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Constraining chameleon models with cosmology
Open accessAbstract
Chameleon fields may modify gravity on cluster scales while recovering general relativity locally. This article reviews signatures of chameleon modifications in the nonlinear cosmological structure, comparing different techniques to model them, summarising the current state of observational constraints, and concluding with an outlook on prospective constraints from future observations and applications of the analytic tools developed in the process to more general scalar‐tensor theories. Particular focus is given to the Hu‐Sawicki and designer models of gravity.
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Lombriser et al. (2014) and Lombriser (2014) combined the spherical collapse model, halo model, linear perturbation theory, quasi-nonlinear interpolation and one-loop perturbations to derive a description of the nonlinear matter power spectrum of f(R) gravity with chameleon screening up to k=0.1 h/Mpc.
“Lombriser et al. (2014) and Lombriser (2014) combined the spherical collapse model, the halo model, linear perturbation theory, quasi-nonlinear interpolation motivated by the above and one-loop perturbations in order to derive a description of nonlinear the nonlinear matter power spectrum of f(R) gravity with chameleon screening on scales of up to h/Mpc.”
From Testing general relativity in cosmology (2019) · cites this paper as Lombriser (2014)
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References 161 · Cited by 104
Research works printed but not linked: 163
- 10.12942/lrr-2006-3 · DOI · Paper page
- 10.1103/PhysRevLett.93.171104 · DOI · Paper page
- Khoury J., 2004, Phys. Rev., 69, 044026
- Brax P., 2004, Phys. Rev., 70, 123518
- Cembranos J., 2006, Phys. Rev., 73, 064029
- Mota D. F., 2007, Phys. Rev., 75, 063501
- 10.1103/PhysRevLett.109.241301 · DOI · Paper page
- Hu W., 2007, Phys. Rev., 76, 064004
- Song Y. S., 2007, Phys. Rev., 75, 044004
- 10.1093/mnras/150.1.1 · DOI
- Starobinsky A. A., 1979, JETP Lett., 30, 682
- Capozziello S., 2003, Recent Res. Dev. Astron. Astrophys., 1, 625
- Carroll S. M., 2004, Phys. Rev., 70, 043528
- Nojiri S., 2003, Phys. Rev., 68, 123512
- 10.1016/j.physletb.2003.09.033 · DOI
- Zhang P., 2006, Phys. Rev., 73, 123504
- 10.1103/PhysRevLett.98.131302 · DOI
- 10.1142/S0218271807010936 · DOI
- Amendola L., 2007, Phys. Rev., 75, 083504
- Li B., 2007, Phys. Rev., 75, 084010
- 10.1103/PhysRevLett.99.141302 · DOI
- Song Y. S., 2007, Phys. Rev., 76, 063517
- Jain B., 2008, Phys. Rev., 78, 063503
- Brax P., 2008, Phys. Rev., 78, 104021
- Zhao G. B., 2009, Phys. Rev., 79, 083513
- Hui L., 2009, Phys. Rev., 80, 104002
- Schmidt F., 2009, Phys. Rev., 80, 083505
- 10.1088/1475-7516/2010/04/030 · DOI · Paper page
- 10.1038/nature08857 · DOI · Paper page
- Lombriser L., 2012, Phys. Rev., 85, 124038
- Yamamoto K., 2010, Phys. Rev., 81, 103517
- 10.1016/j.aop.2010.04.002 · DOI
- 10.1143/PTP.124.541 · DOI
- 10.1016/j.physletb.2011.07.022 · DOI
- 10.1088/0004-637X/747/1/48 · DOI
- Ferraro S., 2011, Phys. Rev., 83, 063503
- 10.1088/1475-7516/2011/03/036 · DOI
- Davis A. C., 2012, Phys. Rev., 85, 123006
- 10.1088/1475-7516/2011/10/032 · DOI
- 10.1088/1475-7516/2011/08/005 · DOI
- Zhao G. B., 2012, Phys. Rev., 85, 123546
- 10.1088/1475-7516/2011/11/019 · DOI
- 10.1038/nature10445 · DOI
- Lombriser L., 2012, Phys. Rev., 85, 102001
- 10.1103/PhysRevLett.109.051301 · DOI
- Terukina A., 2012, Phys. Rev., 86, 103503
- Di Valentino E., 2012, Phys. Rev., 86, 063517
- 10.1088/0004-637X/779/1/39 · DOI · Paper page
- 10.1093/mnras/sts443 · DOI
- He J. h., 2012, Phys. Rev., 86, 103505
- Hu B., 2013, Phys. Rev., 88, 024012
- Okada H., 2013, Phys. Rev., 87, 103002, 10.1103/PhysRevA.87.043427 · DOI
- Hall A., 2013, Phys. Rev., 87, 064026
- 10.1093/mnras/sts493 · DOI · Paper page
- 10.1088/1475-7516/2013/07/009 · DOI
- Lombriser L., 2013, Phys. Rev., 87, 104019
- P.Brax A. C.Davis andJ.Sakstein (2013). · DOI
- Marchini A., 2013, Phys. Rev., 87, 083527
- 10.1088/1475-7516/2013/08/020 · DOI
- Abebe A., 2013, Phys. Rev., 88, 044050
- Lam T. Y., 2013, Phys. Rev., 88, 023012
- 10.1093/mnras/stt1430 · DOI
- Marchini A., 2013, Phys. Rev., 88, 027502
- 10.1103/PhysRevD.88.103523 · DOI
- Hu B., 2013, Phys. Rev., 88, 123514
- 10.1088/1475-7516/2014/01/019 · DOI
- Sakstein J., 2013, Phys. Rev., 88, 124013
- Cai Y. C., 2014, Mon. Not. Roy. Astron. Soc.
