Comparison of SUSY spectra generators for natural SUSY and string landscape predictions

Models of natural supersymmetry give rise to a weak scale m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the strin...

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Published in	The European physical journal. C, Particles and fields Vol. 82; no. 2; pp. 1 - 17
Main Authors	Baer, Howard, Barger, Vernon, Martinez, Dakotah
Format	Journal Article
Language	English
Published	Berlin/Heidelberg Springer Berlin Heidelberg 01.02.2022 Springer Springer Nature B.V SpringerOpen
Subjects	Astronomy Astrophysics and Cosmology Building codes Cosmology Elementary Particles Generators Hadrons Heavy Ions Large Hadron Collider LHC Mass spectra Measurement Science and Instrumentation Nuclear Energy Nuclear Physics Physics Physics and Astronomy PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics Statistical analysis string phenomenology String Theory Strings Supersymmetry
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Abstract	Models of natural supersymmetry give rise to a weak scale m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at m h ∼ 125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure Δ EW . The SSS generators tend to yield a Higgs mass peak ∼ 125 –127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to Δ EW in a more standard notation.
AbstractList	Models of natural supersymmetry give rise to a weak scale mweak∼mW,Z,h∼100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at mh∼125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure ΔEW. The SSS generators tend to yield a Higgs mass peak ∼125–127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to ΔEW in a more standard notation. Models of natural supersymmetry give rise to a weak scale m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at m h ∼ 125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure Δ EW . The SSS generators tend to yield a Higgs mass peak ∼ 125 –127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to Δ EW in a more standard notation. Models of natural supersymmetry give rise to a weak scale $$m_{weak}\sim m_{W,Z,h}\sim 100$$ m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at $$m_h\sim 125$$ m h ∼ 125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure $$\Delta _{EW}$$ Δ EW . The SSS generators tend to yield a Higgs mass peak $$\sim 125$$ ∼ 125 –127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to $$\Delta _{EW}$$ Δ EW in a more standard notation. Models of natural supersymmetry give rise to a weak scale [Formula omitted] GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at [Formula omitted] GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure [Formula omitted]. The SSS generators tend to yield a Higgs mass peak [Formula omitted]-127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to [Formula omitted] in a more standard notation. Abstract Models of natural supersymmetry give rise to a weak scale $$m_{weak}\sim m_{W,Z,h}\sim 100$$ m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at $$m_h\sim 125$$ m h ∼ 125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure $$\Delta _{EW}$$ Δ EW . The SSS generators tend to yield a Higgs mass peak $$\sim 125$$ ∼ 125 –127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to $$\Delta _{EW}$$ Δ EW in a more standard notation. Models of natural supersymmetry give rise to a weak scale mweak ~ mW,Z,h ~ 100 GeV without any (implausible) finetuning of independent contributions to the weak scale. These models, which exhibit radiatively driven naturalness (RNS), are expected to arise from statistical analysis of the string landscape wherein large soft terms are favored, but subject to a not-too-large value of the derived weak scale in each pocket universe of the greater multiverse. The string landscape picture then predicts, using the Isajet SUSY spectra generator Isasugra, a statistical peak at mh ~ 125 GeV with sparticles generally beyond current LHC search limits. In this paper, we investigate how well these conclusions hold up using other popular spectra generators: SOFTSUSY, SPHENO and SUSPECT (SSS). We built a computer code DEW4SLHA which operates on SUSY Les Houches Accord files to calculate the associated electroweak naturalness measure ΔEW. The SSS generators tend to yield a Higgs mass peak ~125–127 GeV with a superparticle mass spectra rather similar to that generated by Isasugra. In an Appendix, we include loop corrections to ΔEW in a more standard notation.
