The Minimal Supersymmetric Standard Model (MSSM) is an extension to the Standard Model that realizes supersymmetry. MSSM is the minimal supersymmetrical model as it considers only "the [minimum] number of new particle states and new interactions consistent with phenomenology".^{[1]} Supersymmetry pairs bosons with fermions; therefore every Standard Model particle has a partner that has yet to be discovered. If the superparticles are found, it may be analogous to discovering dark matter ^{[2]} and depending on the details of what might be found, it could provide evidence for grand unification and might even, in principle, provide hints as to whether string theory describes nature. The failure to find evidence for supersymmetry using the Large Hadron Collider since 2010 has led to suggestions that the theory should be abandoned.^{[3]}
Contents

Background 1

Theoretical motivations 2

Naturalness 2.1

Gaugecoupling unification 2.2

Dark matter 2.3

Predictions of the MSSM regarding hadron colliders 3

Neutralinos 3.1

Charginos 3.2

Squarks 3.3

Gluinos 3.4

Sleptons 3.5

MSSM fields 4

MSSM superfields 4.1

MSSM Higgs Mass 4.2

The MSSM Lagrangian 5

Problems with the MSSM 6

Theories of supersymmetry breaking 7

Gravitymediated supersymmetry breaking 7.1

Gaugemediated supersymmetry breaking (GMSB) 7.2

Anomalymediated supersymmetry breaking (AMSB) 7.3

Phenomenological MSSM (pMSSM) 8

See also 9

References 10

External links 11
Background
The MSSM was originally proposed in 1981 to stabilize the weak scale, solving the [4] The Higgs boson mass of the Standard Model is unstable to quantum corrections and the theory predicts that weak scale should be much weaker than what is observed to be. In the MSSM, the Higgs boson has a fermionic superpartner, the Higgsino, that has the same mass as it would if supersymmetry were an exact symmetry. Because fermion masses are radiatively stable, the Higgs mass inherits this stability. However, in MSSM there is a need for more than one Higgs field, as described below.
The only unambiguous way to claim discovery of supersymmetry is to produce superparticles in the laboratory. Because superparticles are expected to be 100 to 1000 times heavier than the proton, it requires a huge amount of energy to make these particles that can only be achieved at particle accelerators. The Tevatron was actively looking for evidence of the production of supersymmetric particles before it was shut down on 30 September 2011. Most physicists believe that supersymmetry must be discovered at the LHC if it is responsible for stabilizing the weak scale. There are five classes of particle that superpartners of the Standard Model fall into: squarks, gluinos, charginos, neutralinos, and sleptons. These superparticles have their interactions and subsequent decays described by the MSSM and each has characteristic signatures.
An example of a flavor changing neutral current process in MSSM. A strange quark emits a bino, turning into a sdowntype quark, which then emits a Z boson and reabsorbs the bino, turning into a down quark. If the MSSM squark masses are flavor violating, such a process can occur.
The MSSM imposes Rparity to explain the stability of the proton. It adds supersymmetry breaking by introducing explicit soft supersymmetry breaking operators into the Lagrangian that is communicated to it by some unknown (and unspecified) dynamics. This means that there are 120 new parameters in the MSSM. Most of these parameters lead to unnacceptable phenomenology such as large flavor changing neutral currents or large electric dipole moments for the neutron and electron. To avoid these problems, the MSSM takes all of the soft supersymmetry breaking to be diagonal in flavor space and for all of the new CP violating phases to vanish.
Theoretical motivations
There are three principal motivations for the MSSM over other theoretical extensions of the Standard Model, namely:
These motivations come out without much effort and they are the primary reasons why the MSSM is the leading candidate for a new theory to be discovered at collider experiments such as the Tevatron or the LHC.
Naturalness
The original motivation for proposing the MSSM was to stabilize the Higgs mass to radiative corrections that are quadratically divergent in the Standard Model (hierarchy problem). In supersymmetric models, scalars are related to fermions and have the same mass. Since fermion masses are logarithmically divergent, scalar masses inherit the same radiative stability. The Higgs vacuum expectation value is related to the negative scalar mass in the Lagrangian. In order for the radiative corrections to the Higgs mass to not be dramatically larger than the actual value, the mass of the superpartners of the Standard Model should not be significantly heavier than the Higgs VEV—roughly 100 GeV. In 2012, the Higgs particle was discovered at the LHC, and its mass was found to be 125126 GeV.
Gaugecoupling unification
If the superpartners of the Standard Model are near the TeV scale, then measured gauge couplings of the three gauge groups unify at high energies.^{[5]} ^{[6]} ^{[7]} The betafunctions for the MSSM gauge couplings are given by
Gauge Group

