期刊
PHYSICAL REVIEW D
卷 90, 期 10, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.90.105023
关键词
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资金
- European Research Council [StG2010-257080]
- Leverhulme
- Science and Technology Facilities Council (STFC)
- Beecroft Institute for Particle Astrophysics and Cosmology (BIPAC)
- Oxford Martin School
- Royal Society University Research Fellowship
- Perimeter Institute for Theoretical Physics
- Government of Canada through Industry Canada
- Province of Ontario through the Ministry of Economic Development Innovation
- Science and Technology Facilities Council [ST/I00193X/1, ST/K00106X/1] Funding Source: researchfish
- STFC [ST/K00106X/1, ST/I00193X/1] Funding Source: UKRI
The archetypal theory of dark energy is quintessence: a minimally coupled scalar field with a canonical kinetic energy and potential. By studying random potentials, we show that quintessence imposes a restricted set of priors on the equation of state of dark energy. Focusing on the commonly used parametrization, w(a) approximate to w(0) + w(a)(1 - a), we show that there is a natural scale and direction in the (w(0,) w(a)) plane that distinguishes quintessence as a general framework. We calculate the expected information gain for a given survey and show that, because of the nontrivial prior information, it is a function of more than just the figure of merit. This allows us to make a quantitative case for novel survey strategies. We show that the scale of the prior sets target observational requirements for gaining significant information. This corresponds to a figure of merit FOM greater than or similar to 200, a requirement that future galaxy redshift surveys will meet.
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