[HTML][HTML] Feebly-interacting particles: FIPs 2022 workshop report
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
Cosmological constant—the weight of the vacuum
T Padmanabhan - Physics reports, 2003 - Elsevier
Recent cosmological observations suggest the existence of a positive cosmological constant
Λ with the magnitude Λ (Gℏ/c3)≈ 10− 123. This review discusses several aspects of the …
Λ with the magnitude Λ (Gℏ/c3)≈ 10− 123. This review discusses several aspects of the …
[HTML][HTML] The cosmological constant
SM Carroll - Living reviews in relativity, 2001 - Springer
This is a review of the physics and cosmology of the cosmological constant. Focusing on
recent developments, I present a pedagogical overview of cosmology in the presence of a …
recent developments, I present a pedagogical overview of cosmology in the presence of a …
Toward a halo mass function for precision cosmology: The Limits of universality
We measure the mass function of dark matter halos in a large set of collisionless
cosmological simulations of flat ΛCDM cosmology and investigate its evolution at z\lesssim …
cosmological simulations of flat ΛCDM cosmology and investigate its evolution at z\lesssim …
[HTML][HTML] The cosmological constant
The cosmological constant ADS Classic is now deprecated. It will be completely retired in
October 2019. This page will automatically redirect to the new ADS interface at that point …
October 2019. This page will automatically redirect to the new ADS interface at that point …
Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
We present gas and total mass profiles for 13 low-redshift, relaxed clusters spanning a
temperature range 0.7-9 keV, derived from all available Chandra data of sufficient quality. In …
temperature range 0.7-9 keV, derived from all available Chandra data of sufficient quality. In …
The large-scale bias of dark matter halos: Numerical calibration and model tests
We measure the clustering of dark matter halos in a large set of collisionless cosmological
simulations of the flat ΛCDM cosmology. Halos are identified using the spherical overdensity …
simulations of the flat ΛCDM cosmology. Halos are identified using the spherical overdensity …
Semi-analytic modelling of galaxy formation: the local Universe
Using semi-analytic models of galaxy formation, we investigate galaxy properties such as
the Tully-Fisher relation, the B-and K-band LFs, cold gas contents, sizes, metallicities and …
the Tully-Fisher relation, the B-and K-band LFs, cold gas contents, sizes, metallicities and …
Cosmology with the Sunyaev-Zel'dovich effect
JE Carlstrom, GP Holder… - Annual Review of …, 2002 - annualreviews.org
▪ Abstract The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-
scale structure of the universe as traced by massive clusters of galaxies. As a spectral …
scale structure of the universe as traced by massive clusters of galaxies. As a spectral …
Environmental Effects on Late‐Type Galaxies in Nearby Clusters
A Boselli, G Gavazzi - Publications of the Astronomical Society of …, 2006 - iopscience.iop.org
The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …