(Q57630995)

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Observationally determining the properties of dark matter

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Observationally determining the properties of dark matter (English)

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3

Max Tegmark

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Martin White

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Martin White

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4

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Daniel Eisenstein

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2

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Daniel J. Eisenstein

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Wayne Hu

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1

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Wayne Hu

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language of work or name

English

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publication date

17 December 1998

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published in

Physical Review D

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volume

59

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issue

2

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Measurements of the Cosmological Parameters Ω and Λ from the First Seven Supernovae atz≥ 0.35

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Discovery of a supernova explosion at half the age of the Universe

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Constraints on Cosmological Models from [ITAL]Hubble Space Telescope[/ITAL] Observations of High-[CLC][ITAL]z[/ITAL][/CLC] Supernovae

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

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Cosmological consequences of a rolling homogeneous scalar field

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21 January 2018

Cosmology with a time-variable cosmological 'constant'

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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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21 January 2018

Complementary Measures of the Mass Density and Cosmological Constant

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21 January 2018

The Cosmic Microwave Background Spectrum from the FullCOBEFIRAS Data Set

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Effect of physical assumptions on the calculation of microwave background anisotropies

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Why Not Consider Closed Universes?

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A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies

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The Damping Tail of Cosmic Microwave Background Anisotropies

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Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift Surveys

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Acoustic Signatures in the Cosmic Microwave Background

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Cosmology in a String-Dominated Universe

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The Hubble Diagram of the Calan/Tololo Type IA Supernovae and the Value of HO

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Modelling the redshift-space distortion of galaxy clustering

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DOI

10.1103/PHYSREVD.59.023512

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(Q57630995)

Observationally determining the properties of dark matter

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