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Split supersymmetry - Wikipedia, the free encyclopedia

Split supersymmetry

From Wikipedia, the free encyclopedia

In particle physics, split supersymmetry is a recent proposal for new physics beyond the Standard Model. It was proposed separately in three papers. The first by James Wells in June 2003 in a more modest form that mildly relaxed the assumption about naturalness in the Higgs potential. In May 2004 Nima Arkani-Hamed and Savas Dimopoulos argued that naturalness in the Higgs sector may not be an accurate guide to propose new physics beyond the Standard Model and argued that supersymmetry may be realized in a different fashion that preserved gauge coupling unification and has a dark matter candidate. In June 2004 Gian Giudice and Andrea Romanino argued from a general point of view that if one wants gauge coupling unification and a dark matter candidate, that split supersymmetry is one amongst a few theories that exists. Split supersymmetry remains controversial because it is not designed to solve the hierarchy problem which has been the primary motivation for proposals for new physics beyond the Standard Model since 1979.

The new light (~TeV) particles in Split Supersymmetry (beyond the Standard Models particles) are

Field Spin Gauge Charges Name
\tilde{g} \frac{1}{2} (8,1)0 gluino
\tilde{W} \frac{1}{2} (1,3)0 wino
\tilde{B} \frac{1}{2} (1,1)0 bino
\tilde{H}_u \frac{1}{2} (1,2)_{\frac{1}{2}} higgsino
\tilde{H}_d \frac{1}{2} (1,2)_{-\frac{1}{2}} higgsino

The Lagrangian for Split Supersymmetry is constrained from the existence of high energy supersymmetry. There are five couplings in Split Supersymmetry: the Higgs quartic coupling and four Yukawa couplings between the Higgsinos, Higgs and gauginos. The couplings are set by one parameter, tanĪ², at the scale where the supersymmetric scalars decouple. Beneath the supersymmetry breaking scale, these five couplings evolve through the renormalization group equation down to the TeV scale. At a future Linear collider, these couplings could be measured at the 1% level and then renormalization group evolved up to high energies to show that the theory is supersymmetric at an exceedingly high scale.

[edit] Long Lived Gluinos

The striking feature of split supersymmetry is that the gluino becomes a quasi-stable particle with a lifetime that could be upto 100 seconds long. A gluino that lived longer than this would disrupt Big Bang nucleosynthesis or would have been observed as an additional source of cosmic gamma rays. The gluino is long lived because it can only decay into a squark and a quark and because the squarks are so heavy and these decays are highly suppressed.

The potentially long lifetime of the gluino leads to different collider signatures at the Tevatron and LHC. There are three ways to see these particles

  • Measuring the ratio of momentum to energy or velocity in tracking chambers ( dE/dx in the inner tracking chamber or p/v in the outer muon tracking chamber)
  • Looking for excess singlet jet events that arise from initial or final state radiation.
  • Looking for gluinos that have come to rest inside the detector and later decay.

[edit] History

The initial attitute of some of the high energy physics community towards split supersymmetry was illustrated by a parody called supersplit supersymmetry. Often when a new notion in physics is proposed there is a knee-jerk backlash. When naturalness in the Higgs sector was initially proposed as a motivation for new physics, the notion was not taken seriously. After the supersymmetric Standard Model was proposed, Sheldon Glashow quipped that 'half of the particles have already been discovered.' After 25 years, the notion of naturalness had become so ingrained in the community that proposing a theory that did not use naturalness as the primary motivation was ridiculed. Split supersymmetry makes predictions that are distinct from both the Standard Model and the Minimal Supersymmetric Standard Model and the ultimate nature of the naturalness in the Higgs sector will be determined at future colliders.

Many of the original proponents of naturalness no longer believe that it should be an exclusive constraint on new physics. Kenneth Wilson originally advocated for it, but has recently called it one of his biggest mistakes during his career. Steven Weinberg relaxed the notion of naturalness in the cosmological constant and argued for an environmental explanation for it in 1987. Leonard Susskind, who initially proposed technicolor, is a firm advocate of the notion of a landscape and non-naturalness. Savas Dimopoulos, who initially proposed the supersymmetric Standard Model, proposed split supersymmetry.

[edit] External links


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