REVIEW
Soft supersymmetry-breaking terms from supergravity and superstring models
High Energy Physics - Phenomenology · Submitted 1 Jul 1997 · 44 references
Pith's verdict: A solid, honest review of hidden-sector soft terms; its most-quoted numbers are a conditional the paper itself says fails.
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Referee report
The paper
The paper claims
In N=1 supergravity the soft supersymmetry-breaking terms of the visible sector are computable from three functions — the Kähler potential, the superpotential and the gauge kinetic function — and in the dilaton-dominated superstring limit,
The reading
What carries the argument
The engine is the flat-limit reduction of the supergravity Lagrangian: replace the hidden fields $h^m$ and their auxiliary $F$-terms by their vacuum expectation values, let $M_P to infinity$ while holding $m_{3/2} = e^{G/2}$ fixed, and read off the residual global-SUSY Lagrangian plus soft breaking terms. The second piece of machinery is the goldstino-angle parametrization, $F^S = sqrt{3},C,m_{3/2},hatK_{SS}^{-1/2} sin theta,e^{-i gamma_S}$ and $F^i = sqrt{3},C,m_{3/2} cos theta,P^{ij}Theta_j$, which packages all ignorance about the non-perturbative superpotential into one angle $theta$ and a unit vector $Theta_j$; the dilaton-dominated limit is $cos theta = 0$. This lets the authors turn a statement about an unknown supersymmetry-breaking mechanism into a one-parameter family of predictions for measurable soft masses.
Extended reading notes
Core claim
The central claim is that soft supersymmetry breaking in supergravity is not a free input but a derived quantity. Expanding the supergravity Lagrangian in the observable fields and taking the flat limit $M_P to infinity$ with $m_{3/2}$ fixed yields explicit expressions for gaugino masses, scalar masses, trilinear $A$ terms and bilinear $B$ terms in terms of the hidden-sector $F$-terms and the derivatives of the Kähler potential, superpotential and gauge kinetic function. Applied to superstrings, where the hidden sector is the dilaton $S$ and the moduli $T_i$, and with the tree-level gauge kinetic function $f_a = k_a S$, the gaugino masses come out universal and equal to $sqrt{3},C,m_{3/2},e^{-i gamma_S}$. In the limit where the dilaton alone breaks supersymmetry, the whole scalar sector collapses to $m_alpha = m_{3/2}$, $M_a = pm sqrt{3},m_{3/2}$, $A_{alpha beta gamma} = -M_a$ and $B = 2m_{3/2}$, with $hatmu = m_{3/2}$ in orbifolds where the $mu$ term comes from a Kähler bilinear $Z H_1 H_2$. For orbifold models with mixed dilaton/moduli breaking the authors derive a three-scalar sum rule, $m_alpha^2 + m_beta^2 + m_gamma^2 le |M_a|^2 = 3 m_{3/2}^2 sin^2 theta$, and show that the Higgs potential of the untwisted orbifold sector takes the factorized form $V_2 = Bhatmu (hatH_1 + hatH_2^*)(hatH_1^* + hatH_2)$, forcing $tan beta = -1$ at the string scale independently of the goldstino direction.
Load-bearing premise
The whole superstring prediction rests on supersymmetry being broken only by the $F$-terms of the dilaton and moduli, with the factorized Kähler potential of Eq. (44) and no D-term contribution; add another hidden field or a D-term and the universal pattern and its mass ratios no longer follow.
Editorial extensions
If this is right
- If dilaton domination holds, the entire soft spectrum is fixed by the single number $m_{3/2}$, giving sharp low-energy ratios for gluino, squark and slepton masses of roughly $1 : 0.94 : 0.92 : 0.92 : 0.32 : 0.24$.
- In orbifolds with mixed dilaton/moduli breaking, the sum rule forces boundary-scale scalar masses below gaugino masses, so at the weak scale sleptons end up lighter than squarks and gluinos, qualitatively resembling the dilaton-dominated spectrum.
- The $mu$ problem is solved without new physics: a bilinear term $Z H_1 H_2$ in the Kähler potential with $Z = 1/[(T_3+T_3^*)(U_3+U_3^*)]$ generates $hatmu = m_{3/2}$ and $B = 2m_{3/2}$ in the dilaton limit.
