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相关论文: Future Supernovae observations as a probe of dark …

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We investigate the potential of a future supernova dataset, as might be obtained by the proposed SNAP satellite, to discriminate among different ``dark energy'' theories that describe an accelerating Universe. We find that many such models…

天体物理学 · 物理学 2010-04-08 Jochen Weller , Andreas Albrecht

It has now been firmly established that the Universe is expanding at an accelerated rate, driven by a presently unknown form of dark energy that appears to dominate our Universe today. A dedicated satellite mission has been designed to…

天体物理学 · 物理学 2009-11-10 Michael Schubnell

The distance-redshift relation observed for supernovae has led to the discovery that the expansion of the universe is accelerating. A next generation experiment, the Supernova/Acceleration Probe (SNAP), can investigate the nature of the…

天体物理学 · 物理学 2017-08-23 Eric V. Linder

The quality of supernova data will dramatically increase in the next few years by new experiments that will add high-redshift supernova to the currently known ones. In order to use this new data to discriminate between different dark energy…

天体物理学 · 物理学 2015-06-24 Emille E. O. Ishida

We investigate the potential of a future supernovae data set, as might be obtained by the proposed SNAP satellite, to discriminate between two possible explanations for the observed dimming of the high redshift type IA supernovae, namely…

天体物理学 · 物理学 2009-11-06 S. C. C. Ng , D. L. Wiltshire

We explore the prospects for using future supernova observations to probe the dark energy. We focus on quintessence, an evolving scalar field that has been suggested as a candidate for the dark energy. After simulating the observations that…

天体物理学 · 物理学 2009-11-07 Brian F. Gerke , G. Efstathiou

Observation of thousands of type Ia supernovae should offer the most direct approach to probe the dark energy content of the universe. This will be undertaken by future large ground-based surveys followed by a space mission (SNAP/JDEM). We…

天体物理学 · 物理学 2009-11-10 J. -M. Virey , P. Taxil , A. Tilquin , A. Ealet , D. Fouchez , C. Tao

The use of Type Ia supernovae as calibrated standard candles is one of the most powerful tools to study the expansion history of the universe and thereby its energy components. While the analysis of some ~50 supernovae at redshifts around…

天体物理学 · 物理学 2009-11-06 M. Goliath , R. Amanullah , P. Astier , A. Goobar , R. Pain

The Supernova / Acceleration Probe (SNAP) is a proposed space-based experiment designed to study the dark energy and alternative explanations of the acceleration of the Universe's expansion by performing a series of complementary…

The coming few years are likely to witness a dramatic increase in high quality Sn data as current surveys add more high redshift supernovae to their inventory and as newer and deeper supernova experiments become operational. Given the…

天体物理学 · 物理学 2008-11-26 Ujjaini Alam , Varun Sahni , Tarun Deep Saini , A. A. Starobinsky

The Supernova Acceleration Probe (SNAP) will use Type Ia supernovae (SNe Ia) as distance indicators to measure the effect of dark energy on the expansion history of the Universe. (SNAP's weak-lensing program is described in a companion…

天体物理学 · 物理学 2012-08-27 SNAP Collaboration

The SuperNova / Acceleration Probe (SNAP) is a space-based experiment to measure the expansion history of the Universe and study both its dark energy and the dark matter. The experiment is motivated by the startling discovery that the…

天体物理学 · 物理学 2015-06-24 G. Aldering , SNAP collaboration

The SuperNovae Analysis aPplication (SNAP) is a new tool for the analysis of SN observations and validation of SN models. SNAP consists of an open source relational database with (a) observational light curve, (b) theoretical light curve,…

The time dependence of the dark energy density can be an important clue to the nature of dark energy in the universe. We show that future supernova data from dedicated telescopes (such as SNAP), when combined with data of nearby supernovae,…

天体物理学 · 物理学 2014-10-13 Yun Wang , Veselin Kostov , Katherine Freese , Joshua A. Frieman , Paolo Gondolo

The accelerating expansion of the Universe is one of the most surprising and potentially profound discoveries of modern cosmology. Measuring the acceleration well enough to meaningfully constrain interesting physical models requires…

天体物理学 · 物理学 2009-11-13 G. Aldering

The possibility to unambiguously determine the equation-of-state of the cosmic dark energy with existing and future supernovae data is investigated. We consider four evolution laws for this equation-of-state corresponding to four…

天体物理学 · 物理学 2011-05-05 Elisa Di Pietro , Jean-Francois Claeskens

This talk presents a pedagogical discussion of how precision distance-redshift observations can map out the recent expansion history of the universe, including the present acceleration and the transition to matter dominated deceleration.…

天体物理学 · 物理学 2009-11-07 Eric V. Linder

In this paper we discuss the possibility to measure the Hubble parameter and the slope of galaxy density profiles using future supernova data. With future supernova surveys such as SNAP, large numbers of core collapse supernovae will be…

天体物理学 · 物理学 2009-11-10 Edvard Mortsell , Haakon Dahle , Steen Hannestad

The surprising discovery of an accelerating universe led cosmologists to posit the existence of "dark energy"--a mysterious energy field that permeates the universe. Understanding dark energy has become the central problem of modern…

天体物理学 · 物理学 2009-05-18 Christopher Genovese , Peter Freeman , Larry Wasserman , Robert Nichol , Christopher Miller

For true insight into the nature of dark energy, measurements of the precision and accuracy of the Supernova/Acceleration Probe (SNAP) are required. Precursor or scaled-down experiments are unavoidably limited, even for distinguishing the…

天体物理学 · 物理学 2012-08-27 SNAP Collaboration
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