FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3122167721> ?p ?o ?g. }

• W3122167721 abstract "We describe a likelihood analysis using MasterCode of variants of the MSSM in which the soft supersymmetry-breaking parameters are assumed to have universal values at some scale $M_{in}$ below the supersymmetric grand unification scale $M_{GUT}$, as can occur in mirage mediation and other models. In addition to $M_{in}$, such `sub-GUT' models have the 4 parameters of the CMSSM, namely a common gaugino mass $m_{1/2}$, a common soft supersymmetry-breaking scalar mass $m_0$, a common trilinear mixing parameter $A$ and the ratio of MSSM Higgs vevs $tanbeta$, assuming that the Higgs mixing parameter $mu > 0$. We take into account constraints on strongly- and electroweakly-interacting sparticles from $sim 36$/fb of LHC data at 13 TeV and the LUX and 2017 PICO, XENON1T and PandaX-II searches for dark matter scattering, in addition to the previous LHC and dark matter constraints as well as full sets of flavour and electroweak constraints. We find a preference for $M_{in} sim 10^5$ to $10^9$ GeV, with $M_{in} sim M_{GUT}$ disfavoured by $Delta chi^2 sim 3$ due to the ${rm BR}(B_{s, d} to mu^+mu^-)$ constraint. The lower limits on strongly-interacting sparticles are largely determined by LHC searches, and similar to those in the CMSSM. We find a preference for the LSP to be a Bino or Higgsino with $tilde{chi^0_1} sim 1$ TeV, with annihilation via heavy Higgs bosons $H/A$ and stop coannihilation, or chargino coannihilation, bringing the cold dark matter density into the cosmological range. We find that spin-independent dark matter scattering is likely to be within reach of the planned LUX-Zeplin and XENONnT experiments. We probe the impact of the $(g-2)_mu$ constraint, finding similar results whether or not it is included." @default.
• W3122167721 created "2021-02-01" @default.
• W3122167721 creator A5000651436 @default.
• W3122167721 creator A5023397872 @default.
• W3122167721 creator A5023676891 @default.
• W3122167721 creator A5030565352 @default.
• W3122167721 creator A5041396090 @default.
• W3122167721 creator A5041940470 @default.
• W3122167721 creator A5042459968 @default.
• W3122167721 creator A5048133271 @default.
• W3122167721 creator A5051674176 @default.
• W3122167721 creator A5052011846 @default.
• W3122167721 creator A5054531499 @default.
• W3122167721 creator A5065780744 @default.
• W3122167721 creator A5067997629 @default.
• W3122167721 creator A5071010702 @default.
• W3122167721 creator A5075475814 @default.
• W3122167721 creator A5083801345 @default.
• W3122167721 date "2018-02-01" @default.
• W3122167721 modified "2023-10-15" @default.
• W3122167721 title "Likelihood analysis of the sub-GUT MSSM in light of LHC 13-TeV data" @default.
• W3122167721 cites W1512962526 @default.
• W3122167721 cites W1541829547 @default.
• W3122167721 cites W1556797928 @default.
• W3122167721 cites W1590128522 @default.
• W3122167721 cites W1656143837 @default.
• W3122167721 cites W1839094326 @default.
• W3122167721 cites W1884712174 @default.
• W3122167721 cites W1922727670 @default.
• W3122167721 cites W1941812509 @default.
• W3122167721 cites W1957266799 @default.
• W3122167721 cites W1960751468 @default.
• W3122167721 cites W1961848711 @default.
• W3122167721 cites W1967250627 @default.
• W3122167721 cites W1967625111 @default.
• W3122167721 cites W1972268321 @default.
• W3122167721 cites W1972919610 @default.
• W3122167721 cites W1980573344 @default.
• W3122167721 cites W1984532828 @default.
• W3122167721 cites W1999799307 @default.
• W3122167721 cites W2003399426 @default.
• W3122167721 cites W2007169356 @default.
• W3122167721 cites W2008813150 @default.
• W3122167721 cites W2010530001 @default.
• W3122167721 cites W2011301426 @default.
• W3122167721 cites W2012454313 @default.
• W3122167721 cites W2013416637 @default.
• W3122167721 cites W2018645261 @default.
• W3122167721 cites W2020091822 @default.
• W3122167721 cites W2020943201 @default.
• W3122167721 cites W2020980567 @default.
• W3122167721 cites W2025930417 @default.
• W3122167721 cites W2026528542 @default.
• W3122167721 cites W2028160016 @default.
• W3122167721 cites W2030525277 @default.
• W3122167721 cites W2031915452 @default.
• W3122167721 cites W2033542670 @default.
• W3122167721 cites W2038186329 @default.
• W3122167721 cites W2043371852 @default.
• W3122167721 cites W2047383019 @default.
• W3122167721 cites W2047395855 @default.
• W3122167721 cites W204794554 @default.
• W3122167721 cites W2049755489 @default.
• W3122167721 cites W2051449768 @default.
• W3122167721 cites W2053118669 @default.
• W3122167721 cites W2060851574 @default.
• W3122167721 cites W2066436412 @default.
• W3122167721 cites W2073872321 @default.
• W3122167721 cites W2077767449 @default.
• W3122167721 cites W2078728780 @default.
• W3122167721 cites W2079838815 @default.
• W3122167721 cites W2084792108 @default.
• W3122167721 cites W2088243315 @default.
• W3122167721 cites W2091605720 @default.
• W3122167721 cites W2097455027 @default.
• W3122167721 cites W2099745646 @default.
• W3122167721 cites W2100521738 @default.
• W3122167721 cites W2101631969 @default.
• W3122167721 cites W2110743846 @default.
• W3122167721 cites W2114510786 @default.
• W3122167721 cites W2114987342 @default.
• W3122167721 cites W2116109970 @default.
• W3122167721 cites W2118124641 @default.
• W3122167721 cites W2118490223 @default.
• W3122167721 cites W2118663551 @default.
• W3122167721 cites W2121304041 @default.
• W3122167721 cites W2123576665 @default.
• W3122167721 cites W2125835296 @default.
• W3122167721 cites W2126330345 @default.
• W3122167721 cites W2127669635 @default.
• W3122167721 cites W2130336961 @default.
• W3122167721 cites W2131715088 @default.
• W3122167721 cites W2132803409 @default.
• W3122167721 cites W2133742651 @default.
• W3122167721 cites W2137515269 @default.
• W3122167721 cites W2137619955 @default.
• W3122167721 cites W2140052424 @default.
• W3122167721 cites W2142882397 @default.
• W3122167721 cites W2147150488 @default.
• W3122167721 cites W2160246790 @default.

• next