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Constraining Dark Energy with Type Ia Supernovae and Large-Scale Structure

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Constraining Dark Energy with Type Ia Supernovae and Large-Scale Structure (English)

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Martin White

3

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Saul Perlmutter

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Saul Perlmutter

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1

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Michael Turner

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2

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Michael S. Turner

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language of work or name

English

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publication date

26 July 1999

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published in

Physical Review Letters

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volume

83

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issue

4

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page(s)

670-673

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cites work

The High‐Z Supernova Search: Measuring Cosmic Deceleration and Global Curvature of the Universe Using Type Ia Supernovae

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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

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The cosmological constant problem

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Cosmology with ultralight pseudo Nambu-Goldstone bosons.

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Cosmological Imprint of an Energy Component with General Equation of State

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Cosmological consequences of a rolling homogeneous scalar field

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Supernova Limits on the Cosmic Equation of State

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Formation of galaxies and large-scale structure with cold dark matter

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Four-Year [ITAL]COBE[/ITAL] DMR Cosmic Microwave Background Observations: Maps and Basic Results

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Quintessence, Cosmic Coincidence, and the Cosmological Constant

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Complementary Measures of the Mass Density and Cosmological Constant

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The 4 YearCOBENormalization and Large‐Scale Structure

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The cosmic microwave background and observational convergence in the {Omega}_m_-{Omega}_{Lambda}_ plane

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11 October 2022

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The age of globular clusters in light of Hipparcos: resolving the age problem?

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Where is the dark matter?

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An isocurvature cold dark matter cosmogony. II. Observational tests

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An isocurvature cold dark matter cosmogony. I. A worked example of evolution through inflation

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https://opencitations.net/index/coci/api/v1/references/10.1103/PHYSREVLETT.83.670

The deuterium abundance toward QSO 1009+2956

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11 October 2022

https://opencitations.net/index/coci/api/v1/references/10.1103/PHYSREVLETT.83.670

DynamicalΛmodels of structure formation

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11 October 2022

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Constraints on omega-^- and omega-m- from distant type Ia supernovae and cosmic microwave background anisotropies

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11 October 2022

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Galaxy clusters at 0.3 <z< 0.4 and the value of omega-0-

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The deuterium abundance toward Q1937-1009

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11 October 2022

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(Q55889415)

Constraining Dark Energy with Type Ia Supernovae and Large-Scale Structure

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