1,466 results for parameters

arxiv.org/abs/2402.16396v2

Step-reinforced random walks and one-half

Under suitable moment assumptions, we show that a genuinely d-dimensional step-reinforced random walk undergoes a phase transition between recurrence and transience in dimensions $d=1,2$, and that it is transient for all reinforcement parameters in d...

arxiv.org/abs/1410.4496v3

Global Trends of CME Deflections Based on CME and Solar Parameters

Accurate space weather forecasting requires knowledge of the trajectory of coronal mass ejections (CMEs), including any deflections close to the Sun or through interplanetary space. Kay et al. 2013 introduced ForeCAT, a model of CME deflection result...

arxiv.org/abs/2010.12944v1

On automorphism groups of a biplane (121,16,2)

The existence of a biplane with parameters $(121,16,2)$ is an open problem. Recently, it has been proved by Alavi, Daneshkhah and Praeger that the order of an automorphism group of a of possible biplane ${\mathcal D}$ of order $14$ divides $2^7\cdot3...

arxiv.org/abs/2004.04535v1

Symmetries of biplanes

In this paper, we first study biplanes $\mathcal{D}$ with parameters $(v,k,2)$, where the block size $k\in\{13,16\}$. These are the smallest parameter values for which a classification is not available. We show that if $k=13$, then either $\mathcal{D...

arxiv.org/abs/0810.1758v2

A Simple Comptonization Model

We present an empirical model of Comptonization for fitting the spectra of X-ray binaries. This model, "simpl", has been developed as a package implemented in XSPEC. With only two free parameters, simpl is competitive as the simplest empirical mode...

arxiv.org/abs/1004.3121v2

NLTE wind models of hot subdwarf stars

We calculate NLTE models of stellar winds of hot compact stars (central stars of planetary nebulae and subdwarf stars). The studied range of subdwarf parameters is selected to cover a large part of these stars. The models predict the wind hydrodynami...

arxiv.org/abs/2311.05939v1

SusHi 2.0 -- Higgs production cross sections in BSM models

A new upcoming version of SusHi is introduced. It features unified input for the Standard Model (SM) and beyond the SM models (BSM) parameters for higher-order total cross sections for Higgs production in gluon fusion, heavy-quark annhilation, as wel...

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arxiv.org/abs/2306.14152v1

Low-Rank Prune-And-Factorize for Language Model Compression

The components underpinning PLMs -- large weight matrices -- were shown to bear considerable redundancy. Matrix factorization, a well-established technique from matrix theory, has been utilized to reduce the number of parameters in PLM. However, it f...