ArticleNumber	172
Audience	Academic
Author	Baer, Howard Barger, Vernon Martinez, Dakotah
Author_xml	– sequence: 1 givenname: Howard surname: Baer fullname: Baer, Howard email: baer@ou.edu organization: Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Department of Physics, University of Wisconsin – sequence: 2 givenname: Vernon surname: Barger fullname: Barger, Vernon organization: Department of Physics, University of Wisconsin – sequence: 3 givenname: Dakotah surname: Martinez fullname: Martinez, Dakotah organization: Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma
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Cites_doi	10.1007/s12648-014-0504-8 10.1007/JHEP07(2015)15910.1007/JHEP07(2015)159 10.1016/S0010-4655(03)00222-4 10.1017/CBO9780511617270 10.1016/S0550-3213(96)00683-9 10.1140/epjst/e2020-000020-x 10.1103/PhysRevD.93.035016 10.1103/PhysRevResearch.1.033179 10.1103/PhysRevD.90.115007 10.1016/0370-2693(95)00961-J 10.1007/JHEP02(2021)143 10.1016/j.physletb.2010.03.032 10.1007/JHEP03(2018)00210.1007/JHEP03(2018)002 10.1103/PhysRevD.72.015003 10.1103/PhysRevD.96.035015 10.1016/S0550-3213(03)00173-1 10.1103/PhysRevD.88.095013 10.1103/PhysRevD.89.115019 10.1088/1126-6708/2005/07/065 10.1007/JHEP11(2011)031 10.1103/PhysRevD.52.1693 10.1016/0550-3213(88)90171-X 10.1146/annurev-nucl-102014-022053 10.1103/PhysRevD.102.075012 10.1140/epjc/s10052-021-09198-2 10.1007/JHEP10(2019)244 10.1103/PhysRevD.63.015011 10.1007/JHEP03(2012)103 10.1103/PhysRevLett.80.1822 10.1103/PhysRevD.66.015005 10.1103/PhysRevD.10.897 10.1103/PhysRevD.51.1046 10.1103/PhysRevLett.109.161802 10.1103/PhysRevD.57.5480 10.1142/9789812839657_0001 10.1088/1126-6708/2004/07/036 10.1016/j.cpc.2006.11.009 10.1142/S0217732386000105 10.1038/scientificamerican0514-34 10.1016/S0010-4655(01)00460-X 10.1088/1475-7516/2011/06/031 10.1007/JHEP09(2021)019 10.1103/PhysRevD.65.116003 10.1016/S0550-3213(02)01144-6 10.1007/JHEP01(2020)147 10.1007/JHEP09(2012)035 10.1016/j.cpc.2019.107099 10.1103/PhysRevD.87.115028 10.1142/9789812775344_0040 10.1103/PhysRevResearch.1.023001
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References	Martin (CR56) 2002; 65 Baer, Mustafayev, Tata (CR27) 2014; 90 CR39 Dimopoulos, Giudice (CR3) 1995; 357 Aad (CR5) 2021; 02 Baer, Barger, Sengupta (CR24) 2019; 1 Barbieri, Giudice (CR2) 1988; 306 Belanger, Kraml, Pukhov (CR46) 2005; 72 CR30 Bahl, Hahn, Heinemeyer, Hollik, Paßehr, Rzehak, Weiglein (CR35) 2020; 249 Djouadi, Kneur, Moultaka (CR32) 2007; 176 Martin (CR19) 1998; 18 Baer, Barger, Mickelson, Padeffke-Kirkland (CR14) 2014; 89 Skands (CR38) 2004; 07 Allanach (CR33) 2002; 143 Baer, Chen, Munroe, Paige, Tata (CR31) 1995; 51 van Beekveld, Caron, Ruiz de Austri (CR48) 2020; 01 CR7 Brust, Katz, Lawrence, Sundrum (CR21) 2012; 03 Baer, Lessa, Rajagopalan, Sreethawong (CR29) 2011; 06 Dine (CR9) 2015; 65 Lykken, Spiropulu (CR8) 2014; 310 CR45 CR41 CR40 Baer, Barger, Salam, Sengupta, Sinha (CR25) 2020; 229 Agrawal, Barr, Donoghue, Seckel (CR44) 1998; 80 Broeckel, Cicoli, Maharana, Singh, Sinha (CR42) 2020; 10 Agrawal, Barr, Donoghue, Seckel (CR43) 1998; 57 Baer, Tata (CR11) 2006 Gaillard, Lee (CR18) 1974; 10 Baer, Mustafayev, Profumo, Belyaev, Tata (CR50) 2005; 07 Mustafayev, Tata (CR13) 2014; 88 Slavich (CR37) 2021; 81 Baer, Barger, Salam, Sengupta (CR54) 2020; 102 van Beekveld, Beenakker, Caron, Peeters, Ruiz de Austri (CR47) 2017; 96 Baer, Barger, Huang, Mustafayev, Tata (CR15) 2012; 109 Baer, Balazs, Mercadante, Tata, Wang (CR23) 2001; 63 Baer, Barger, Huang (CR26) 2011; 11 CR10 Baer, Barger, Savoy (CR17) 2016; 93 Ellis, Enqvist, Nanopoulos, Zwirner (CR1) 1986; 1 CR52 Baer, Barger, Serce, Sinha (CR55) 2018; 03 Cassel, Ghilencea, Ross (CR53) 2010; 687 Ellis, Falk, Olive, Santoso (CR49) 2003; 652 Baer, Barger, Huang, Mickelson, Mustafayev, Tata (CR16) 2013; 87 Baer, Barger, Mickelson (CR12) 2013; 88 Sirunyan (CR6) 2019; 10 CR28 Porod (CR34) 2003; 153 Papucci, Ruderman, Weiler (CR22) 2012; 09 Pardo Vega, Villadoro (CR36) 2015; 07 Pierce, Bagger, Matchev, Zhang (CR51) 1997; 491 Dedes, Slavich (CR20) 2003; 657 Ibrahim, Nath (CR57) 2002; 66 Anderson, Castano (CR4) 1995; 52 P Slavich (10141_CR37) 2021; 81 H Baer (10141_CR14) 2014; 89 T Ibrahim (10141_CR57) 2002; 66 MK Gaillard (10141_CR18) 1974; 10 M van Beekveld (10141_CR48) 2020; 01 H Bahl (10141_CR35) 2020; 249 M van Beekveld (10141_CR47) 2017; 96 GW Anderson (10141_CR4) 1995; 52 A Dedes (10141_CR20) 2003; 657 H Baer (10141_CR24) 2019; 1 A Djouadi (10141_CR32) 2007; 176 H Baer (10141_CR55) 2018; 03 10141_CR52 10141_CR7 H Baer (10141_CR54) 2020; 102 10141_CR10 H Baer (10141_CR27) 2014; 90 H Baer (10141_CR31) 1995; 51 H Baer (10141_CR15) 2012; 109 H Baer (10141_CR25) 2020; 229 H Baer (10141_CR23) 2001; 63 PZ Skands (10141_CR38) 2004; 07 SP Martin (10141_CR56) 2002; 65 H Baer (10141_CR29) 2011; 06 SP Martin (10141_CR19) 1998; 18 10141_CR45 H Baer (10141_CR12) 2013; 88 H Baer (10141_CR17) 2016; 93 I Broeckel (10141_CR42) 2020; 10 DM Pierce (10141_CR51) 1997; 491 C Brust (10141_CR21) 2012; 03 R Barbieri (10141_CR2) 1988; 306 G Belanger (10141_CR46) 2005; 72 10141_CR40 10141_CR41 H Baer (10141_CR16) 2013; 87 AM Sirunyan (10141_CR6) 2019; 10 H Baer (10141_CR26) 2011; 11 G Aad (10141_CR5) 2021; 02 H Baer (10141_CR11) 2006 W Porod (10141_CR34) 2003; 153 S Cassel (10141_CR53) 2010; 687 A Mustafayev (10141_CR13) 2014; 88 J Pardo Vega (10141_CR36) 2015; 07 10141_CR39 BC Allanach (10141_CR33) 2002; 143 M Papucci (10141_CR22) 2012; 09 10141_CR30 JR Ellis (10141_CR49) 2003; 652 JR Ellis (10141_CR1) 1986; 1 S Dimopoulos (10141_CR3) 1995; 357 V Agrawal (10141_CR44) 1998; 80 J Lykken (10141_CR8) 2014; 310 H Baer (10141_CR50) 2005; 07 10141_CR28 V Agrawal (10141_CR43) 1998; 57 M Dine (10141_CR9) 2015; 65
References_xml	– ident: CR45 – volume: 88 start-page: 991 year: 2014 end-page: 1004 ident: CR13 article-title: Supersymmetry, naturalness, and light higgsinos publication-title: Indian J. Phys. doi: 10.1007/s12648-014-0504-8 – volume: 07 start-page: 159 year: 2015 ident: CR36 article-title: SusyHD: Higgs mass Determination in Supersymmetry publication-title: JHEP doi: 10.1007/JHEP07(2015)15910.1007/JHEP07(2015)159 – volume: 153 start-page: 275 year: 2003 end-page: 315 ident: CR34 article-title: SPheno, a program for calculating supersymmetric spectra, SUSY particle decays and SUSY particle production at e+ e- colliders publication-title: Comput. Phys. Commun. doi: 10.1016/S0010-4655(03)00222-4 – ident: CR39 – year: 2006 ident: CR11 publication-title: Weak scale supersymmetry: from superfields to scattering events doi: 10.1017/CBO9780511617270 – volume: 491 start-page: 3 year: 1997 end-page: 67 ident: CR51 article-title: Precision corrections in the minimal supersymmetric standard model publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(96)00683-9 – volume: 229 start-page: 3085 issue: 21 year: 