GravitinoPack and decays of supersymmetric metastable particles

Abstract We present the package GravitinoPack that calculates the two- and three-body decays of unstable supersymmetric particles involving the gravitino in the final or initial state. In a previous paper, we already showed results for the gravitino decaying into two and three particles. In this paper, we incorporate the processes where an unstable neutralino, stau or stop decays into a gravitino and Standard Model particles. This is the case in gravitino dark matter supersymmetric models, where the gravitino is the lightest SUSY particle. We give instructions for the installation and the use of the package. In the numerical analysis, we discuss various MSSM scenarios. We show that the calculation of all the decay channels and the three-body decay branching ratios is essential for the accurate application of cosmological bounds on these models. Program summary Program title: GravitinoPack Catalogue identifier: AEZL_v1_0 Program summary URL: http://cpc.cs.qub.ac.uk/summaries/AEZL_v1_0.html Program obtainable from: CPC Program Library, Queen’s University, Belfast, N. Ireland Licensing provisions: Standard CPC licence, http://cpc.cs.qub.ac.uk/licence/licence.html No. of lines in distributed program, including test data, etc.: 97708 No. of bytes in distributed program, including test data, etc.: 1217167 Distribution format: tar.gz Programming language: Fortran 77 and C for the MathLink. Computer: Workstation, PC, Mac. Operating system: Linux, Mac OSX. Classification: 11.1. Nature of problem: If Supersymmetry (SUSY) is realized in nature, each Standard Model (SM) particle is accompanied by its superpartner. The gravitino, the spin 3/2 superpartner of the graviton, belongs to the spectrum of the most important supersymmetric models. The gravitino can be the Lightest Supersymmetric Particle (LSP), in the so-called gravitino Dark Matter (DM) models. Thus, the Next to the Lightest Supersymmetric Particle (NLSP) is long-lived, since it decays gravitationally to the LSP (gravitino) and SM particles. Such decays produce electromagnetic energy and hadrons which can affect the primordial Big-Bang Nucleosynthesis (BBN) predictions for the abundance of the light nuclei. Similarly, when the gravitino is not the LSP it decays into the LSP which can be another SUSY particle, like the neutralino, and SM particles. GravitinoPack provides important results on all these decays, making the application of the BBN data more accurate. Solution method: GravitinoPack is a package for the evaluation of processes with gravitino interaction. The version GravitinoPack1.0 includes all two-body decays of the gravitino and all three-body decays of the gravitino to a neutralino and a pair of two particles. In the case that the gravitino is the LSP all two- and three-body decays of the lightest neutralino, the light stop or stau NLSP are included. GravitinoPack works at Fortran77 level and has a Mathematica interface. Unusual features: MathLink works properly only up to version Mathematica 9. There is still a conflict between Mathematica 10 and the used integration routine CUBA. Running time: All two-body decay widths are calculated in a time far below one second. The three-body decay calculations can be fast, especially the stop and stau decays, or slow with times up to a few minutes, especially when the phase space becomes large and no approximation is chosen.

[1]  T. Hahn,et al.  The implementation of the Minimal Supersymmetric Standard Model in FeynArts and FormCalc , 2002 .

[2]  E. Condon The Theory of Groups and Quantum Mechanics , 1932 .

[3]  B. Fields,et al.  Nucleosynthesis constraints on a massive gravitino in neutralino dark matter scenarios , 2009, 0907.5003.

[4]  M. P. Casado,et al.  Summary of the ATLAS experiment’s sensitivity to supersymmetry after LHC Run 1 — interpreted in the phenomenological MSSM , 2015, 1508.06608.

[5]  M. Drees,et al.  Neutralino relic density in minimal N=1 supergravity. , 1992, Physical Review D, Particles and fields.

[6]  A. Belyaev,et al.  Neutralino cold dark matter in a one parameter extension of the minimal supe , 2004, hep-ph/0412059.

[7]  Updated Nucleosynthesis Constraints on Unstable Relic Particles , 2002, astro-ph/0211258.

[8]  J. Pradler Electroweak Contributions to Thermal Gravitino Production , 2007, 0708.2786.

[9]  S. M. Etesami,et al.  Searches for third-generation squark production in fully hadronic final states in proton-proton collisions at s=8$$ \sqrt{s}=8 $$ TeV , 2015 .

[10]  Claude Duhr,et al.  FeynRules 2.0 - A complete toolbox for tree-level phenomenology , 2013, Comput. Phys. Commun..

[11]  C. A. Oxborrow,et al.  Planck2015 results , 2015, Astronomy & Astrophysics.

[12]  Werner Porod,et al.  SPheno 3.1: extensions including flavour, CP-phases and models beyond the MSSM , 2011, Comput. Phys. Commun..

[13]  Kane,et al.  Study of constrained minimal supersymmetry. , 1993, Physical review. D, Particles and fields.

[14]  S. Heinemeyer,et al.  Towards high-precision predictions for the MSSM Higgs sector , 2002, hep-ph/0212020.

[15]  Khachatryan,et al.  Search for supersymmetry with photons in pp collisions at √s=8 TeV , 2015 .

[16]  T. Hahn,et al.  Automatized One-Loop Calculations in 4 and D dimensions , 1998 .

[17]  J. T. Childers,et al.  Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC , 2012 .

[18]  J. Ellis,et al.  The Cosmology of Decaying Gravitinos , 1985 .

