Supersymmetry
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Supersymmetry

In particle physics, supersymmetry (SUSY) is a conjectured relationship between two basic classes of elementary particles: bosons, which have an integer-valued spin, and fermions, which have a half-integer spin.[1][2] A type of spacetime symmetry, supersymmetry is a possible candidate for undiscovered particle physics, and seen by some physicists as an elegant solution to many current problems in particle physics if confirmed correct, which could resolve various areas where current theories are believed to be incomplete. A supersymmetrical extension to the Standard Model could resolve major hierarchy problems within gauge theory, by guaranteeing that quadratic divergences of all orders will cancel out in perturbation theory.

In supersymmetry, each particle from one group would have an associated particle in the other, known as its superpartner, the spin of which differs by a half-integer. These superpartners would be new and undiscovered particles; for example, there would be a particle called a "selectron" (superpartner electron), a bosonic partner of the electron. In the simplest supersymmetry theories, with perfectly "unbroken" supersymmetry, each pair of superpartners would share the same mass and internal quantum numbers besides spin. Since we expect to find these "superpartners" using present-day equipment, if supersymmetry exists then it consists of a spontaneously broken symmetry, allowing superpartners to differ in mass.[3][4][5] Spontaneously broken supersymmetry could solve many problems in particle physics, including the hierarchy problem.

There is no experimental evidence that supersymmetry is correct, or whether or not other extensions to current models might be more accurate. It is only since around 2010 that particle accelerators specifically designed to study physics beyond the Standard Model have become operational (i.e. the LHC), and it is not known where exactly to look, nor the energies required for a successful search.

The main reasons for supersymmetry being supported by some physicists is that the current theories are known to be incomplete and their limitations are well established, and supersymmetry could be an attractive solution to some of the major concerns.[6][7]

## Motivations

Direct confirmation would entail production of superpartners in collider experiments, such as the Large Hadron Collider (LHC). The first runs of the LHC found no previously-unknown particles other than the Higgs boson which was already suspected to exist as part of the Standard Model, and therefore no evidence for supersymmetry.[6][7]

Indirect methods include the search for a permanent electric dipole moment (EDM) in the known Standard Model particles, which can arise when the Standard Model particle interacts with the supersymmetric particles. The current best constraint on the electron electric dipole moment put it to be smaller than 10-28 e·cm, equivalent to a sensitivity to new physics at the TeV scale and matching that of the current best particle colliders.[8] A permanent EDM in any fundamental particle points towards time-reversal violating physics, and therefore also CP-symmetry violation via the CPT theorem. Such EDM experiments are also much more scalable than conventional particle accelerators and offer a practical alternative to detecting physics beyond the standard model as accelerator experiments become increasingly costly and complicated to maintain.

These findings disappointed many physicists, who believed that supersymmetry (and other theories relying upon it) were by far the most promising theories for "new" physics, and had hoped for signs of unexpected results from these runs.[9][10] Former enthusiastic supporter Mikhail Shifman went as far as urging the theoretical community to search for new ideas and accept that supersymmetry was a failed theory.[11] This opinion is not universally accepted with some researchers suggesting that this "naturalness" crisis was premature because various calculations were too optimistic about the limits of masses which would allow a supersymmetry based solution.[12][13]

To reconcile the lack of experimental evidence for SUSY, some researchers suggest that the string theory landscape could have a power law statistical pull on soft SUSY breaking terms to large values (depending on the number of hidden sector SUSY breaking fields contributing to the soft terms).[14] If this is coupled with an anthropic requirement that contributions to the weak scale not exceed a factor between 2 and 5 from its measured value (as argued by Agrawal et al.[15]), then the Higgs mass is pulled up to the vicinity of 125 GeV while most sparticles are pulled to values beyond the current reach of LHC.[16] An exception occurs for higgsinos which gain mass not from SUSY breaking but rather from whatever mechanism solves the SUSY mu problem. Light higgsino pair production in association with hard initial state jet radiation leads to a soft opposite-sign dilepton plus jet plus missing transverse energy signal.[17] Such an excess seems to be appearing in current Atlas data with 139 fb-1 of integrated luminosity.[18]

## Prospective benefits

There are numerous phenomenological motivations for supersymmetry close to the electroweak scale, as well as technical motivations for supersymmetry at any scale.