- M.Baldi F.Villaescusa‐Navarro M.Viel E.Puchwein V.Springelet al. (2013). · DOI
- Christian A., 2013, Mon. Not. R. Astron. Soc., 440, 833
- 10.1088/1475-7516/2014/03/021 · DOI · Paper page
- 10.1088/1475-7516/2014/02/018 · DOI
- W. A.Hellwing A.Barreira C. S.Frenk B.Li andS.Cole (2014). · DOI
- A. C.Davis R.Gregory R.Jha andJ.Muir (2014). · DOI
- D.Munshi B.Hu A.Renzi A.Heavens andP.Coles (2014). · DOI
- 10.1103/PhysRevLett.110.171101 · DOI
- 10.1103/PhysRevLett.109.041301 · DOI
- Oyaizu H., 2008, Phys. Rev., 78, 123523
- Oyaizu H., 2008, Phys. Rev., 78, 123524
- Li B., 2009, Phys. Rev., 80, 044027
- 10.1088/0004-637X/728/2/109 · DOI
- Zhao G. B., 2011, Phys. Rev., 83, 044007
- 10.1088/1475-7516/2012/01/051 · DOI
- 10.1093/mnras/stt1575 · DOI · Paper page
- Hu W., 2007, Phys. Rev., 76, 104043
- Zhao G. B., 2010, Phys. Rev., 81, 103510
- Li Y., 2011, Phys. Rev., 84, 084033
- Schmidt F., 2010, Phys. Rev., 81, 103002
- 10.1088/1475-7516/2011/12/005 · DOI
- Lombriser L., 2012, Phys. Rev., 85, 124054
- Schmidt F., 2009, Phys. Rev., 79, 083518
- Borisov A., 2012, Phys. Rev., 85, 063518, 10.1103/PhysRevB.85.134410 · DOI
- 10.1111/j.1365-2966.2011.20404.x · DOI
- 10.1103/PhysRevD.87.123511 · DOI
- 10.1111/j.1365-2966.2012.21592.x · DOI
- 10.1111/j.1365-2966.2012.21746.x · DOI
- Kopp M., 2013, Phys. Rev., 88, 084015
- Koyama K., 2009, Phys. Rev., 79, 123512
- Brax P., 2013, Phys. Rev., 88, 023527
- 10.1007/BF01807638 · DOI · Paper page
- Deffayet C., 2011, Phys. Rev., 84, 064039
- Nicolis A., 2009, Phys. Rev., 79, 064036
- 10.1103/PhysRevLett.104.231301 · DOI · Paper page
- Upadhye A., 2012, Phys. Rev., 86, 102003
- Pogosian L., 2008, Phys. Rev., 77, 023503
- Nojiri S., 2006, Phys. Rev., 74, 086005
- 10.1088/1742-6596/66/1/012005 · DOI
- 10.1016/j.physrep.2011.04.001 · DOI
- Esposito‐Farese G., 2001, Phys. Rev., 63, 063504
- Tsujikawa S., 2008, Phys. Rev., 77, 103009, 10.1103/PhysRevB.77.054413 · DOI
- Hojjati A., 2012, Phys. Rev., 86, 123503
- 10.1103/PhysRevD.88.043521 · DOI
- Noller J., 2014, Phys. Rev., 89, 023521
- Lombriser L., 2011, Phys. Rev., 83, 063519
- 10.1046/j.1365-8711.2001.04532.x · DOI
- 10.1093/mnras/sts072 · DOI
- Teyssier R., 2002, Astron. Astrophys., 385, 337, 10.1051/0004-6361:20011817 · DOI
- 10.1111/j.1365-2966.2005.09655.x · DOI · Paper page
- 10.1103/PhysRevLett.110.161101 · DOI
- 10.1111/j.1365-2966.2012.21567.x · DOI · Paper page
- 10.1093/mnras/stt1763 · DOI
- 10.1088/1475-7516/2010/08/033 · DOI
- 10.1111/j.1365-2966.2012.20573.x · DOI
- 10.1111/j.1365-2966.2008.13038.x · DOI
- 10.1086/152650 · DOI