2020 end-page: 3141 ident: CR25 article-title: Status of weak scale supersymmetry after LHC Run 2 and ton-scale noble liquid WIMP searches publication-title: Eur. Phys. J. ST doi: 10.1140/epjst/e2020-000020-x – volume: 93 start-page: 035016 issue: 3 year: 2016 ident: CR17 article-title: Upper bounds on sparticle masses from naturalness or how to disprove weak scale supersymmetry publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.93.035016 – volume: 1 start-page: 033179 issue: 3 year: 2019 ident: CR24 article-title: Landscape solution to the SUSY flavor and CP problems publication-title: Phys. Rev. Res. doi: 10.1103/PhysRevResearch.1.033179 – volume: 90 start-page: 115007 issue: 11 year: 2014 ident: CR27 article-title: Monojet plus soft dilepton signal from light higgsino pair production at LHC14 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.90.115007 – volume: 357 start-page: 573 year: 1995 end-page: 578 ident: CR3 article-title: Naturalness constraints in supersymmetric theories with nonuniversal soft terms publication-title: Phys. Lett. B doi: 10.1016/0370-2693(95)00961-J – volume: 02 start-page: 143 year: 2021 ident: CR5 article-title: Search for squarks and gluinos in final states with jets and missing transverse momentum using 139 fb of =13 TeV collision data with the ATLAS detector publication-title: JHEP doi: 10.1007/JHEP02(2021)143 – volume: 687 start-page: 214 year: 2010 end-page: 218 ident: CR53 article-title: Testing SUSY publication-title: Phys. Lett. B doi: 10.1016/j.physletb.2010.03.032 – volume: 03 start-page: 002 year: 2018 ident: CR55 article-title: Higgs and superparticle mass predictions from the landscape publication-title: JHEP doi: 10.1007/JHEP03(2018)00210.1007/JHEP03(2018)002 – volume: 72 start-page: 015003 year: 2005 ident: CR46 article-title: Comparison of SUSY spectrum calculations and impact on the relic density constraints from WMAP publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.72.015003 – volume: 96 start-page: 035015 issue: 3 year: 2017 ident: CR47 article-title: Supersymmetry with Dark Matter is still natural publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.96.035015 – volume: 657 start-page: 333 year: 2003 end-page: 354 ident: CR20 article-title: Two loop corrections to radiative electroweak symmetry breaking in the MSSM publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(03)00173-1 – volume: 88 start-page: 095013 issue: 9 year: 2013 ident: CR12 article-title: How conventional measures overestimate electroweak fine-tuning in supersymmetric theory publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.88.095013 – volume: 89 start-page: 115019 issue: 11 year: 2014 ident: CR14 article-title: SUSY models under siege: LHC constraints and electroweak fine-tuning publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.89.115019 – volume: 07 start-page: 065 year: 2005 ident: CR50 article-title: Direct, indirect and collider detection of neutralino dark matter in SUSY models with non-universal Higgs masses publication-title: JHEP doi: 10.1088/1126-6708/2005/07/065 – volume: 11 start-page: 031 year: 2011 ident: CR26 article-title: Hidden SUSY at the LHC: the light higgsino-world scenario and the role of a lepton collider publication-title: JHEP doi: 10.1007/JHEP11(2011)031 – volume: 52 start-page: 1693 year: 1995 end-page: 1700 ident: CR4 article-title: Naturalness and superpartner masses or when