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University of Birmingham > Talks@bham > Astrophysics Talks Series > Testing Modified Gravity at the Saddle Point with LISA Pathfinder
![]() Testing Modified Gravity at the Saddle Point with LISA PathfinderAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Ilya Mandel. It has now been known for around 80 years that the observed galactic rotation curves cannot be explained assuming just the visible mass and our standard theory of gravitation. Despite concentrated efforts, the direct search for Dark Matter remains largely fruitless, and various proposals to modify the laws of gravitation have been put forward over the last decades. The difficulty with these proposals is that almost by definition, significant deviations from standard gravitation are predicted only in extreme environments outside the Solar System, seemingly beyond the reach of direct experimentation. However, some of the proposed models predict potentially measureable effects around gravitational saddle points inside the Solar System. It has been pointed out that LISA Pathfinder could in principle be re-directed to the Sun-Earth Saddle Point, following its nominal mission. The sensitivity of the gravity gradiometer on board appears sufficient to subject some of the theoretical models to quite a stringent, controlled experimental test. This talk discusses the progress that has been made on establishing the feasibility and significance of such a direct test. This talk is part of the Astrophysics Talks Series series. This talk is included in these lists:Note that ex-directory lists are not shown. |
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