- 10.1046/j.1365-8711.1999.02692.x · DOI
- 10.1046/j.1365-8711.2001.04006.x · DOI
- 10.1046/j.1365-8711.2002.04950.x · DOI
- Hui L., 2008, Phys. Rev., 77, 043527
- Martino M. C., 2009, Phys. Rev., 79, 084013
- Parfrey K., 2011, Phys. Rev., 83, 063511
- 10.1086/177173 · DOI · Paper page
- 10.1046/j.1365-8711.2001.04068.x · DOI
- 10.1046/j.1365-8711.2000.03779.x · DOI
- 10.1046/j.1365-8711.2000.03715.x · DOI
- 10.1016/S0370-1573(02)00276-4 · DOI
- 10.1086/305424 · DOI
- 10.1086/306640 · DOI
- 10.1046/j.1365-8711.2003.06503.x · DOI · Paper page
- Valageas P., 2013, Phys. Rev., 87, 083522
- 10.1103/PhysRevLett.110.151104 · DOI
- Bolton A. S., 2006, Phys. Rev., 74, 061501
- 10.1088/0004-637X/763/1/28 · DOI
- 10.1103/PhysRevLett.107.071303 · DOI
- 10.1093/mnras/stt219 · DOI
- 10.1016/j.physletb.2011.11.028 · DOI
- 10.1088/1475-7516/2013/11/056 · DOI
- A.Barreira B.Li W. A.Hellwing L.Lombriser C. M.Baughet al. (2014). · DOI
- 10.1088/1475-7516/2013/10/027 · DOI
- 10.1088/1475-7516/2013/11/012 · DOI
- Schmidt F., 2010, Phys. Rev., 81, 063005
- 10.1016/S0370-2693(00)00669-9 · DOI · Paper page
- Schmidt F., 2009, Phys. Rev., 80, 123003
- Fang W., 2008, Phys. Rev., 78, 103509
- Lombriser L., 2009, Phys. Rev., 80, 063536
- 10.1093/mnras/stt1517 · DOI
- 10.1088/1475-7516/2014/02/048 · DOI
- 10.1088/1475-7516/2012/08/026 · DOI
- Barreira A., 2013, Phys. Rev., 87, 103511
- 10.1088/1475-7516/2013/08/010 · DOI · Paper page
- Baker T., 2013, Phys. Rev., 87, 024015
- C.de Rham (2014). · DOI
- 10.1002/andp.19163540702 · DOI · Paper page
Metadata
- Authors
- Lombriser, L.
- Affiliations
- Royal Observatory (GB)
- Corresponding author
- Lombriser, Lucas
- ORCID
- Lombriser, Lucas
- Venue
- Annalen der Physik
- Publisher
- Wiley
- Published
- 2014-06-16
- Volume
- 526
- Issue
- 7-8
- Pages
- 259-282
- ISSN
- 0003-3804 (ISSN-L)
- 1521-3889
- OpenAlex
- W2949258779
- Cited by
- 104
- References
- 161
- Citations by year
- 2026: 2 · 2025: 2 · 2024: 5 · 2023: 6 · 2022: 4 · 2021: 4 · 2020: 11 · 2019: 14 · 2018: 15 · 2017: 6 · 2016: 18 · 2015: 13 · 2014: 4
- FWCI
- 7.37
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Annalen der Physik (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- arXiv (Cornell University)
- Funders
- University of Edinburgh
- Science and Technology Facilities Council
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- chameleon mechanism, modified gravity, scalar-tensor gravity, Hu-Sawicki model, structure formation, nonlinear structures, observational constraints
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