论文标题

COSMOBIT:用于计算宇宙学观察力和可能性的Gambit模块

CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods

论文作者

Workgroup, The GAMBIT Cosmology, :, Renk, Janina J., Stöcker, Patrick, Bloor, Sanjay, Hotinli, Selim, Balázs, Csaba, Bringmann, Torsten, Gonzalo, Tomás E., Handley, Will, Hoof, Sebastian, Howlett, Cullan, Kahlhoefer, Felix, Scott, Pat, Vincent, Aaron C., White, Martin

论文摘要

我们介绍了$ \ sf {cosmobit} $,一个开源$ \ sf {gambit} $软件框架中的一个模块,用于探索宇宙学与粒子物理之间的连接,并具有联合全球拟合。 $ \ sf {cosmobit} $提供了一个灵活的框架,可用于研究$λ$ CDM以上的各种情况,例如通货膨胀模型,自由度相对论的有效数量的修改,an灭或衰减的暗物质中的异国情调能量注入,以及诸如中性群体和诸如中性群体质量的质量和含量的各种元素的质量。通过$ \ sf {cosmobit} $中的许多可观察力和可能性是通过接口计算到$ \ sf {alterbbn} $,$ \ sf {class} $,$ \ sf {darkages} $,$ \ sf {darkages} $,$ \ sf {montepython} $,$ \ sf} $, $ \ sf {plc} $。这使得可以从大规模结构,IA型超新星,大爆炸核合成和宇宙微波背景中采用广泛的约束。可以使用$ \ sf {gambit} $框架中可用的许多不同统计抽样算法进行参数扫描,并且可以将结果与其他$ \ sf {gambit} $模块的计算结合在一起,这些模块集中在粒子物理和暗物质上。我们包括广泛的验证图,以及对具有非标准相对论自由度和中微子温度的方案的首次应用,表明对中微子质量总和的相应约束要比标准方案中的较弱得多。

We introduce $\sf{CosmoBit}$, a module within the open-source $\sf{GAMBIT}$ software framework for exploring connections between cosmology and particle physics with joint global fits. $\sf{CosmoBit}$ provides a flexible framework for studying various scenarios beyond $Λ$CDM, such as models of inflation, modifications of the effective number of relativistic degrees of freedom, exotic energy injection from annihilating or decaying dark matter, and variations of the properties of elementary particles such as neutrino masses and the lifetime of the neutron. Many observables and likelihoods in $\sf{CosmoBit}$ are computed via interfaces to $\sf{AlterBBN}$, $\sf{CLASS}$, $\sf{DarkAges}$, $\sf{MontePython}$, $\sf{MultiModeCode}$, and $\sf{plc}$. This makes it possible to apply a wide range of constraints from large-scale structure, Type Ia supernovae, Big Bang Nucleosynthesis and the cosmic microwave background. Parameter scans can be performed using the many different statistical sampling algorithms available within the $\sf{GAMBIT}$ framework, and results can be combined with calculations from other $\sf{GAMBIT}$ modules focused on particle physics and dark matter. We include extensive validation plots and a first application to scenarios with non-standard relativistic degrees of freedom and neutrino temperature, showing that the corresponding constraint on the sum of neutrino masses is much weaker than in the standard scenario.

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