- The untwisted orbifold Higgs potential is fixed to the form $Bhatmu(hatH_1+hatH_2^*)(hatH_1^*+hatH_2)$, so $tan beta = -1$ at the superstring scale for any goldstino direction.
- The authors report that these boundary conditions are not consistent with the measured top-quark mass under radiative electroweak breaking, and that the dilaton-dominated limit is also excluded by bounds on charge- and colour-breaking minima, so viable mixed breaking must be dominantly moduli-driven.
Reading between the lines
- Because the soft terms are read directly off the Kähler potential and gauge kinetic function, any compactification with a known low-energy Kähler potential yields a parameter-free spectrum; this makes the soft-term computation a practical bridge between string model building and collider measurements rather than a formal exercise.
- The failure of the dilaton limit on the top mass can be read as a constraint on the goldstino direction rather than on the framework as a whole — in this language, a measured squark-to-gluino mass ratio would pin the angle $theta$ and discriminate dilaton from moduli domination.
- The three-scalar sum rule is a boundary-scale statement and is washed out by gaugino loop running, so a low-energy measurement of the three scalar masses entering a single Yukawa coupling cannot test it directly; only the pattern of sleptons, which feel no gluino loops, retains memory of the boundary condition.
- The outlook notes that S-duality and M-theory modify the dilaton Kähler potential, which suggests the universal predictions are an artifact of the perturbative heterotic tree-level limit and should be expected to shift once non-perturbative corrections are included.
Original abstract
We review the origin of soft supersymmetry-breaking terms in N=1 supergravity models of particle physics. We first consider general formulae for those terms in general models with a hidden sector breaking supersymmetry at an intermediate energy scale. The results for some simple models are given. We then consider the results obtained in some simple superstring models in which particular assumptions about the origin of supersymmetry breaking are made. These are models in which the seed of supersymmetry breaking is assumed to be originated in the dilaton/moduli sector of the theory.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
We review the origin of soft supersymmetry-breaking terms in N=1 supergravity models of particle physics. We first consider general formulae for those terms in general models with a hidden sector breaking supersymmetry at an intermediate energy scale. The results for some simple models are given. We then consider the results obtained in some simple superstring models in which particular assumptions about the origin of supersymmetry breaking are made. These are models in which the seed of supersymmetry breaking is assumed to be originated in the dilaton/moduli sector of the theory.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We review the origin of soft supersymmetry-breaking terms in N=1 supergravity models of particle physics. | contribution 0.80 | 0.35 | 0.06 | asserted 0.62 |
| s1 | We first consider general formulae for those terms in general models with a hidden sector breaking supersymmetry at an intermediate energy scale. | method 0.55 | 0.52 | 0.04 | asserted 0.78 |
| s2 | The results for some simple models are given. | result 0.48 | 0.72 | 0.05 | asserted 0.92 |
| s3 | We then consider the results obtained in some simple superstring models in which particular assumptions about the origin of supersymmetry breaking are made. | contribution 0.82 | 0.43 | 0.06 | asserted 0.97 |
| s4 | These are models in which the seed of supersymmetry breaking is assumed to be originated in the dilaton/moduli sector of the theory. | method 0.64 | 0.09 | 0.05 | asserted 0.92 |
What was examined, and what was not
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References
How later papers used it
95 later papers cite it
6 later papers by other authors are listed below: 6 used its method or tool.
Uses its method or tool 6 of 12 papers with this label
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Applied the supergravity formulae of this paper, assuming shift symmetry, to give the normalized soft Higgs masses.
The Higgs mass from a String-Theoretic Perspective (2013) · 0.95 · paraphrased: the licence does not allow quoting
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Used this paper's standard expressions for the scalar masses, trilinear A-terms and the B-term to derive the rest of the soft terms.
Global Fits of the Large Volume String Scenario to WMAP5 and Other Indirect Constraints Using Markov Chain Monte Carlo (2008) · 0.94 · paraphrased: the licence does not allow quoting
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Computed the masses of the unnormalized scalars from this paper's general expression.
Kahler Independence of the G2-MSSM (2008) · 0.84 · paraphrased: the licence does not allow quoting
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Used the formalism from this paper to compute the soft supersymmetry breaking masses on magnetized D7-branes wrapping the small cycle.
