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Massive neutrinos and cosmology
The present experimental results on neutrino flavour oscillations provide evidence for non-
zero neutrino masses, but give no hint on their absolute mass scale, which is the target of …
zero neutrino masses, but give no hint on their absolute mass scale, which is the target of …
Theoretical models of dark energy
J Yoo, Y Watanabe - International Journal of Modern Physics D, 2012 - World Scientific
Mounting observational data confirm that about 73% of the energy density consists of dark
energy which is responsible for the current accelerated expansion of the Universe. We …
energy which is responsible for the current accelerated expansion of the Universe. We …
Inflation, the Hubble tension, and early dark energy: An alternative overview
W Giarè - Physical Review D, 2024 - APS
I review and discuss the possible implications for inflation resulting from considering new
physics in light of the Hubble tension. My study is motivated by a simple argument that the …
physics in light of the Hubble tension. My study is motivated by a simple argument that the …
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
ABSTRACT We introduce the Illustris Project, a series of large-scale hydrodynamical
simulations of galaxy formation. The highest resolution simulation, Illustris-1, covers a …
simulations of galaxy formation. The highest resolution simulation, Illustris-1, covers a …
Planck 2013 results. I. Overview of products and scientific results
PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2014 - aanda.org
The European Space Agency's Planck satellite, dedicated to studying the early Universe
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …
SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope
We describe the design of a new polarization sensitive receiver, spt-3g, for the 10-meter
South Pole Telescope (spt). The spt-3g receiver will deliver a factor of~ 20 improvement in …
South Pole Telescope (spt). The spt-3g receiver will deliver a factor of~ 20 improvement in …
Planck 2013 results. XII. Diffuse component separation
PAR Ade, N Aghanim, C Armitage-Caplan… - Astronomy & …, 2014 - aanda.org
Planck has produced detailed all-sky observations over nine frequency bands between 30
and 857 GHz. These observations allow robust reconstruction of the primordial cosmic …
and 857 GHz. These observations allow robust reconstruction of the primordial cosmic …
The 10 meter south pole telescope
JE Carlstrom, PAR Ade, KA Aird… - Publications of the …, 2011 - iopscience.iop.org
ABSTRACT The South Pole Telescope (SPT) is a 10 m diameter, wide-field, offset Gregorian
telescope with a 966 pixel, multicolor, millimeter-wave, bolometer camera. It is located at the …
telescope with a 966 pixel, multicolor, millimeter-wave, bolometer camera. It is located at the …
TASI lectures on inflation
D Baumann - arxiv preprint arxiv:0907.5424, 2009 - arxiv.org
In a series of five lectures I review inflationary cosmology. I begin with a description of the
initial conditions problems of the Friedmann-Robertson-Walker (FRW) cosmology and then …
initial conditions problems of the Friedmann-Robertson-Walker (FRW) cosmology and then …
Measuring the reionization optical depth without large-scale CMB polarization
We study the possibility of measuring the optical depth at reionization τ without relying on
large-scale cosmic microwave background (CMB) polarization. Our analysis is driven by the …
large-scale cosmic microwave background (CMB) polarization. Our analysis is driven by the …