to give up on weak scale supersymmetry publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.52.1693 – volume: 306 start-page: 63 year: 1988 end-page: 76 ident: CR2 article-title: Upper bounds on supersymmetric particle masses publication-title: Nucl. Phys. B doi: 10.1016/0550-3213(88)90171-X – volume: 65 start-page: 43 year: 2015 end-page: 62 ident: CR9 article-title: Naturalness under stress publication-title: Ann. Rev. Nucl. Part. Sci. doi: 10.1146/annurev-nucl-102014-022053 – volume: 102 start-page: 075012 issue: 7 year: 2020 ident: CR54 article-title: String landscape guide to soft SUSY breaking terms publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.102.075012 – volume: 81 start-page: 450 issue: 5 year: 2021 ident: CR37 article-title: Higgs-mass predictions in the MSSM and beyond publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-021-09198-2 – volume: 10 start-page: 244 year: 2019 ident: CR6 article-title: Search for supersymmetry in proton-proton collisions at 13 TeV in final states with jets and missing transverse momentum publication-title: JHEP doi: 10.1007/JHEP10(2019)244 – volume: 63 start-page: 015011 year: 2001 ident: CR23 article-title: Viable supersymmetric models with an inverted scalar mass hierarchy at the GUT scale publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.63.015011 – volume: 03 start-page: 103 year: 2012 ident: CR21 article-title: SUSY, the Third Generation and the LHC publication-title: JHEP doi: 10.1007/JHEP03(2012)103 – ident: CR30 – volume: 80 start-page: 1822 year: 1998 end-page: 1825 ident: CR44 article-title: Anthropic considerations in multiple domain theories and the scale of electroweak symmetry breaking publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.80.1822 – ident: CR10 – volume: 66 start-page: 015005 year: 2002 ident: CR57 article-title: Neutralino exchange corrections to the Higgs boson mixings with explicit CP violation publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.66.015005 – volume: 10 start-page: 897 year: 1974 ident: CR18 article-title: Rare decay modes of the K-mesons in gauge theories publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.10.897 – volume: 51 start-page: 1046 year: 1995 end-page: 1050 ident: CR31 article-title: Multichannel search for minimal supergravity at and colliders publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.51.1046 – volume: 109 start-page: 161802 year: 2012 ident: CR15 article-title: Radiative natural SUSY with a 125 GeV Higgs boson publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.109.161802 – volume: 57 start-page: 5480 year: 1998 end-page: 5492 ident: CR43 article-title: Viable range of the mass scale of the standard model publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.57.5480 – ident: CR40 – volume: 18 start-page: 1 year: 1998 end-page: 98 ident: CR19 article-title: A supersymmetry primer publication-title: Adv. Ser. Direct. High Energy Phys. doi: 10.1142/9789812839657_0001 – volume: 07 start-page: 036 year: 2004 ident: CR38 article-title: SUSY Les Houches accord: interfacing SUSY spectrum calculators, decay packages, and event generators publication-title: JHEP doi: 10.1088/1126-6708/2004/07/036 – volume: 176 start-page: 426 year: 2007 end-page: 455 ident: CR32 article-title: SuSpect: A Fortran code for the supersymmetric and Higgs particle spectrum in the MSSM publication-title: Comput. Phys. Commun. doi: 