### The hierarchy problem

Supersymmetry close to the electroweak scale solves the hierarchy problem that afflicts the Standard Model.[19] In the Standard Model, the electroweak scale receives enormous Planck-scale quantum corrections. The observed hierarchy between the electroweak scale and the Planck scale must be achieved with extraordinary fine tuning. In a supersymmetric theory, on the other hand, Planck-scale quantum corrections cancel between partners and superpartners (owing to a minus sign associated with fermionic loops). The hierarchy between the electroweak scale and the Planck scale is achieved in a natural manner, without extraordinary fine-tuning.

### Gauge coupling unification

The idea that the gauge symmetry groups unify at high-energy is called Grand unification theory. In the Standard Model, however, the weak, strong and electromagnetic couplings fail to unify at high energy. In a supersymmetry theory, the running of the gauge couplings are modified, and precise high-energy unification of the gauge couplings is achieved. The modified running also provides a natural mechanism for radiative electroweak symmetry breaking.

### Dark matter

TeV-scale supersymmetry (augmented with a discrete symmetry) typically provides a candidate dark matter particle at a mass scale consistent with thermal relic abundance calculations.[20][21]

### Other technical motivations

Supersymmetry is also motivated by solutions to several theoretical problems, for generally providing many desirable mathematical properties, and for ensuring sensible behavior at high energies. Supersymmetric quantum field theory is often much easier to analyze, as many more problems become mathematically tractable. When supersymmetry is imposed as a local symmetry, Einstein's theory of general relativity is included automatically, and the result is said to be a theory of supergravity. It is also a necessary feature of the most popular candidate for a theory of everything, superstring theory, and a SUSY theory could explain the issue of cosmological inflation.

Another theoretically appealing property of supersymmetry is that it offers the only "loophole" to the Coleman-Mandula theorem, which prohibits spacetime and internal symmetries from being combined in any nontrivial way, for quantum field theories like the Standard Model with very general assumptions. The Haag-?opusza?ski-Sohnius theorem demonstrates that supersymmetry is the only way spacetime and internal symmetries can be combined consistently.[22]

## History

A supersymmetry relating mesons and baryons was first proposed, in the context of hadronic physics, by Hironari Miyazawa in 1966. This supersymmetry did not involve spacetime, that is, it concerned internal symmetry, and was broken badly. Miyazawa's work was largely ignored at the time.[23][24][25][26]

J. L. Gervais and B. Sakita (in 1971),[27]Yu. A. Golfand and E. P. Likhtman (also in 1971), and D. V. Volkov and V. P. Akulov (1972),[28][full ] independently rediscovered supersymmetry in the context of quantum field theory, a radically new type of symmetry of spacetime and fundamental fields, which establishes a relationship between elementary particles of different quantum nature, bosons and fermions, and unifies spacetime and internal symmetries of microscopic phenomena. Supersymmetry with a consistent Lie-algebraic graded structure on which the Gervais-Sakita rediscovery was based directly first arose in 1971[29] in the context of an early version of string theory by Pierre Ramond, John H. Schwarz and André Neveu.

Finally, Julius Wess and Bruno Zumino (in 1974)[30] identified the characteristic renormalization features of four-dimensional supersymmetric field theories, which identified them as remarkable QFTs, and they and Abdus Salam and their fellow researchers introduced early particle physics applications. The mathematical structure of supersymmetry (graded Lie superalgebras) has subsequently been applied successfully to other topics of physics, ranging from nuclear physics,[31][32]critical phenomena,[33]quantum mechanics to statistical physics. It remains a vital part of many proposed theories of physics.

The first realistic supersymmetric version of the Standard Model was proposed in 1977 by Pierre Fayet and is known as the Minimal Supersymmetric Standard Model or MSSM for short. It was proposed to solve, amongst other things, the hierarchy problem.

## Applications

### Extension of possible symmetry groups

One reason that physicists explored supersymmetry is because it offers an extension to the more familiar symmetries of quantum field theory. These symmetries are grouped into the Poincaré group and internal symmetries and the Coleman-Mandula theorem showed that under certain assumptions, the symmetries of the S-matrix must be a direct product of the Poincaré group with a compact internal symmetry group or if there is not any mass gap, the conformal group with a compact internal symmetry group. In 1971 Golfand and Likhtman were the first to show that the Poincaré algebra can be extended through introduction of four anticommuting spinor generators (in four dimensions), which later became known as supercharges. In 1975, the Haag-?opusza?ski-Sohnius theorem analyzed all possible superalgebras in the general form, including those with an extended number of the supergenerators and central charges. This extended super-Poincaré algebra paved the way for obtaining a very large and important class of supersymmetric field theories.

