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The local dark sector. Probing gravitation's low-acceleration frontier and dark matter in the Solar System neighborhood

Bergé, Joel and Baudis, Laura and Brax, Philippe and Chiow, Sheng-Wey and Christophe, Bruno and Doré, Olivier and Fayet, Pierre and Hees, Aurelien and Jetzer, Philippe and Lämmerzahl, Claus and List, Meike and Métris, Gilles and Pernot-Borràs, Martin and Read, Justin and Reynaud, Serge and Rhodes, Jason and Rievers, Benny and Rodrigues, Manuel and Sumner, Timothy and Uzan, Jean-Philippe and Yu, Nan (2019) The local dark sector. Probing gravitation's low-acceleration frontier and dark matter in the Solar System neighborhood. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20190925-083539849

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Abstract

We speculate on the development and availability of new innovative propulsion techniques in the 2040s, that will allow us to fly a spacecraft outside the Solar System (at 150 AU and more) in a reasonable amount of time, in order to directly probe our (gravitational) Solar System neighborhood and answer pressing questions regarding the dark sector (dark energy and dark matter). We identify two closely related main science goals, as well as secondary objectives that could be fulfilled by a mission dedicated to probing the local dark sector: (i) begin the exploration of gravitation's low-acceleration regime with a man-made spacecraft and (ii) improve our knowledge of the local dark matter and baryon densities. Those questions can be answered by directly measuring the gravitational potential with an atomic clock on-board a spacecraft on an outbound Solar System orbit, and by comparing the spacecraft's trajectory with that predicted by General Relativity through the combination of ranging data and the in-situ measurement (and correction) of non-gravitational accelerations with an on-board accelerometer. Despite a wealth of new experiments getting online in the near future, that will bring new knowledge about the dark sector, it is very unlikely that those science questions will be closed in the next two decades. More importantly, it is likely that it will be even more urgent than currently to answer them. Tracking a spacecraft carrying a clock and an accelerometer as it leaves the Solar System may well be the easiest and fastest way to directly probe our dark environment.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1909.00834arXivDiscussion Paper
ORCID:
AuthorORCID
Doré, Olivier0000-0002-5009-7563
Hees, Aurelien0000-0002-2186-644X
Rhodes, Jason0000-0002-4485-8549
Record Number:CaltechAUTHORS:20190925-083539849
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190925-083539849
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98839
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Sep 2019 17:48
Last Modified:03 Oct 2019 21:44

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