1,408 results for Parameter HD Wallpaper

arxiv.org/abs/1207.4476v1

The nature of assembly bias - II. Halo spin

We study an assembly-type bias parametrized by the dimensionless spin parameter that affects massive structures. In numerical simulations higher spin haloes are more strongly clustered than lower spin haloes of equal mass. We detect a difference of o...

arxiv.org/abs/1307.8444v2

pMSSM Studies at the 7, 8 and 14 TeV LHC

The 19/20-parameter p(henomenological)MSSM with either a neutralino or gravitino LSP offers a flexible framework for the study of a wide variety of R-parity conserving MSSM SUSY phenomena at the 7, 8 and 14 TeV LHC. Here we present the results of a s...

arxiv.org/abs/2302.00460v2

Explaining the Entropy Forming Ability with the atomic size mismatch

To quickly screen for single-phased multi-principal-element materials, a so-called entropy forming ability (EFA) parameter is sometimes used as a descriptor. The higher the EFA, the higher is the propensity to form a single-phase structure, which is...

arxiv.org/abs/astro-ph/0203304v1

UU Aqr from high to low state

In this paper we present Physical Parameter Eclipse Mapping (PPEM) of UBVRI eclipse light curves of UU Aqr from high to low states. We used a simple, pure hydrogen LTE model to derive the temperature and surface density distribution in the accretio...

arxiv.org/abs/2406.08892v1

Minimaxity under the half-Cauchy prior

This is a follow-up paper of Polson and Scott (2012, Bayesian Analysis), which claimed that the half-Cauchy prior is a sensible default prior for a scale parameter in hierarchical models. For estimation of a p-variate normal mean under the quadratic...

arxiv.org/abs/2203.05616v1

Cosmologia com aglomerados de galáxias

Galaxy clusters are important cosmological probes since their abundance and spatial distribution are directly linked to structure formation on large scales. The principal uncertainty source on the cosmological parameter constraints concerns the clust...