#### The supersymmetry algebra

Traditional symmetries of physics are generated by objects that transform by the tensor representations of the Poincaré group and internal symmetries. Supersymmetries, however, are generated by objects that transform by the spin representations. According to the spin-statistics theorem, bosonic fields commute while fermionic fields anticommute. Combining the two kinds of fields into a single algebra requires the introduction of a Z2-grading under which the bosons are the even elements and the fermions are the odd elements. Such an algebra is called a Lie superalgebra.

The simplest supersymmetric extension of the Poincaré algebra is the Super-Poincaré algebra. Expressed in terms of two Weyl spinors, has the following anti-commutation relation:

${\displaystyle \{Q_{\alpha },{\bar {Q}}_{\dot {\beta }}\}=2(\sigma ^{\mu })_{\alpha {\dot {\beta }}}P_{\mu }}$

and all other anti-commutation relations between the Qs and commutation relations between the Qs and Ps vanish. In the above expression are the generators of translation and ?? are the Pauli matrices.

There are representations of a Lie superalgebra that are analogous to representations of a Lie algebra. Each Lie algebra has an associated Lie group and a Lie superalgebra can sometimes be extended into representations of a Lie supergroup.

### The Supersymmetric Standard Model

Incorporating supersymmetry into the Standard Model requires doubling the number of particles since there is no way that any of the particles in the Standard Model can be superpartners of each other. With the addition of new particles, there are many possible new interactions. The simplest possible supersymmetric model consistent with the Standard Model is the Minimal Supersymmetric Standard Model (MSSM) which can include the necessary additional new particles that are able to be superpartners of those in the Standard Model.

Cancellation of the Higgs boson quadratic mass renormalization between fermionic top quark loop and scalar stop squark tadpole Feynman diagrams in a supersymmetric extension of the Standard Model

One of the main motivations for SUSY comes from the quadratically divergent contributions to the Higgs mass squared. The quantum mechanical interactions of the Higgs boson causes a large renormalization of the Higgs mass and unless there is an accidental cancellation, the natural size of the Higgs mass is the greatest scale possible. This problem is known as the hierarchy problem. Supersymmetry reduces the size of the quantum corrections by having automatic cancellations between fermionic and bosonic Higgs interactions. If supersymmetry is restored at the weak scale, then the Higgs mass is related to supersymmetry breaking which can be induced from small non-perturbative effects explaining the vastly different scales in the weak interactions and gravitational interactions.

In many supersymmetric Standard Models there is a heavy stable particle (such as neutralino) which could serve as a weakly interacting massive particle (WIMP) dark matter candidate. The existence of a supersymmetric dark matter candidate is related closely to R-parity.

The standard paradigm for incorporating supersymmetry into a realistic theory is to have the underlying dynamics of the theory be supersymmetric, but the ground state of the theory does not respect the symmetry and supersymmetry is broken spontaneously. The supersymmetry break can not be done permanently by the particles of the MSSM as they currently appear. This means that there is a new sector of the theory that is responsible for the breaking. The only constraint on this new sector is that it must break supersymmetry permanently and must give superparticles TeV scale masses. There are many models that can do this and most of their details do not matter. In order to parameterize the relevant features of supersymmetry breaking, arbitrary soft SUSY breaking terms are added to the theory which temporarily break SUSY explicitly but could never arise from a complete theory of supersymmetry breaking.

#### Gauge-coupling unification

One piece of evidence for supersymmetry existing is gauge coupling unification. The renormalization group evolution of the three gauge coupling constants of the Standard Model is somewhat sensitive to the present particle content of the theory. These coupling constants do not quite meet together at a common energy scale if we run the renormalization group using the Standard Model.[34][35] After incorporating minimal SUSY, joint convergence of the coupling constants is projected at approximately 1016 GeV.[34]

### Supersymmetric quantum mechanics

Supersymmetric quantum mechanics adds the SUSY superalgebra to quantum mechanics as opposed to quantum field theory. Supersymmetric quantum mechanics often becomes relevant when studying the dynamics of supersymmetric solitons, and due to the simplified nature of having fields which are only functions of time (rather than space-time), a great deal of progress has been made in this subject and it is now studied in its own right.

