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Physical Review Letters|October 10, 2006
No-go theorem for k-essence dark energyCamille Bonvin, Chiara Caprini, Ruth DurrerPhysical Review Letters|June 29, 2006
Dipole of the luminosity distance: a direct measure of H(z)Camille Bonvin, Ruth Durrer, Martin KunzPhysical Review Letters|June 1, 2014
Can primordial magnetic fields be the origin of the BICEP2 data?Camille Bonvin, Ruth Durrer, Roy MaartensPhilosophical Transactions. Series A, Mathematical, Physical, and Engineering Sciences|November 16, 2011
What do we really know about dark energy?Ruth DurrerGeneral Relativity and Gravitation|August 23, 2022
Testing general relativity with cosmological large scale structureRuth DurrerPhysical Review Letters|October 13, 2007
Dynamical casimir effect in braneworldsRuth Durrer, Marcus RuserPhysical Review Letters|December 6, 2024
Testing General Relativity through the E_{G} Statistic Using the Weyl Potential and Galaxy VelocitiesNastassia Grimm, Camille Bonvin, Isaac TutusausNature Communications|November 3, 2025
Comparing the motion of dark matter and standard model particles on cosmological scalesNastassia Grimm, Camille Bonvin, Isaac TutusausNature Communications|November 11, 2024
Measurement of the Weyl potential evolution from the first three years of dark energy survey dataIsaac Tutusaus, Camille Bonvin, Nastassia GrimmPhysical Review Letters|February 21, 2015
Does small scale structure significantly affect cosmological dynamics?Julian Adamek, Chris Clarkson, Ruth Durrer, et al.Pageof 2