Fierz Pauli masive gravity theory: graviton can it have mass? 1939.
van Dam, Veltman Zhakharov 1970 massless limit is ne GR. so problem.
But then nonlinearities cause the limit to be eq to GR (Vainshtein 1972)
Boulware Deser ghosts in non-linear theory?! 1972, so not viable..
But de Rham, Gabadadze and Tolley 2010 solved this issue.
But no FLRW in this cosmology (2011)???
Gumrukcuoglu, Lin Mukhoyama 2011a, 1206.2273
No predictions yet for how to distinguish between massive gravity and GR and on what scales we should be searching. A general prediction is that there should be statistical anisotropy...
Brian Schmidt:
Oguri:
Ask about flux anamolies: Radio loud quasars are rarer...
Selection function
Gravitational lenses using quasar galaxy cross correlations?
Surface photometry to study Sandage & Tammann's criticism.
Fukugita & Hogan, 1990
Lahav, Lilje, Primack & Hogan 1991
Number counts of galaxies
Alcock paczynski test
Strong lensing statistics: Fukugita et al.
Number count of faint galaxies: Fukugita Takahara Yamashita and Yoshii 1990
Fukugita, Futamase and Kasai 1990 Strong lensing Oguri et al. 2012
Efstathiou et al. 1990 Large scale power in w(theta) and evolution
Fukugita, Hogan and Peebles 1993?! Nature
Scaling of the light curves of SNeIa:
1984; SneIa Pskovskii
1993 Phillips
1996: Riess, Press and Kirshner
1992: Announcement of CMB inhomgenities DT/T ~ 5 E-6...
1996: 250 Anniversary Princeton: All observations are consistent with Lambda ne 0
Perlmutter et al. 1997 ( Lambda ~ 0.06 \pm 0.03
Schmidt 1998 Lambda ~ 0.6 \pm 0.5
Riess et al. 1998 \Lambda ~ 7-9 sigma
Perlmutter et al. 1999 (lambda ~ 0.72 \pm 0.09)
MF + Yanagida 1995
Mukhoyama: Nonlinear massive gravity.
Fierz Pauli masive gravity theory: graviton can it have mass? 1939.
van Dam, Veltman Zhakharov 1970 massless limit is ne GR. so problem.
But then nonlinearities cause the limit to be eq to GR (Vainshtein 1972)
Boulware Deser ghosts in non-linear theory?! 1972, so not viable..
But de Rham, Gabadadze and Tolley 2010 solved this issue.
But no FLRW in this cosmology (2011)???
Gumrukcuoglu, Lin Mukhoyama 2011a, 1206.2273
No predictions yet for how to distinguish between massive gravity and GR and on what scales we should be searching. A general prediction is that there should be statistical anisotropy...
Brian Schmidt:
Oguri:
Ask about flux anamolies: Radio loud quasars are rarer...
Selection function
Gravitational lenses using quasar galaxy cross correlations?