SUSY quantum mechanics involves pairs of Hamiltonians which share a particular mathematical relationship, which are called partner Hamiltonians. (The potential energy terms which occur in the Hamiltonians are then known as partner potentials.) An introductory theorem shows that for every eigenstate of one Hamiltonian, its partner Hamiltonian has a corresponding eigenstate with the same energy. This fact can be exploited to deduce many properties of the eigenstate spectrum. It is analogous to the original description of SUSY, which referred to bosons and fermions. We can imagine a "bosonic Hamiltonian", whose eigenstates are the various bosons of our theory. The SUSY partner of this Hamiltonian would be "fermionic", and its eigenstates would be the theory's fermions. Each boson would have a fermionic partner of equal energy.

### Supersymmetry in condensed matter physics

SUSY concepts have provided useful extensions to the WKB approximation. Additionally, SUSY has been applied to disorder averaged systems both quantum and non-quantum (through statistical mechanics), the Fokker-Planck equation being an example of a non-quantum theory. The 'supersymmetry' in all these systems arises from the fact that one is modelling one particle and as such the 'statistics' do not matter. The use of the supersymmetry method provides a mathematical rigorous alternative to the replica trick, but only in non-interacting systems, which attempts to address the so-called 'problem of the denominator' under disorder averaging. For more on the applications of supersymmetry in condensed matter physics see Efetov (1997).[36]

### Supersymmetry in optics

Integrated optics was recently found[37] to provide a fertile ground on which certain ramifications of SUSY can be explored in readily-accessible laboratory settings. Making use of the analogous mathematical structure of the quantum-mechanical Schrödinger equation and the wave equation governing the evolution of light in one-dimensional settings, one may interpret the refractive index distribution of a structure as a potential landscape in which optical wave packets propagate. In this manner, a new class of functional optical structures with possible applications in phase matching, mode conversion[38] and space-division multiplexing becomes possible. SUSY transformations have been also proposed as a way to address inverse scattering problems in optics and as a one-dimensional transformation optics[39]

### Supersymmetry in dynamical systems

All stochastic (partial) differential equations, the models for all types of continuous time dynamical systems, possess topological supersymmetry.[40][41] In the operator representation of stochastic evolution, the topological supersymmetry is the exterior derivative which is commutative with the stochastic evolution operator defined as the stochastically averaged pullback induced on differential forms by SDE-defined diffeomorphisms of the phase space. The topological sector of the so-emerging supersymmetric theory of stochastic dynamics can be recognized as the Witten-type topological field theory.

The meaning of the topological supersymmetry in dynamical systems is the preservation of the phase space continuity--infinitely close points will remain close during continuous time evolution even in the presence of noise. When the topological supersymmetry is broken spontaneously, this property is violated in the limit of the infinitely long temporal evolution and the model can be said to exhibit (the stochastic generalization of) the butterfly effect. From a more general perspective, spontaneous breakdown of the topological supersymmetry is the theoretical essence of the ubiquitous dynamical phenomenon variously known as chaos, turbulence, self-organized criticality etc. The Goldstone theorem explains the associated emergence of the long-range dynamical behavior that manifests itself as noise, butterfly effect, and the scale-free statistics of sudden (instantonic) processes, such as earthquakes, neuroavalanches, and solar flares, known as the Zipf's law and the Richter scale.

### Supersymmetry in mathematics

SUSY is also sometimes studied mathematically for its intrinsic properties. This is because it describes complex fields satisfying a property known as holomorphy, which allows holomorphic quantities to be exactly computed. This makes supersymmetric models useful "toy models" of more realistic theories. A prime example of this has been the demonstration of S-duality in four-dimensional gauge theories[42] that interchanges particles and monopoles.

The proof of the Atiyah-Singer index theorem is much simplified by the use of supersymmetric quantum mechanics.

### Supersymmetry in quantum gravity

Supersymmetry is part of superstring theory, a string theory of quantum gravity, although it could in theory be a component of other quantum gravity theories as well, such as loop quantum gravity. For superstring theory to be consistent, supersymmetry seems to be required at some level (although it may be a strongly broken symmetry). If experimental evidence confirms supersymmetry in the form of supersymmetric particles such as the neutralino that is often believed to be the lightest superpartner, some people believe this would be a major boost to superstring theory. Since supersymmetry is a required component of superstring theory, any discovered supersymmetry would be consistent with superstring theory. If the Large Hadron Collider and other major particle physics experiments fail to detect supersymmetric partners, many versions of superstring theory which had predicted certain low mass superpartners to existing particles may need to be significantly revised.

