SecondPeriodProjectA1 - TransRegio

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Quintessence, Branes and Higher Dimensions

Principal Investigators: H. P. Nilles, S. Förste (Bonn); C. Wetterich (Heidelberg)

A1 Project Page Bonn

A1 Project Page Heidelberg

A1 Renewal Review Poster


Possible explanations of Dark Energy arise from a space-time in more than four dimensions, characteristic of a theoretical unification with other fundamental interactions, as found e.g. in string and M-theory. Such schemes offer new, unconventional and promising ways to address cosmological questions. They also allow the investigation of a relation between the source of Dark Energy and other questions, like inflation and Dark Matter of the universe. Light scalar fields related to Dark Energy may correspond to moduli fields in compactified string theory that play a significant role in the process of supersymmetry breaking. These in turn might be tested indirectly in particle physics experiments. The adjustment of the vacuum energy in string theory often requires a specific uplifting scheme from AdS? space in higher dimensions, which leaves characteristic traces in the low energy effective theories. It is now the time to consider explicit string theory realisations of particle physics models and explore the wide range of applications towards an understanding of the nature of Dark Energy and Dark Matter.

Another route explores the relation between quintessence and higher-dimensional dilatation symmetry. Dilatation symmetry may be realised approximately if the late time behaviour of a cosmological runaway solution approaches a fixed point. The light scalar field can then be associated to the Goldstone boson of spontaneously broken dilatation symmetry. This cosmon field acquires a potential and a mass only due to dilatation anomalies that vanish for asymptotically large time as the fixed point is approached. Interesting suggestions that higher-dimensional dilatation symmetry forbids an effective four-dimensional cosmological constant will be pursued. Time varying scalar fields may also lead to a time variation of fundamental couplings. We will investigate the consequences for observational tests of such variations.

Role within the Transregional Collaborative Research Centre

There are strong connections between the theory groups in Bonn, Heidelberg and Munich, as can be seen by the exchange of people (Dr. Lüdeling from Heidelberg to Bonn, Dr. Vaudrevange from Bonn to Munich, Dr. Groot Nibbelink from Heidelberg to Munich) and by a number of joint publications. Within the TR33, this will lead to collaboration with the projects A2 and A3 which investigate inflationary and more formal aspects, respectively. Furthermore, the search for indirect evidence about Dark Energy will certainly also connect to Dark Matter, in particular A4 and C4, and the astrophysical observations of the B projects. Finally, models of Dark Energy will possibly lead to modifications of gravity due to some higher-dimensional effects (A6) and might help to answer the "Why Now" problem, project C6.
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