\alpha^{1}(M_{Z^0})

b_0^\mathrm{MSSM}

SU(3)

8.5

3

SU(2)

29.6

+1

U(1)

59.2

+6\frac{3}{5}

where \alpha^{1}_{1} is measured in SU(5) normalization—a factor of \frac{3}{5} different than the Standard Model's normalization and predicted by Georgi–Glashow SU(5) .
The condition for gauge coupling unification at one loop is whether the following expression is satisfied \frac{\alpha^{1}_3  \alpha^{1}_2}{\alpha^{1}_2\alpha^{1}_1} = \frac{b_{0\,3}  b_{0\,2}}{b_{0\,2} b_{0\,1}}.
Remarkably, this is precisely satisfied to experimental errors in the values of \alpha^{1}(M_{Z^0}). There are two loop corrections and both TeVscale and GUTscale threshold corrections that alter this condition on gauge coupling unification, and the results of more extensive calculations reveal that gauge coupling unification occurs to an accuracy of 1%, though this is about 3 standard deviations from the theoretical expectations.
This prediction is generally considered as indirect evidence for both the MSSM and SUSY GUTs.^{[8]} It should be noted that gauge coupling unification does not necessarily imply grand unification and there exist other mechanisms to reproduce gauge coupling unification. However, if superpartners are found in the near future, the apparent success of gauge coupling unification would suggest that a supersymmetric grand unified theory is a promising candidate for high scale physics.
Dark matter
If Rparity is preserved, then the lightest superparticle (LSP) of the MSSM is stable and is a Weakly interacting massive particle (WIMP) — i.e. it does not have electromagnetic or strong interactions. This makes the LSP a good dark matter candidate and falls into the category of cold dark matter (CDM) particle.
Predictions of the MSSM regarding hadron colliders
The Tevatron and LHC have active experimental programs searching for supersymmetric particles. Since both of these machines are hadron colliders — proton antiproton for the Tevatron and proton proton for the LHC — they search best for strongly interacting particles. Therefore, most experimental signature involve production of squarks or gluinos. Since the MSSM has Rparity, the lightest supersymmetric particle is stable and after the squarks and gluinos decay each decay chain will contain one LSP that will leave the detector unseen. This leads to the generic prediction that the MSSM will produce a 'missing energy' signal from these particles leaving the detector.
Neutralinos
There are four neutralinos that are fermions and are electrically neutral, the lightest of which is typically stable. They are typically labeled N͂0
1, N͂0
2, N͂0
3, N͂0
4 (although sometimes \tilde{\chi}_1^0, \ldots, \tilde{\chi}_4^0 is used instead). These four states are mixtures of the Bino and the neutral Wino (which are the neutral electroweak Gauginos), and the neutral Higgsinos. As the neutralinos are Majorana fermions, each of them is identical with its antiparticle. Because these particles only interact with the weak vector bosons, they are not directly produced at hadron colliders in copious numbers. They primarily appear as particles in cascade decays of heavier particles usually originating from colored supersymmetric particles such as squarks or gluinos.
In Rparity conserving models, the lightest neutralino is stable and all supersymmetric cascades decays end up decaying into this particle which leaves the detector unseen and its existence can only be inferred by looking for unbalanced momentum in a detector.
The heavier neutralinos typically decay through a Z0 to a lighter neutralino or through a W± to chargino. Thus a typical decay is
N͂0
2