## General supersymmetry

Supersymmetry appears in many related contexts of theoretical physics. It is possible to have multiple supersymmetries and also have supersymmetric extra dimensions.

### Extended supersymmetry

It is possible to have more than one kind of supersymmetry transformation. Theories with more than one supersymmetry transformation are known as extended supersymmetric theories. The more supersymmetry a theory has, the more constrained are the field content and interactions. Typically the number of copies of a supersymmetry is a power of 2 (1, 2, 4, 8...). In four dimensions, a spinor has four degrees of freedom and thus the minimal number of supersymmetry generators is four in four dimensions and having eight copies of supersymmetry means that there are 32 supersymmetry generators.

The maximal number of supersymmetry generators possible is 32. Theories with more than 32 supersymmetry generators automatically have massless fields with spin greater than 2. It is not known how to make massless fields with spin greater than two interact, so the maximal number of supersymmetry generators considered is 32. This is due to the Weinberg-Witten theorem. This corresponds to an N = 8 supersymmetry theory. Theories with 32 supersymmetries automatically have a graviton.

For four dimensions there are the following theories, with the corresponding multiplets[43] (CPT adds a copy, whenever they are not invariant under such symmetry):

 N = 1 N = 2 N = 4 N = 8 Chiral multiplet (0, ) Vector multiplet (, 1) Gravitino multiplet (1, ) Graviton multiplet (, 2) Hypermultiplet (-, 02, ) Vector multiplet (0, 2, 1) Supergravity multiplet (1, 2, 2) Vector multiplet (-1, - 4, 06, 4, 1) Supergravity multiplet (0, 4, 16, 4, 2) Supergravity multiplet (-2, - 8, -128, - 56, 070, 56, 128, 8, 2)

### Supersymmetry in alternate numbers of dimensions

It is possible to have supersymmetry in dimensions other than four. Because the properties of spinors change drastically between different dimensions, each dimension has its characteristic. In d dimensions, the size of spinors is approximately 2d/2 or 2(d - 1)/2. Since the maximum number of supersymmetries is 32, the greatest number of dimensions in which a supersymmetric theory can exist is eleven.[]

### Fractional supersymmetry

Fractional supersymmetry is a generalization of the notion of supersymmetry in which the minimal positive amount of spin does not have to be but can be an arbitrary for integer value of N. Such a generalization is possible in two or fewer spacetime dimensions.

## Current status

Supersymmetric models are constrained by a variety of experiments, including measurements of low-energy observables - for example, the anomalous magnetic moment of the muon at Fermilab; the WMAP dark matter density measurement and direct detection experiments - for example, XENON-100 and LUX; and by particle collider experiments, including B-physics, Higgs phenomenology and direct searches for superpartners (sparticles), at the Large Electron-Positron Collider, Tevatron and the LHC. In fact, CERN publicly states that if supersymmetry "is correct, supersymmetric particles should appear in collisions at the LHC."[44]

Historically, the tightest limits were from direct production at colliders. The first mass limits for squarks and gluinos were made at CERN by the UA1 experiment and the UA2 experiment at the Super Proton Synchrotron. LEP later set very strong limits,[45] which in 2006 were extended by the D0 experiment at the Tevatron.[46][47] From 2003-2015, WMAP's and Planck's dark matter density measurements have strongly constrained supersymmetry models, which, if they explain dark matter, have to be tuned to invoke a particular mechanism to sufficiently reduce the neutralino density.

Prior to the beginning of the LHC, in 2009, fits of available data to CMSSM and NUHM1 indicated that squarks and gluinos were most likely to have masses in the 500 to 800 GeV range, though values as high as 2.5 TeV were allowed with low probabilities. Neutralinos and sleptons were expected to be quite light, with the lightest neutralino and the lightest stau most likely to be found between 100 and 150 GeV.[48]

The first run of the LHC found no evidence for supersymmetry, and, as a result, surpassed existing experimental limits from the Large Electron-Positron Collider and Tevatron and partially excluded the aforementioned expected ranges.[49]

In 2011-12, the LHC discovered a Higgs boson with a mass of about 125 GeV, and with couplings to fermions and bosons which are consistent with the Standard Model. The MSSM predicts that the mass of the lightest Higgs boson should not be much higher than the mass of the Z boson, and, in the absence of fine tuning (with the supersymmetry breaking scale on the order of 1 TeV), should not exceed 135 GeV.[50]

The LHC result seems problematic for the minimal supersymmetric model, as the value of 125 GeV is relatively large for the model and can only be achieved with large radiative loop corrections from top squarks, which many theorists consider to be "unnatural" (see naturalness (physics) and fine tuning).[51] Some researchers seek to reconcile the current situation with the concept of "stringy naturalness",[52] where the Higgs mass is pulled via string landscape effects up to 125 GeV and sparticles masses pulled beyond the current LHC reach.

