002/prop.200510284 · DOI
- Gmeiner, F., 2006, J. High Energy Phys., 004, 10.1088/1126-6708/2006/01/004 · DOI
- 10.1007/s00220-004-1167-7 · DOI
- Gomez-Reino, M., 2002, J. High Energy Phys., 020, 10.1088/1126-6708/2002/09/020 · DOI
- Gomis, J., 2005, J. High Energy Phys., 021, 10.1088/1126-6708/2005/11/021 · DOI
- Gorlich, L., 2004, J. High Energy Phys., 074
- 10.1016/j.physrep.2005.10.008 · DOI
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Metadata
- Authors
- Douglas, M. R., & Kachru, S.
- Affiliations
- Rutgers, The State University of New Jersey (US)
- ORCID
- Douglas, Michael R.
- Venue
- Reviews of Modern Physics
- Publisher
- American Physical Society (APS)
- Published
- 2007-05-25
- Volume
- 79
- Issue
- 2
- Pages
- 733-796
- ISSN
- 0034-6861 (ISSN-L)
- 1539-0756
- OpenAlex
- W3037032868
- Cited by
- 1,122
- References
- 9
- Citations by year
- 2026: 46 · 2025: 28 · 2024: 30 · 2023: 49 · 2022: 48 · 2021: 41 · 2020: 35 · 2019: 41 · 2018: 37 · 2017: 33 · 2016: 54 · 2015: 61 · 2014: 56 · 2013: 52 · 2012: 54
- FWCI
- 75.79
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Reviews of Modern Physics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- University of North Texas Digital Library (University of North Texas) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation (DE-AC02-76SF00515, 0244728)
- U.S. Department of Energy (DEFG0296ER40959, DE‐FG02‐, 76SF00515, DE–AC02–76SF00515, AC02‐76SF00515, FG02-96ER40959, DE-AC02-)
- California Institute of Technology
- Kavli Institute for Theoretical Physics, University of California, Santa Barbara
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Keywords
- flux compactification, string compactification, M-theory, moduli stabilization, supersymmetry breaking, positive cosmological constant, string landscape, string vacua, early universe cosmology, supersymmetry breaking scale
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