→

N͂0
1

+

Z0


→

Missing energy

+

l+

+

l−

N͂0
2

→

C\tilde \chi±
1

+

W∓

→

N͂0
1

+

W±

+

W∓

→

Missing energy

+

l+

+

l−

The mass splittings between the different Neutralinos will dictate which patterns of decays are allowed.
Charginos
There are two Charginos that are fermions and are electrically charged. They are typically labeled C\tilde \chi±
1 and C\tilde \chi±
2 (although sometimes \tilde{\chi}_1^\pm and \tilde{\chi}_2^\pm is used instead). The heavier chargino can decay through Z0 to the lighter chargino. Both can decay through a W± to neutralino.
Squarks
The squarks are the scalar superpartners of the quarks and there is one version for each Standard Model quark. Due to phenomenological constraints from flavor changing neutral currents, typically the lighter two generations of squarks have to be nearly the same in mass and therefore are not given distinct names. The superpartners of the top and bottom quark can be split from the lighter squarks and are called stop and sbottom.
On the other way, there may be a remarkable leftright mixing of the stops \tilde{t} and of the sbottoms \tilde{b} because of the high masses of the partner quarks top and bottom: ^{[9]}

\tilde{t}_1 = e^{+i\phi} \cos(\theta) \tilde{t_L} + \sin(\theta) \tilde{t_R}

\tilde{t}_2 = e^{i\phi} \cos(\theta) \tilde{t_R}  \sin(\theta) \tilde{t_L}
Same holds for bottom \tilde{b} with its own parameters \phi and \theta.
Squarks can be produced through strong interactions and therefore are easily produced at hadron colliders. They decay to quarks and neutralinos or charginos which further decay. In Rparity conserving scenarios, squarks are pair produced and therefore a typical signal is

\tilde{q}\tilde{\bar{q}} \rightarrow q \tilde{N}^0_1 \bar{q} \tilde{N}^0_1 \rightarrow 2 jets + missing energy

\tilde{q}\tilde{\bar{q}} \rightarrow q \tilde{N}^0_2 \bar{q} \tilde{N}^0_1 \rightarrow q \tilde{N}^0_1 \ell \bar{\ell} \bar{q} \tilde{N}^0_1 \rightarrow 2 jets + 2 leptons + missing energy
Gluinos
Gluinos are Majorana fermionic partners of the gluon which means that they are their own antiparticles. They interact strongly and therefore can be produced significantly at the LHC. They can only decay to a quark and a squark and thus a typical gluino signal is

\tilde{g}\tilde{g}\rightarrow (q \tilde{\bar{q}}) (\bar{q} \tilde{q}) \rightarrow (q \bar{q} \tilde{N}^0_1) (\bar{q} q \tilde{N}^0_1) \rightarrow 4 jets + Missing energy
Because gluinos are Majorana, gluinos can decay to either a quark+antisquark or an antiquark+squark with equal probability. Therefore, pairs of gluinos can decay to

\tilde{g}\tilde{g}\rightarrow (\bar{q} \tilde{q}) (\bar{q} \tilde{q}) \rightarrow (q \bar{q} \tilde{C}^+_1) (q \bar{q} \tilde{C}^+_1) \rightarrow (q \bar{q} W^+) (q \bar{q} W^+) \rightarrow 4 jets+ \ell^+ \ell^++ Missing energy
This is a distinctive signature because it has samesign dileptons and has very little background in the Standard Model.
Sleptons
Sleptons are the scalar partners of the leptons of the Standard Model. They are not strongly interacting and therefore are not produced very often at hadron colliders unless they are very light.
Because of the high mass of the tau lepton there will be leftright mixing of the stau similar to that of stop and sbottom (see above).
Sfermions will typically be found in decays of a charginos and neutralinos if they are light enough to be a decay product

\tilde{C}^+\rightarrow \tilde{\ell}^+ \nu

\tilde{N}^0 \rightarrow \tilde{\ell}^+ \ell^
MSSM fields
Fermions have bosonic superpartners (called sfermions), and bosons have fermionic superpartners (called bosinos). For most of the Standard Model particles, doubling is very straightforward. However, for the Higgs boson, it is more complicated.
A single Higgsino (the fermionic superpartner of the Higgs boson) would lead to a gauge anomaly and would cause the theory to be inconsistent. However, if two Higgsinos are added, there is no gauge anomaly. The simplest theory is one with two Higgsinos and therefore two scalar Higgs doublets. Another reason for having two scalar Higgs doublets rather than one is in order to have Yukawa couplings between the Higgs and both downtype quarks and uptype quarks; these are the terms responsible for the quarks' masses. In the Standard Model the downtype quarks couple to the Higgs field (which has Y=1/2) and the uptype quarks to its complex conjugate (which has Y=+1/2). However, in a supersymmetric theory this is not allowed, so two types of Higgs fields are needed.
SM Particle type

