ON THE CONTRIBUTION OF DENSITY PERTURBATIONS AND GRAVITATIONAL WAVES TO THE LOWER ORDER MULTIPOLES OF THE COSMIC MICROWAVE BACKGROUND RADIATION [PDF]
A. Dimitropoulos, L. P. Grishchuk
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What does cosmology teach us about non-gravitational properties of dark matter?
Cosmological observations provide our most robust evidence for dark matter that is (approximately) collisionless and cold, and furthermore can provide powerful tests of the non-gravitational properties of dark matter.
Tracy R. Slatyer
doaj
It is well known that multiple Galactic thermal dust emission components may exist along the line of sight, but a single-component approximation is still widely used, since a full multicomponent estimation requires a large number of frequency bands that ...
Hao Liu, Jia-Rui Li, Yi-Fu Cai
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Southern Hemisphere measurements of the anisotropy in the cosmic microwave background radiation
G. F. Smoot, P. M. Lubin
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The Annulus‐filteredEandBModes in Cosmic Microwave Background Radiation Polarization [PDF]
Tzihong Chiueh, Cheng‐Jiun Ma
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Alleviating H 0 and S 8 Tensions Simultaneously in K-essence Cosmology
The present work begins by examining the early-Universe inflationary epoch of a special K-essence model, which incorporates a linear coupling term between the scalar field potential and the canonical Lagrangian.
Seyed Ali Hosseini Mansoori+1 more
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The cosmic microwave background radiation power spectrum as a random bit generator for symmetric- and asymmetric-key cryptography. [PDF]
Lee JS, Cleaver GB.
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Measurements of the cosmic microwave background radiation temperature at 90 GHz
Marco Bersanelli+6 more
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First Measurements of the Polarization of the Cosmic Microwave Background Radiation at Small Angular Scales from CAPMAP [PDF]
D. Barkats+12 more
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