## References

1. ^ Haber, Howie. "Supersymmetry, Part I (Theory)" (PDF). Reviews, Tables and Plots. Particle Data Group (PDG). Retrieved 2015.
2. ^ "supersymmetry". Merriam-Webster. Retrieved 2017.
3. ^ Martin, Stephen P. (1997). "A Supersymmetry Primer". Perspectives on Supersymmetry. Advanced Series on Directions in High Energy Physics. 18. pp. 1-98. arXiv:hep-ph/9709356. doi:10.1142/9789812839657_0001. ISBN 978-981-02-3553-6. S2CID 118973381.
4. ^ Baer, Howard; Tata, Xerxes (2006). Weak scale supersymmetry: From superfields to scattering events.
5. ^ Dine, Michael (2007). Supersymmetry and String Theory: Beyond the Standard Model. p. 169.
6. ^ a b "ATLAS Supersymmetry Public Results". ATLAS Collaboration. CERN. Retrieved 2017.
7. ^ a b "CMS Supersymmetry Public Results". CMS. CERN. Retrieved 2017.
8. ^ Baron J, Campbell WC, Demille D, Doyle JM, Gabrielse G, et al. (2014). "Order of Magnitude Smaller Limit on the Electric Dipole Moment of the Electron". Science. 343 (6168): 269-272. arXiv:1310.7534. Bibcode:2014Sci...343..269B. doi:10.1126/science.1248213. PMID 24356114. S2CID 564518.
9. ^ Wolchover, Natalie (November 20, 2012). "Supersymmetry Fails Test, Forcing Physics to Seek New Ideas". Quanta Magazine.
10. ^ Wolchover, Natalie (August 9, 2016). "What No New Particles Means for Physics". Quanta Magazine.
11. ^ Shifman, M. (31 October 2012). Reflections and Impressionistic Portrait. Frontiers Beyond the Standard Model. FTPI. arXiv:1211.0004v1.
12. ^ Howard Baer; Vernon Barger; Dan Mickelson (September 2013). "How conventional measures overestimate electroweak fine-tuning in supersymmetric theory". Physical Review D. 88 (9): 095013. arXiv:1309.2984. Bibcode:2013PhRvD..88i5013B. doi:10.1103/PhysRevD.88.095013. S2CID 119288477.
13. ^ Howard Baer; Vernon Barger; Peisi Huang; Dan Mickelson; Azar Mustafayev; Xerxes Tata (December 2012). "Radiative natural supersymmetry: Reconciling electroweak fine-tuning and the Higgs boson mass". Physical Review D. 87 (11): 115028. arXiv:1212.2655. Bibcode:2013PhRvD..87k5028B. doi:10.1103/PhysRevD.87.115028. S2CID 73588737.
14. ^ Michael R. Douglas (May 2004). "Statistical analysis of the supersymmetry breaking scale". arXiv:hep-th/0405279.
15. ^ V. Agrawal; S. Barr; J. F. Donoghue; D. Seckel (January 1998). "Anthropic considerations in multiple domain theories and the scale of electroweak symmetry breaking". Physical Review Letters. 80 (9): 1822-1825. arXiv:hep-ph/9801253. Bibcode:1998PhRvL..80.1822A. doi:10.1103/PhysRevLett.80.1822. S2CID 14397884.
16. ^ H. Baer; V. Barger; H. Serce; K. Sinha (December 2017). "Higgs and superparticle mass predictions from the landscape". Journal of High Energy Physics. 1803 (3): 002. arXiv:1712.01399. doi:10.1007/JHEP03(2018)002. S2CID 113404486.
17. ^ H. Baer; A. Mustafayev; X. Tata (September 2014). "Monojet plus soft dilepton signal from light higgsino pair production at LHC14". Physical Review D. 90 (11): 115007. arXiv:1409.7058. Bibcode:2014PhRvD..90k5007B. doi:10.1103/PhysRevD.90.115007. S2CID 119194219.
18. ^ Atlas Collaboration (May 2019). "Searches for electroweak production of supersymmetric particles with compressed mass spectra in roots=13 TeV pp collisions with the ATLAS detector". Atlas-Conf-2019-014.