Particle

Symbol

Spin

RParity

Superpartner

Symbol

Spin

Rparity

Fermions

Quark

q

\begin{matrix} \frac{1}{2} \end{matrix}

+1

Squark

\tilde{q}

0

1

Lepton

\ell

\begin{matrix} \frac{1}{2} \end{matrix}

+1

Slepton

\tilde{\ell}

0

1

Bosons

W

W

1

+1

Wino

\tilde{W}

\begin{matrix} \frac{1}{2} \end{matrix}

1

B

B

1

+1

Bino

\tilde{B}

\begin{matrix} \frac{1}{2} \end{matrix}

1

Gluon

g

1

+1

Gluino

\tilde{g}

\begin{matrix} \frac{1}{2} \end{matrix}

1

Higgs bosons

Higgs

h_u, h_d

0

+1

Higgsinos

\tilde{h}_u, \tilde{h}_d

\begin{matrix} \frac{1}{2} \end{matrix}

1

MSSM superfields
In supersymmetric theories, every field and its superpartner can be written together as a superfield. The superfield formulation of supersymmetry is very convenient to write down manifestly supersymmetric theories (i.e. one does not have to tediously check that the theory is supersymmetric term by term in the Lagrangian). The MSSM contains vector superfields associated with the Standard Model gauge groups which contain the vector bosons and associated gauginos. It also contains chiral superfields for the Standard Model fermions and Higgs bosons (and their respective superpartners).
MSSM Higgs Mass
The MSSM Higgs Mass is a prediction of the Minimal Supersymmetric Standard Model. The mass of the lightest Higgs boson is set by the Higgs quartic coupling. Quartic couplings are not soft supersymmetrybreaking parameters since they lead to a quadratic divergence of the Higgs mass. Furthermore, there are no supersymmetric parameters to make the Higgs mass a free parameter in the MSSM (though not in nonminimal extensions). This means that Higgs mass is a prediction of the MSSM. The LEP II and the IV experiments placed a lower limit on the Higgs mass of 114.4 GeV. This lower limit is significantly above where the MSSM would typically predict it to be, and while it does not rule out the MSSM, the discovery of the Higgs with a mass of 125 GeV makes proponents of the MSSM nervous.^{[10]}^{[11]}
Formulas
The only susypreserving operator that creates a quartic coupling for the Higgs in the MSSM arise for the Dterms of the SU(2) and U(1) gauge sector and the magnitude of the quartic coupling is set by the size of the gauge couplings.
This leads to the prediction that the Standard Modellike Higgs mass (the scalar that couples approximately to the vev) is limited to be less than the Z mass
m_{h^0}^2 \le m_{Z^0}^2\cos^2 2\beta .
Since supersymmetry is broken, there are radiative corrections to the quartic coupling that can increase the Higgs mass. These dominantly arise from the 'top sector'
m_{h^0}^2 \le m_{Z^0}^2\cos^2 2\beta + \frac{3}{\pi^2} \frac{m_t^4 \sin^4\beta}{v^2} \log \frac{m_{\tilde{t}}}{m_t}
where m_t is the Top quark mass and m_{\tilde{t}} is the mass of the top squark. This result can be interpreted as the RG running of the Higgs quartic coupling from the scale of supersymmetry to the top mass—however since the top squark mass should be relatively close to the top mass, this is usually a fairly modest contribution and increases the Higgs mass to roughly the LEP II bound of 114 GeV before the top squark becomes too heavy.
Finally there is a contribution from the top squark Aterms
\mathcal{L} = y_t\, m_{\tilde{t}}\, a\; h_u \tilde{q}_3 \tilde{u}^c_3
where a is a dimensionless number. This contributes an additional term to the Higgs mass at loop level, but is not logarithmically enhanced
m_{h^0}^2 \le m_{Z^0}^2\cos^2 2\beta + \frac{3}{\pi^2} \frac{m_t^4 \sin^4\beta}{v^2} \left(\log \frac{m_{\tilde{t}}}{m_t} + a^2 ( 1  a^2/12) \right)
by pushing a \rightarrow \sqrt{6} (known as 'maximal mixing') it is possible to push the Higgs mass to 125 GeV without decoupling the top squark or adding new dynamics to the MSSM.
As the Higgs was found at around 125 GeV (along with no other superparticles) at the LHC, this strongly hints at new dynamics beyond the MSSM, such as the 'Next to Minimal Supersymmetric Standard Model' (NMSSM); and suggests some correlation to the little hierarchy problem.
The MSSM Lagrangian
The Lagrangian for the MSSM contains several pieces.

