Results 141 to 150 of about 298,499 (308)

HI and Cosmology: What We Need To Know [PDF]

open access: yes, 2008
There are three distinct regimes in which radio observations of the redshifted 21 cm line of HI can contribute directly to cosmology in unique ways. The regimes are naturally divided by redshift, from high to low, into: inflationary physics, the Dark ...
Bowman, Judd D.
core   +1 more source

Cosmology and Astrophysics

open access: yes, 2005
76 pages, 36 figures, invited Lectures, to appear in the Proceedings of the CERN-JINR European School of High Energy Physics, San Feliu (Spain), 30 May - 12 June ...
openaire   +2 more sources

The Evolution of a Polar Cap Patch Into a Blob in the Nightside Ionosphere: Direct Observations of Multiple Blob Formation Mechanisms Acting Simultaneously on the Same Plasma

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract A polar cap patch was observed to exit the polar cap to become a blob as it entered the auroral oval on the nightside of the Earth under moderately quiet geomagnetic conditions (Kp = 3−). Auroral particle precipitation led to an increase in the electron density of the blob.
S. J. Maguire   +9 more
wiley   +1 more source

Diffusion-HMC: Parameter Inference with Diffusion-model-driven Hamiltonian Monte Carlo

open access: yesThe Astrophysical Journal
Diffusion generative models have excelled at diverse image generation and reconstruction tasks across fields. A less explored avenue is their application to discriminative tasks involving regression or classification problems.
Nayantara Mudur   +2 more
doaj   +1 more source

Astrophysics and Cosmology

open access: yes, 2000
Invited Lectures at 1999 European School of High Energy Physics, Casta-Papiernicka, Slovak Republic, 22 August - 4 September 1999 78 pages, 42 figures, uses cernrep ...
openaire   +2 more sources

Phase‐Space Synchronization Driven by Moon‐Magnetosphere Coupling in Gas Giants

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract We present a new theoretical framework to describe the rapid and spatially localized loss of energetic particles in planetary radiation belts, focusing on interactions between gas giant magnetospheres and their moons. Observations show that flux depletions—known as microsignatures—often refill on timescales comparable to a single drift period,
Adnane Osmane   +2 more
wiley   +1 more source

Periodic Density Structures Observed in Ulysses Data: First Results

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract Periodic density structures (PDSs) are advecting quasi‐periodic (periodicities between several minutes and several hours) density enhancements observed in the solar wind and corona. There is strong evidence that PDSs are formed at the Sun.
Brent M. Randol   +3 more
wiley   +1 more source

Characterizing the Signals and Backgrounds in a Low Earth Orbiting Cherenkov Detector, and Background Mitigation Strategies

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract Cherenkov detectors have been used in space for decades to measure Galactic Cosmic Rays (GCRs), Solar Energetic Particles (SEPs) and trapped particles. We present proof‐of‐concept GRAS/Geant4 simulations to both show that a cubic fused silica Cherenkov detector with SiPM in LEO has a good sensitivity to SEP and GCR protons as a function of cut‐
C. S. W. Davis   +6 more
wiley   +1 more source

Characterizing the Nanohertz Gravitational Wave Background Using a t-process Power Spectral Density

open access: yesThe Astrophysical Journal
Pulsar timing arrays (PTAs) are sensitive to low-frequency gravitational waves (GWs), which induce correlated changes in millisecond pulsars’ timing residuals.
Shashwat C. Sardesai   +2 more
doaj   +1 more source

Stellar populations in the ELT perspective

open access: yes, 2014
We discuss the impact that the next generation of Extremely Large Telescopes will have on the open astrophysical problems of resolved stellar populations.
Bono, G.   +13 more
core  

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