10.1016/j.cpc.2006.11.009 – ident: CR52 – volume: 1 start-page: 57 year: 1986 ident: CR1 article-title: Observables in low-energy superstring models publication-title: Mod. Phys. Lett. A doi: 10.1142/S0217732386000105 – volume: 310 start-page: 36 issue: 5 year: 2014 end-page: 39 ident: CR8 article-title: Supersymmetry and the crisis in physics publication-title: Sci. Am. doi: 10.1038/scientificamerican0514-34 – volume: 143 start-page: 305 year: 2002 end-page: 331 ident: CR33 article-title: SOFTSUSY: a program for calculating supersymmetric spectra publication-title: Comput. Phys. Commun. doi: 10.1016/S0010-4655(01)00460-X – volume: 06 start-page: 031 year: 2011 ident: CR29 article-title: Mixed axion/neutralino cold dark matter in supersymmetric models publication-title: JCAP doi: 10.1088/1475-7516/2011/06/031 – volume: 10 start-page: 015 year: 2020 ident: CR42 article-title: Moduli stabilisation and the statistics of SUSY breaking in the landscape publication-title: JHEP doi: 10.1007/JHEP09(2021)019 – ident: CR7 – volume: 65 start-page: 116003 year: 2002 ident: CR56 article-title: Two loop effective potential for a general renormalizable theory and softly broken supersymmetry publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.65.116003 – ident: CR28 – ident: CR41 – volume: 652 start-page: 259 year: 2003 end-page: 347 ident: CR49 article-title: Exploration of the MSSM with nonuniversal Higgs masses publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(02)01144-6 – volume: 01 start-page: 147 year: 2020 ident: CR48 article-title: The current status of fine-tuning in supersymmetry publication-title: JHEP doi: 10.1007/JHEP01(2020)147 – volume: 09 start-page: 035 year: 2012 ident: CR22 article-title: Natural SUSY Endures publication-title: JHEP doi: 10.1007/JHEP09(2012)035 – volume: 249 start-page: 107099 year: 2020 ident: CR35 article-title: Precision calculations in the MSSM Higgs-boson sector with FeynHiggs 2.14 publication-title: Comput. Phys. Commun. doi: 10.1016/j.cpc.2019.107099 – volume: 87 start-page: 115028 issue: 11 year: 2013 ident: CR16 article-title: Radiative natural supersymmetry: reconciling electroweak fine-tuning and the Higgs boson mass publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.87.115028 – volume: 63 start-page: 015011 year: 2001 ident: 10141_CR23 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.63.015011 – volume: 229 start-page: 3085 issue: 21 year: 2020 ident: 10141_CR25 publication-title: Eur. Phys. J. ST doi: 10.1140/epjst/e2020-000020-x – volume-title: Weak scale supersymmetry: from superfields to scattering events year: 2006 ident: 10141_CR11 doi: 10.1017/CBO9780511617270 – volume: 81 start-page: 450 issue: 5 year: 2021 ident: 10141_CR37 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-021-09198-2 – volume: 10 start-page: 897 year: 1974 ident: 10141_CR18 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.10.897 – volume: 02 start-page: 143 year: 2021 ident: 10141_CR5 publication-title: JHEP doi: 10.1007/JHEP02(2021)143 – volume: 10 start-page: 015 year: 2020 ident: 10141_CR42 publication-title: JHEP doi: 10.1007/JHEP09(2021)019 – volume: 51 start-page: 1046 year: 1995 ident: 10141_CR31 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.51.1046 – volume: 03 start-page: 002 year: 2018 ident: 10141_CR55 publication-title: JHEP doi: 10.1007/JHEP03(2018)00210.1007/JHEP03(2018)002 – volume: 657 start-page: 