The first is the Kähler potential for the matter and Higgs fields which produces the kinetic terms for the fields.

The second piece is the gauge field superpotential that produces the kinetic terms for the gauge bosons and gauginos.

The next term is the superpotential for the matter and Higgs fields. These produce the Yukawa couplings for the Standard Model fermions and also the mass term for the Higgsinos. After imposing Rparity, the renormalizable, gauge invariant operators in the superpotential are
W_{}^{} = \mu H_u H_d+ y_u H_u Q U^c+ y_d H_d Q D^c + y_l H_d L E^c
The constant term is unphysical in global supersymmetry (as opposed to supergravity).
Soft Susy breaking
The last piece of the MSSM Lagrangian is the soft supersymmetry breaking Lagrangian. The vast majority of the parameters of the MSSM are in the susy breaking Lagrangian. The soft susy breaking are divided into roughly three pieces.

The first are the gaugino masses
\mathcal{L} \supset m_{\frac{1}{2}} \tilde{\lambda}\tilde{\lambda} + \text{h.c.}
Where \tilde{\lambda} are the gauginos and m_{\frac{1}{2}} is different for the wino, bino and gluino.

The next are the soft masses for the scalar fields
\mathcal{L} \supset m^2_0 \phi^\dagger \phi
where \phi are any of the scalars in the MSSM and m_0 are 3\times 3 hermitean matrices for the squarks and sleptons of a given set of gauge quantum numbers. The eigenvalues of these matrices are actually the masses squared, rather than the masses.

There are the A and B terms which are given by
\mathcal{L} \supset B_{\mu} h_u h_d + A h_u \tilde{q} \tilde{u^c}+ A h_d \tilde{q} \tilde{d^c} +A h_d \tilde{l} \tilde{e^c} + \text{h.c.}
The A terms are 3\times 3 complex matrices much as the scalar masses are.

Although not often mentioned with regard to soft terms, to be consistent with observation, one must also include Gravitino and Goldstino soft masses given by
\mathcal{L} \supset m_{3/2}\Psi_{\mu}^{\alpha}(\sigma^{\mu\nu})_{\alpha}^{\beta}\Psi_{\beta} + m_{3/2}G^{\alpha}G_{\alpha}+\text{h.c.}
The reason these soft terms are not often mentioned are that they arise through local supersymmetry and not global supersymmetry, although they are required otherwise if the Goldstino were massless it would contradict observation. The Goldstino mode is eaten by the Gravitino to become massive, through a gauge shift, which also absorbs the wouldbe "mass" term of the Goldstino.
Problems with the MSSM
There are several problems with the MSSM — most of them falling into understanding the parameters.

The mu problem: The Higgsino mass parameter μ appears as the following term in the superpotential: μH_{u}H_{d}. It should have the same order of magnitude as the electroweak scale, many orders of magnitude smaller than that of the Planck scale, which is the natural cutoff scale. The soft supersymmetry breaking terms should also be of the same order of magnitude as the electroweak scale. This brings about a problem of naturalness: why are these scales so much smaller than the cutoff scale yet happen to fall so close to each other?

Flavor universality of soft masses and Aterms: since no flavor mixing additional to that predicted by the standard model has been discovered so far, the coefficients of the additional terms in the MSSM Lagrangian must be, at least approximately, flavor invariant (i.e. the same for all flavors).

