SuperIso v3.0, flavor physics observables calculations: extension to NMSSM

SuperIso v3.0, flavor physics observables calculations: extension to NMSSM
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SuperIso v3.0,风味物理可观测量计算:扩展到 NMSSM

DOI:
10.1016/j.cpc.2009.05.001
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发表时间:
2009
期刊:
Comput. Phys. Commun.
影响因子:
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通讯作者:
F. Mahmoudi
F. Mahmoudi
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文献类型:
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作者:
F. Mahmoudi

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SuperIso v3.0是一个公共程序,用于评估标准模型的最小超对称扩展(MSSM)和标准模型的次最小超对称扩展(NMSSM)中的风味物理可观测性。SuperIso v3.0融合了B→Xsγ的包含性分支率、B→K∗γ的同位旋不对称性、BS→μ+μ−的分支率、B→τντ的分支率、B→Dτντ的分支率、K→μνμ的分支率以及ds→τντ和ds→μνμ的分支率等多种风味观察结果。B→xsγ支化比的计算包含了NNLO标准模型贡献。该程序还计算了Muon反常磁矩(g−2)。该包包括七个样本模型,即用于MSSM的mSUGRA、NUHM、AMSB和GMSB,以及用于NMSSM的CNMSSM、NGMSB和NNUHM。SuperIso使用SUSY Les Houches Accord文件(SLHA1或SLHA2)作为输入,该文件可以由程序通过调用外部频谱计算器(SOFTSUSY、ISAJET或NMSSMTools)自动生成,也可以由用户提供。新版计划概要:计划标题:SuperISO v3.0目录标识符:AEAN_V3_0计划概要URL:http://cpc.cs.qub.ac.uk/summaries/AEAN_v3_0.html计划可从:爱尔兰贝尔法斯特女王大学CPC计划图书馆获得许可条款:GNU通用公共许可证号。分布式程序中的行数,包括测试数据等:6869第分布式程序中的字节数,包括测试数据等:42 627分布格式:tar.gz编程语言:C(符合C99标准)计算机:32位或位PC,Mac操作系统:LINUX,MacOSRAM:小于1MB分类:11.6外部例程:ISASUGRA/ISAJET,SOFTSUSY和/或NMS工具新版本是否取代了以前的版本?:是的,问题的性质:在最小的超对称标准模型中,在最小的违反最小的超对称标准模型中,以及在次小的超对称模型中,为了推导对超对称参数空间的约束,计算风味物理观察值以及Muon反常磁矩。解决方法:SuperIso使用SUSY Les Houches Accord(SLHA1或SLHA2)文件,该文件可以通过调用SOFTSUSY、ISAJET或NMSSMTools自动生成,也可以由用户提供。该文件包含超对称粒子的质量、混合和耦合。然后,SuperIso计算出最受约束的味道物理可观测值和介子(g−2)。SuperIso能够在不同的超对称破缺场景下执行计算,如mSUGRA、NUHM、AMSB和GMSB,以及约束的NMSSM场景,如CNMSSM、NNUHM和NGMSB。新版本的原因:SuperIso已经扩展到标准模型的下一个最小超对称扩展(NMSSM)。因此,实现的例程被广泛修改。修订摘要:不寻常的特点:代码非常灵活,可以很容易地添加新的可观测对象。运行时间:不到1秒
SuperIso v3.0 is a public program for evaluation of flavor physics observables in the minimal supersymmetric extension of the Standard Model (MSSM) and the next to minimal supersymmetric extension of the Standard Model (NMSSM). SuperIso v3.0 incorporates many flavor observables such as the inclusive branching ratio of B→Xsγ, the isospin asymmetry of B→K∗γ, the branching ratio of Bs→μ+μ−, the branching ratio of B→τντ, the branching ratio of B→Dτντ, the branching ratio of K→μνμand the branching ratios of Ds→τντand Ds→μνμ. The calculation of the branching ratio of B→Xsγ includes NNLO Standard Model contributions. The program also computes the muon anomalous magnetic moment (g−2). Seven sample models are included in the package, namely mSUGRA, NUHM, AMSB and GMSB for the MSSM, and CNMSSM, NGMSB and NNUHM for the NMSSM. SuperIso uses a SUSY Les Houches Accord file (SLHA1 or SLHA2) as input, which can be either generated automatically by the program via a call to external spectrum calculators (SOFTSUSY, ISAJET or NMSSMTools), or provided by the user. NEW VERSION PROGRAM SUMMARY: Program title:SuperIso v3.0 Catalogue identifier: AEAN_v3_0 Program summary URL:http://cpc.cs.qub.ac.uk/summaries/AEAN_v3_0.html Program obtainable from: CPC Program Library, Queen's University, Belfast, N. Ireland Licensing provisions: GNU General Public Licence No. of lines in distributed program, including test data, etc.: 6869 No. of bytes in distributed program, including test data, etc.: 42 627 Distribution format: tar.gz Programming language: C (C99 Standard compliant) Computer: 32- or 64-bit PC, Mac Operating system: Linux, MacOS RAM: less than 1 MB Classification: 11.6 External routines: ISASUGRA/ISAJET, SOFTSUSY and/or NMSSMTools Does the new version supersede the previous version?: Yes Nature of problem: Calculation of flavor physics observables as well as the muon anomalous magnetic moment in the Minimal Supersymmetric Standard Model with minimal flavor violation and in the Next to Minimal Supersymmetric Standard Model, in order to derive constraints on the supersymmetric parameter spaces. Solution method:SuperIso uses a SUSY Les Houches Accord (SLHA1 or SLHA2) file, which can be either generated automatically via a call to SOFTSUSY, ISAJET or NMSSMTools, or provided by the user. This file contains the masses, mixings and couplings of the supersymmetric particles. SuperIso then computes the most constraining flavor physics observables and the muon (g−2). SuperIso is able to perform the calculations in different supersymmetry breaking scenarios, such as mSUGRA, NUHM, AMSB and GMSB, as well as constrained NMSSM scenarios such as CNMSSM, NNUHM and NGMSB. Reasons for new version:SuperIso has been extended to the next to minimal supersymmetric extension of the Standard Model (NMSSM). The implemented routines are therefore extensively modified. Summary of revisions: Unusual features: The code is very flexible, and new observables can be added easily. Running time: Less than 1 sec