333 year: 2003 ident: 10141_CR20 publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(03)00173-1 – volume: 1 start-page: 57 year: 1986 ident: 10141_CR1 publication-title: Mod. Phys. Lett. A doi: 10.1142/S0217732386000105 – volume: 06 start-page: 031 year: 2011 ident: 10141_CR29 publication-title: JCAP doi: 10.1088/1475-7516/2011/06/031 – volume: 310 start-page: 36 issue: 5 year: 2014 ident: 10141_CR8 publication-title: Sci. Am. doi: 10.1038/scientificamerican0514-34 – volume: 109 start-page: 161802 year: 2012 ident: 10141_CR15 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.109.161802 – volume: 72 start-page: 015003 year: 2005 ident: 10141_CR46 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.72.015003 – volume: 07 start-page: 159 year: 2015 ident: 10141_CR36 publication-title: JHEP doi: 10.1007/JHEP07(2015)15910.1007/JHEP07(2015)159 – volume: 65 start-page: 43 year: 2015 ident: 10141_CR9 publication-title: Ann. Rev. Nucl. Part. Sci. doi: 10.1146/annurev-nucl-102014-022053 – ident: 10141_CR10 – volume: 65 start-page: 116003 year: 2002 ident: 10141_CR56 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.65.116003 – volume: 01 start-page: 147 year: 2020 ident: 10141_CR48 publication-title: JHEP doi: 10.1007/JHEP01(2020)147 – volume: 652 start-page: 259 year: 2003 ident: 10141_CR49 publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(02)01144-6 – ident: 10141_CR28 – volume: 57 start-page: 5480 year: 1998 ident: 10141_CR43 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.57.5480 – volume: 249 start-page: 107099 year: 2020 ident: 10141_CR35 publication-title: Comput. Phys. Commun. doi: 10.1016/j.cpc.2019.107099 – volume: 88 start-page: 095013 issue: 9 year: 2013 ident: 10141_CR12 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.88.095013 – volume: 153 start-page: 275 year: 2003 ident: 10141_CR34 publication-title: Comput. Phys. Commun. doi: 10.1016/S0010-4655(03)00222-4 – volume: 102 start-page: 075012 issue: 7 year: 2020 ident: 10141_CR54 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.102.075012 – ident: 10141_CR30 – volume: 11 start-page: 031 year: 2011 ident: 10141_CR26 publication-title: JHEP doi: 10.1007/JHEP11(2011)031 – volume: 143 start-page: 305 year: 2002 ident: 10141_CR33 publication-title: Comput. Phys. Commun. doi: 10.1016/S0010-4655(01)00460-X – volume: 306 start-page: 63 year: 1988 ident: 10141_CR2 publication-title: Nucl. Phys. B doi: 10.1016/0550-3213(88)90171-X – volume: 1 start-page: 033179 issue: 3 year: 2019 ident: 10141_CR24 publication-title: Phys. Rev. Res. doi: 10.1103/PhysRevResearch.1.033179 – volume: 176 start-page: 426 year: 2007 ident: 10141_CR32 publication-title: Comput. Phys. Commun. doi: 10.1016/j.cpc.2006.11.009 – volume: 10 start-page: 244 year: 2019 ident: 10141_CR6 publication-title: JHEP doi: 10.1007/JHEP10(2019)244 – volume: 88 start-page: 991 year: 2014 ident: 10141_CR13 publication-title: Indian J. Phys. doi: 10.1007/s12648-014-0504-8 – ident: 10141_CR7 – ident: 10141_CR41 – volume: 96 start-page: 035015 issue: 3 year: 2017 ident: 10141_CR47 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.96.035015 – volume: 52 start-page: 1693 year: 1995 ident: 10141_CR4 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.52.1693 – volume: 89 start-page: 115019 issue: 11 year: 2014 ident: 10141_CR14 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.89.115019 – volume: 07 start-page: 065 