Smallness of CP violating phases: since no CP violation additional to that predicted by the standard model has been discovered so far, the additional terms in the MSSM Lagrangian must be, at least approximately, CP invariant, so that their CP violating phases are small.
Theories of supersymmetry breaking
A large amount of theoretical effort has been spent trying to understand the mechanism for soft supersymmetry breaking that produces the desired properties in the superpartner masses and interactions. The three most extensively studied mechanisms are:
Gravitymediated supersymmetry breaking
Gravitymediated supersymmetry breaking is a method of communicating supersymmetry breaking to the supersymmetric Standard Model through gravitational interactions. It was the first method proposed to communicate supersymmetry breaking. In gravitymediated supersymmetrybreaking models, there is a part of the theory that only interacts with the MSSM through gravitational interaction. This hidden sector of the theory breaks supersymmetry. Through the supersymmetric version of the Higgs mechanism, the gravitino, the supersymmetric version of the graviton, acquires a mass. After the gravitino has a mass, gravitational radiative corrections to soft masses are incompletely cancelled beneath the gravitino's mass.
It is currently believed that it is not generic to have a sector completely decoupled from the MSSM and there should be higher dimension operators that couple different sectors together with the higher dimension operators suppressed by the Planck scale. These operators give as large of a contribution to the soft supersymmetry breaking masses as the gravitational loops; therefore, today people usually consider gravity mediation to be gravitational sized direct interactions between the hidden sector and the MSSM.
mSUGRA
stands for minimal supergravity. The construction of a realistic model of interactions within N = 1 supergravity framework where supersymmetry breaking is communicated through the supergravity interactions was carried out by Ali Chamseddine, Richard Arnowitt, and Pran Nath in 1982.^{[12]} mSUGRA is one of the most widely investigated models of particle physics due to its predictive power requiring only 4 input parameters and a sign, to determine the low energy phenomenology from the scale of Grand Unification. The most widely used set of parameters is:
Symbol

Description

m_0

the common mass of the scalars (sleptons, squarks, Higgs bosons) at the Grand Unification scale

m_{1/2}

the common mass of the gauginos and higgsinos at the Grand Unification scale

A_0

the common trilinear coupling

\tan \beta

the ratio of the vacuum expectation values of the two Higgs doublets

\mathrm{sign}(\mu)

the sign of the higgsino mass parameter

GravityMediated Supersymmetry Breaking was assumed to be flavor universal because of the universality of gravity; however, in 1986 Hall, Kostelecky, and Raby ^{[13]} showed that Planckscale physics that are necessary to generate the StandardModel Yukawa couplings spoil the universality of the supersymmetry breaking.
Gaugemediated supersymmetry breaking (GMSB)
Gaugemediated supersymmetry breaking is method of communicating supersymmetry breaking to the supersymmetric Standard Model through the Standard Model's gauge interactions. Typically a hidden sector breaks supersymmetry and communicates it to massive messenger fields that are charged under the Standard Model. These messenger fields induce a gaugino mass at one loop and then this is transmitted on to the scalar superpartners at two loops. Requiring stop squarks below 2 TeV, the maximum Higg's boson mass predicted is just 121.5GeV.^{[14]} With the Higgs being discovered at 125GeV  this model requires stops above 2 TeV.
Anomalymediated supersymmetry breaking (AMSB)
Anomalymediated supersymmetry breaking is a special type of gravity mediated supersymmetry breaking that results in supersymmetry breaking being communicated to the supersymmetric Standard Model through the conformal anomaly.^{[15]}^{[16]} Requiring stop squarks below 2 TeV, the maximum Higg's boson mass predicted is just 121.0GeV.^{[14]} With the Higgs being discovered at 125GeV  this scenario requires stops heavier than 2 TeV.
Phenomenological MSSM (pMSSM)
The unconstrained MSSM has more than 100 parameters in addition to the Standard Model parameters. This makes any phenomenological analysis (e.g. finding regions in parameter space consistent with observed data) impractical. Under the following three assumptions:

no new source of CPviolation

no Flavour Changing Neutral Currents

first and second generation universality
one can reduce the number of additional parameters to the following 19 quantities of the phenomenological MSSM (pMSSM):^{[17]} The large parameter space of pMSSM makes searches in pMSSM extremely challenging and makes pMSSM difficult to exclude.
Symbol