19. ^ David, Curtin (August 2011). Model Building And Collider Physics Above The Weak Scale (PDF) (PhD thesis). Cornell University.
20. ^ Feng, Jonathan (11 May 2007). "Supersymmetric Dark Matter" (PDF). University of California, Irvine.
21. ^ Bringmann, Torsten. "The WIMP "Miracle"" (PDF). University of Hamburg. Archived from the original (PDF) on 1 March 2013.
22. ^ Haag, Rudolf; ?opusza?ski, Jan T.; Sohnius, Martin (1975). "All possible generators of supersymmetries of the S-matrix". Nuclear Physics B. 88 (2): 257-274. Bibcode:1975NuPhB..88..257H. doi:10.1016/0550-3213(75)90279-5.
23. ^ H. Miyazawa (1966). "Baryon Number Changing Currents". Prog. Theor. Phys. 36 (6): 1266-1276. Bibcode:1966PThPh..36.1266M. doi:10.1143/PTP.36.1266.
24. ^ H. Miyazawa (1968). "Spinor Currents and Symmetries of Baryons and Mesons". Phys. Rev. 170 (5): 1586-1590. Bibcode:1968PhRv..170.1586M. doi:10.1103/PhysRev.170.1586.
25. ^ Kaku, Michio (1993). Quantum Field Theory. p. 663. ISBN 0-19-509158-2.
26. ^ Freund, Peter (1988-03-31). Introduction to Supersymmetry. pp. 26-27, 138. ISBN 0-521-35675-X.
27. ^ Gervais, J.-L.; Sakita, B. (1971). "Field theory interpretation of supergauges in dual models". Nuclear Physics B. 34 (2): 632-639. Bibcode:1971NuPhB..34..632G. doi:10.1016/0550-3213(71)90351-8.
28. ^ D. V. Volkov, V. P. Akulov, Pisma Zh.Eksp.Teor.Fiz. 16 (1972) 621; Phys.Lett. B46 (1973) 109; V.P. Akulov, D.V. Volkov, Teor.Mat.Fiz. 18 (1974) 39
29. ^ Ramond, P. (1971). "Dual Theory for Free Fermions". Physical Review D. 3 (10): 2415-2418. Bibcode:1971PhRvD...3.2415R. doi:10.1103/PhysRevD.3.2415.
30. ^ Wess, J.; Zumino, B. (1974). "Supergauge transformations in four dimensions". Nuclear Physics B (Submitted manuscript). 70 (1): 39-50. Bibcode:1974NuPhB..70...39W. doi:10.1016/0550-3213(74)90355-1.
31. ^ Hagen Kleinert, Discovery of Supersymmetry in Nuclei
32. ^ Iachello, F. (1980). "Dynamical Supersymmetries in Nuclei". Physical Review Letters. 44 (12): 772-775. Bibcode:1980PhRvL..44..772I. doi:10.1103/PhysRevLett.44.772. S2CID 14130911.
33. ^ Friedan, D.; Qiu, Z.; Shenker, S. (1984). "Conformal Invariance, Unitarity, and Critical Exponents in Two Dimensions". Physical Review Letters. 52 (18): 1575-1578. Bibcode:1984PhRvL..52.1575F. doi:10.1103/PhysRevLett.52.1575. S2CID 122320349.
34. ^ a b Kane, Gordon L. (June 2003). "The Dawn of Physics Beyond the Standard Model". Scientific American. 288 (6): 68-75. Bibcode:2003SciAm.288f..68K. doi:10.1038/scientificamerican0603-68. PMID 12764939.
35. ^ "The Frontiers of Physics". Scientific American Special Edition. 15 (3): 8. 2005.
36. ^ Efetov, Konstantin (1997). Supersymmetry in Disorder and Chaos. Cambridge University Press.
37. ^ Miri, M.-A.; Heinrich, M.; El-Ganainy, R.; Christodoulides, D. N. (2013). "Superymmetric optical structures". Physical Review Letters. 110 (23): 233902. arXiv:1304.6646. Bibcode:2013PhRvL.110w3902M. doi:10.1103/PhysRevLett.110.233902. PMID 25167493. S2CID 15354588.
38. ^ Heinrich, M.; Miri, M.-A.; Stützer, S.; El-Ganainy, R.; Nolte, S.; Szameit, A.; Christodoulides, D. N. (2014). "Superymmetric mode converters". Nature Communications. 5: 3698. arXiv:1401.5734. Bibcode:2014NatCo...5.3698H. doi:10.1038/ncomms4698. PMID 24739256. S2CID 2070325.