year: 2005 ident: 10141_CR50 publication-title: JHEP doi: 10.1088/1126-6708/2005/07/065 – ident: 10141_CR45 – ident: 10141_CR40 doi: 10.1142/9789812775344_0040 – volume: 66 start-page: 015005 year: 2002 ident: 10141_CR57 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.66.015005 – ident: 10141_CR39 – volume: 357 start-page: 573 year: 1995 ident: 10141_CR3 publication-title: Phys. Lett. B doi: 10.1016/0370-2693(95)00961-J – ident: 10141_CR52 doi: 10.1103/PhysRevResearch.1.023001 – volume: 18 start-page: 1 year: 1998 ident: 10141_CR19 publication-title: Adv. Ser. Direct. High Energy Phys. doi: 10.1142/9789812839657_0001 – volume: 93 start-page: 035016 issue: 3 year: 2016 ident: 10141_CR17 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.93.035016 – volume: 491 start-page: 3 year: 1997 ident: 10141_CR51 publication-title: Nucl. Phys. B doi: 10.1016/S0550-3213(96)00683-9 – volume: 03 start-page: 103 year: 2012 ident: 10141_CR21 publication-title: JHEP doi: 10.1007/JHEP03(2012)103 – volume: 687 start-page: 214 year: 2010 ident: 10141_CR53 publication-title: Phys. Lett. B doi: 10.1016/j.physletb.2010.03.032 – volume: 90 start-page: 115007 issue: 11 year: 2014 ident: 10141_CR27 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.90.115007 – volume: 87 start-page: 115028 issue: 11 year: 2013 ident: 10141_CR16 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.87.115028 – volume: 80 start-page: 1822 year: 1998 ident: 10141_CR44 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.80.1822 – volume: 07 start-page: 036 year: 2004 ident: 10141_CR38 publication-title: JHEP doi: 10.1088/1126-6708/2004/07/036 – volume: 09 start-page: 035 year: 2012 ident: 10141_CR22 publication-title: JHEP doi: 10.1007/JHEP09(2012)035
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Snippet	Models of natural supersymmetry give rise to a weak scale m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible) finetuning of independent contributions to... Models of natural supersymmetry give rise to a weak scale $$m_{weak}\sim m_{W,Z,h}\sim 100$$ m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible)... Models of natural supersymmetry give rise to a weak scale [Formula omitted] GeV without any (implausible) finetuning of independent contributions to the weak... Models of natural supersymmetry give rise to a weak scale mweak∼mW,Z,h∼100 GeV without any (implausible) finetuning of independent contributions to the weak... Models of natural supersymmetry give rise to a weak scale mweak ~ mW,Z,h ~ 100 GeV without any (implausible) finetuning of independent contributions to the... Abstract Models of natural supersymmetry give rise to a weak scale $$m_{weak}\sim m_{W,Z,h}\sim 100$$ m weak ∼ m W , Z , h ∼ 100 GeV without any (implausible)...
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SubjectTerms	Astronomy Astrophysics and Cosmology Building codes Cosmology Elementary Particles Generators Hadrons Heavy Ions Large Hadron Collider LHC Mass spectra Measurement Science and Instrumentation Nuclear Energy Nuclear Physics Physics Physics and Astronomy PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics Statistical analysis string phenomenology String Theory Strings Supersymmetry
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Title	Comparison of SUSY spectra generators for natural SUSY and string landscape predictions
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