Description

number of parameters

\tan \beta

the ratio of the vacuum expectation values of the two Higgs doublets

1

M_A

the mass of the pseudoscalar Higgs boson

1

\mu

the higgsino mass parameter

1

M_1

the bino mass parameter

1

M_2

the wino mass parameter

1

M_3

the gluino mass parameter

1

m_\tilde{q}, m_{\tilde{u}_R}, m_{\tilde{d}_R}

the first and second generation squark masses

3

m_\tilde{l}, m_{\tilde{e}_R}

the first and second generation slepton masses

2

m_\tilde{Q}, m_{\tilde{t}_R}, m_{\tilde{b}_R}

the third generation squark masses

3

m_\tilde{L}, m_{\tilde{\tau}_R}

the third generation slepton masses

2

A_t, A_b, A_\tau

the third generation trilinear couplings

3

See also
References

^ Howard Baer; Xerxes Tata (2006). "8  The Minimal Supersymmetric Standard Model". Weak Scale Supersymmetry From Superfields to Scattering Events. Cambridge: Cambridge University Press. p. 127.

^ Murayama, Hitoshi (2000). "Supersymmetry phenomenology".

^ Wolchover, Natalie (November 29, 2012). "Supersymmetry Fails Test, Forcing Physics to Seek New Ideas". Scientific American.

^ S. Dimopoulos, H. Georgi; Georgi (1981). "Softly Broken Supersymmetry and SU(5)".

^ S. Dimopoulos, S. Raby and F. Wilczek; Raby; Wilczek (1981). "Supersymmetry and the Scale of Unification".

^ L.E. Ibanez and G.G. Ross; Ross (1981). "Lowenergy predictions in supersymmetric grand unified theories".

^ W.J. Marciano and G. Senjanovic; Senjanović (1982). "Predictions of supersymmetric grand unified theories".

^ Gordon Kane, "The Dawn of Physics Beyond the Standard Model", Scientific American, June 2003, page 60 and The frontiers of physics, special edition, Vol 15, #3, page 8 "Indirect evidence for supersymmetry comes from the extrapolation of interactions to high energies."

^ Bartl, A.; Hesselbach, S.; Hidaka, K.; Kernreiter, T.; Porod, W. (2003). "Impact of SUSY CP Phases on Stop and Sbottom Decays in the MSSM".

^ Heinemeyer, S.; Stål, O.; Weiglein, G. (2012). "Interpreting the LHC Higgs search results in the MSSM". Physics Letters B 710: 201.

^ Carena, M.; Heinemeyer, S.; Wagner, C. E. M.; Weiglein, G. (2006). "MSSM Higgs boson searches at the evatron and the LHC: Impact of different benchmark scenarios" (PDF). The European Physical Journal C 45 (3): 797.

^ A. Chamseddine, R. Arnowitt, P. Nath; Arnowitt; Nath (1982). "Locally Supersymmetric Grand Unification".

^ L.J. Hall, V.A. Kostelecky, S. Raby; Kostelecky; Raby (1986). "New Flavor Violations in Supergravity Models".

^ ^{a} ^{b} Arbey, A.; Battaglia, M.; Djouadi, A.; Mahmoudi, F.; Quevillon, J. (2011). "Implications of a 125 GeV Higgs for supersymmetric models". Physics Letters B. 3 708 (2012): 162–169.

^ L. Randall, R. Sundrum; Sundrum (1999). "Out of this world supersymmetry breaking".

^ G. Giudice, M. Luty, H. Murayama, R. Rattazzi; Rattazzi; Luty; Murayama (1998). "Gaugino mass without singlets".

^ Djouadi, A.; RosierLees, S.; Bezouh, M.; Bizouard, M. A.; Boehm, C.; Borzumati, F.; Briot, C.; Carr, J.; Causse, M. B.; Charles, F.; Chereau, X.; Colas, P.; Duflot, L.; Dupperin, A.; Ealet, A.; ElMamouni, H.; Ghodbane, N.; Gieres, F.; GonzalezPineiro, B.; Gourmelen, S.; Grenier, G.; Gris, Ph.; Grivaz, J. F.; Hebrard, C.; Ille, B.; Kneur, J. L.; Kostantinidis, N.; Layssac, J.; Lebrun, P.; et al. (1999). "The Minimal Supersymmetric Standard Model: Group Summary Report".
External links

MSSM on arxiv.org

Stephen P. Martin (1997). "A Supersymmetry Primer".

Particle Data Group review of MSSM and search for MSSM predicted particles

Ian J R Aitchison (2005). "Supersymmetry and the MSSM: An Elementary Introduction".
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