[19]  D. Lindley Hadronic decays of cosmological gravitinos , 1986 .

[20]  D. Lindley Cosmological constraints on the lifetime of massive particles , 1985 .

[21]  D. Nanopoulos,et al.  Neutralino relic density in a universe with a nonvanishing cosmological constant , 1999, hep-ph/9909497.

[22]  J. Ellis,et al.  Supersymmetric dark matter in the light of LEP 1.5 , 1996, hep-ph/9607292.

[23]  The CMSSM parameter space at large /tanβ , 2001, hep-ph/0102098.

[24]  S. Heinemeyer,et al.  The Higgs Boson Masses and Mixings of the Complex MSSM in the Feynman-Diagrammatic Approach , 2007 .

[25]  M. Turner,et al.  Primordial nucleosynthesis with decaying particles. I. Entropy-producing decays. II. Inert decays , 1988 .

[26]  H. Eberl,et al.  Three-body gravitino decays in the MSSM , 2013, 1305.6934.

[27]  Cosmological relic density from minimal supergravity with implications for collider physics. , 1995, Physical review. D, Particles and fields.

[28]  J. T. Childers,et al.  Search for the decay Bs0→μ+μ- with the ATLAS detector , 2012 .

[29]  Hadronic decay of late-decaying particles and big-bang nucleosynthesis , 2004, astro-ph/0402490.

[30]  G. Starkman,et al.  Limits on Late Decaying Particles From Nucleosynthesis , 1989 .

[31]  T. Hahn,et al.  Generating Feynman Diagrams and Amplitudes with FeynArts 3 , 2001 .

[32]  S. M. Etesami,et al.  Observation of the rare Bs0 →µ+µ− decay from the combined analysis of CMS and LHCb data , 2014, Nature.

[33]  G. Starkman,et al.  Is the Universe Closed by Baryons? Nucleosynthesis with a Late-decaying Massive Particle , 1988 .

[34]  Ryszard S. Romaniuk,et al.  Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC , 2012 .

[35]  Gravitino Production in the Inflationary Universe and the Effects on Big-Bang Nucleosynthesis , 1994, hep-ph/9403364.

[36]  M. Tinkham Group Theory and Quantum Mechanics , 1964 .

[37]  New Cosmological and Experimental Constraints on the CMSSM , 2001, hep-ph/0106334.

[38]  A. Denner,et al.  Feyn Arts ― computer-algebraic generation of Feynman graphs and amplitudes , 1990 .

[39]  Thomas Hahn,et al.  SUSY Les Houches Accord 2 , 2007, Comput. Phys. Commun..

[40]  D. Seckel,et al.  Primordial nucleosynthesis: The effects of injecting hadrons. , 1988, Physical review. D, Particles and fields.

[41]  Big-Bang nucleosynthesis and hadronic decay of long-lived massive particles , 2004, astro-ph/0408426.

[42]  P. Catastini,et al.  Summary of the searches for squarks and gluinos using s=8$$ \sqrt{s}=8 $$ TeV pp collisions with the ATLAS experiment at the LHC , 2015 .

[43]  P Skands,et al.  SUSY Les Houches accord: interfacing SUSY spectrum calculators, decay packages, and event generators , 2003, hep-ph/0311123.

[44]  J. L. Lopez,et al.  Astrophysical constraints on massive unstable neutral relic particles , 1992 .

[45]  S. Dittmaier Weyl-van der Waerden formalism for helicity amplitudes of massive particles , 1998, hep-ph/9805445.

[46]  Werner Porod,et al.  SPheno, a program for calculating supersymmetric spectra, SUSY particle decays and SUSY particle production at e+e− colliders☆ , 2003, hep-ph/0301101.

[47]  H. Weyl The Theory Of Groups And Quantum Mechanics , 1931 .

[48]  Did something decay, evaporate, or annihilate during Big Bang nucleosynthesis? , 2004, astro-ph/0402344.

[49]  U. Chattopadhyay,et al.  Supersymmetric dark matter and Yukawa unification , 2001, hep-ph/0201001.

[50]  J. Ellis,et al.  Constraining supersymmetry , 2002, hep-ph/0202110.

[51]  J. Ellis,et al.  Varying the universality of supersymmetry-breaking contributions to MSSM Higgs boson masses , 2008, 0805.2343.

[52]  E Aprile,et al.  Dark matter results from 225 live days of XENON100 data. , 2012, Physical review letters.

[53]  Alexander Belyaev,et al.  Direct, indirect and collider detection of neutralino dark matter in SUSY models with non-universal Higgs masses , 2005, hep-ph/0504001.

[54]  C. Duhr,et al.  Simulating spin-$\frac{3}{2}$ particles at colliders , 2013, 1308.1668.

[55]  Edward J. Wollack,et al.  NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS , 2012, 1212.5226.

[56]  Thomas Hahn,et al.  Cuba - a library for multidimensional numerical integration , 2004, Comput. Phys. Commun..

[57]  R. Arnowitt,et al.  Nonuniversal soft supersymmetry breaking and dark matter , 1997 .

[58]  Supersymmetric dark matter in light of WMAP , 2003, hep-ph/0303043.

[59]  B. Fields,et al.  Gravitino decays and the cosmological lithium problem in light of the LHC Higgs and supersymmetry searches , 2013, 1303.0574.

[60]  V. Spanos,et al.  Refining the predictions of supersymmetric CP-violating models: A top-down approach , 2008, 0804.2613.