39. ^ Miri, M.-A.; Heinrich, Matthias; Christodoulides, D. N. (2014). "SUSY-inspired one-dimensional transformation optics". Optica. 1 (2): 89-95. arXiv:1408.0832. Bibcode:2014arXiv1408.0832M. doi:10.1364/OPTICA.1.000089. S2CID 15561466.
40. ^ Ovchinnikov, Igor (March 2016). "Introduction to Supersymmetric Theory of Stochastics". Entropy. 18 (4): 108. arXiv:1511.03393. Bibcode:2016Entrp..18..108O. doi:10.3390/e18040108. S2CID 2388285.
41. ^ Ovchinnikov, Igor; Ensslin, Torsten (April 2016). "Kinematic dynamo, supersymmetry breaking, and chaos". Physical Review D. 93 (8): 085023. arXiv:1512.01651. Bibcode:2016PhRvD..93h5023O. doi:10.1103/PhysRevD.93.085023. S2CID 59367815.
42. ^ Krasnitz, Michael (2003). Correlation functions in supersymmetric gauge theories from supergravity fluctuations (PDF). Princeton University Department of Physics: Princeton University Department of Physics. p. 91.
43. ^ Polchinski, J. String Theory. Vol. 2: Superstring theory and beyond, Appendix B
44. ^ "Supersymmetry predicts a partner particle for each particle in the Standard Model, to help explain why particles have mass". CERN: Supersymmetry. Retrieved 2019.
45. ^ LEPSUSYWG, ALEPH, DELPHI, L3 and OPAL experiments, charginos, large m0 LEPSUSYWG/01-03.1
46. ^ The D0-Collaboration (2009). "Search for associated production of charginos and neutralinos in the trilepton final state using 2.3 fb-1 of data". Physics Letters B. 680 (1): 34-43. arXiv:0901.0646. Bibcode:2009PhLB..680...34D. doi:10.1016/j.physletb.2009.08.011. hdl:10211.3/195394. S2CID 54016374.
47. ^ The D0 Collaboration (2008). "Search for squarks and gluinos in events with jets and missing transverse energy using 2.1 fb-1 of pp- collision data at s = 1.96 TeV". Physics Letters B. 660 (5): 449-457. arXiv:0712.3805. Bibcode:2008PhLB..660..449D. doi:10.1016/j.physletb.2008.01.042. S2CID 18574837.
48. ^ Buchmueller O, et al. (2009). "Likelihood Functions for Supersymmetric Observables in Frequentist Analyses of the CMSSM and NUHM1". The European Physical Journal C. 64 (3): 391-415. arXiv:0907.5568. Bibcode:2009EPJC...64..391B. doi:10.1140/epjc/s10052-009-1159-z. S2CID 9430917.
49. ^ Roszkowski, Leszek; Sessolo, Enrico Maria; Williams, Andrew J. (11 August 2014). "What next for the CMSSM and the NUHM: improved prospects for superpartner and dark matter detection". Journal of High Energy Physics. 2014 (8): 67. arXiv:1405.4289. Bibcode:2014JHEP...08..067R. doi:10.1007/JHEP08(2014)067. S2CID 53526400.
50. ^ Marcela Carena and Howard E. Haber; Haber (2003). "Higgs Boson Theory and Phenomenology". Progress in Particle and Nuclear Physics. 50 (1): 63-152. arXiv:hep-ph/0208209. Bibcode:2003PrPNP..50...63C. doi:10.1016/S0146-6410(02)00177-1. S2CID 5163410.
51. ^ Draper, Patrick; Meade, Patrick; Reece, Matthew; Shih, David (December 2011). "Implications of a 125 GeV Higgs for the MSSM and Low-Scale SUSY Breaking". Physical Review D. 85 (9): 095007. arXiv:1112.3068. Bibcode:2012PhRvD..85i5007D. doi:10.1103/PhysRevD.85.095007. S2CID 118577425.
52. ^ H. Baer; V. Barger; S. Salam (June 2019). "Naturalness versus stringy naturalness (with implications for collider and dark matter searches)". Physical Review Research. 1 (2): 023001. arXiv:1906.07741. Bibcode:2019arXiv190607741B. doi:10.1103/PhysRevResearch.1.023001. S2CID 195068902.

### On experiments

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