A Flux-Scaling Scenario for High-Scale Moduli Stabilization in String Theory (2015) · 0.96 · paraphrased: the licence does not allow quoting
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Computed the universal tree-level contribution to the gaugino masses as given by this paper.
Supersymmetry Breaking, Moduli Stabilization and Hidden U(1) Breaking in M-Theory (2011) · 0.85 · paraphrased: the licence does not allow quoting
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Took the general expressions for the un-normalized scalar masses and trilinear parameters from this paper.
The $G_2$-MSSM - An $M$ Theory motivated model of Particle Physics (2008) · 0.81 · paraphrased: the licence does not allow quoting
How the literature uses it
92 arXiv papers cite this in 132 sentences
Papers citing it · 79 sentences without a confident label
Uses its method or tool 12 papers
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Hence, assuming also shift symmetry and applying the supergravity formulae of [ref] , the normalized soft Higgs masses are simply given by [equation] The mass of the heavy Higgs doublet is therefore set to $m_S^2= 4 m_3/2^2 .$
The Higgs mass from a String-Theoretic Perspective · Bulk Higgs vs. intersection-curve Higgs · 0.95
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Using [ref] and the standard supergravity formulae [ref] it is easy to verify that a series of cancellations leads to the following result for the soft terms of the MSSM fields (not yet canonically normalized, which we emphasize with the hats): M̂^2_a b̅ = 2/3 V_0/M_Pl^2 K̃_ab̅ ≃0 , Â_abc = e^K/2 F^m ∂_m Y_a b c , Bμ̂ = e^K/2 M_Pl^2 μ[F^m (∂_mlogμ-W_m/3 W)]+μV_0/3W+𝒪(Z) , where $V_0$ is the vacuum energy at the minimum of the F-term potential, which we are assuming is negligibly small, and $𝒪(Z)$ stands for terms proportional to $Z$ and its derivatives, which we omit for simplicity.
Sequestering in String Compactifications · Sort-of sequestering · 0.92
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To derive the rest of the soft terms we use following standard expressions for the scalar masses, trilinear $A$-terms and the $B$-term [ref] : [equation] where $K̃_αβ̅ = K̃_α δ_αβ̅$ ( without summing over $α$) is the matter field metric.
Global Fits of the Large Volume String Scenario to WMAP5 and Other Indirect Constraints Using Markov Chain Monte Carlo · Soft Terms · 0.94
Uses its data or values 1 paper
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From [ref] we know that the moduli vevs are approximately $⟨s ⟩∼0.1 m_pl$, $⟨F_s ⟩∼m_1/2 m_pl$ and from the standard supergravity Lagrangian [ref] we get an effective $μ$-term: μ= ⟨m_3/2 K_H_u H_d - F^k K_H_u H_d k ⟩, which leads to μ∼⟨s ⟩/m_pl m_3/2 + ⟨F_s ⟩/m_pl .
SO(10) Grand Unification in M theory on a G2 manifold · $SU(5)$ · 0.97
Cites it as support 2 papers
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These have been studied extensively by [ref] (and references therein) who find that whenever the manifold is not pure no-scale i.e. $K^Φ_iΦ_j^†K_Φ_iK_Φ_j^†3$ the soft masses are always of order $m_3/2$ and so one can conclude that these models do not evade the supergravity breaking constraints.
Astrophysical Tests of Modified Gravity · No-Scale-Type Models · 0.97
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The assumption that the third generation squarks are heavier than those of the first two generations, a hierarchy which appears naturally in the quark and lepton sectors in the SM, can be theoretically implemented in the effective theory of superstring models [ref] .
Hunting Squarks in Higgsino LSP scenarios at the LHC · Introduction · 0.97
Cites it as background 36 papers
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On the other hand, the VCMSSM [ref] imposes the supplementary constraint $B_0 = A_0 - m_0$ on the CMSSM, thereby removing $$ as a free input and leaving three parameters, on which the further constraint $m_3/2 = m_0$ in mSUGRA [ref] imposes a severe restriction.
Implications of Initial LHC Searches for Supersymmetry · Introduction · 0.89
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These have been worked out for heterotic vacua [ref] (see e.g. Ref. [ref] for a review and further references) and generalized for the more recent case of Type II orientifold compactifications [ref] .
A 119-125 GeV Higgs from a string derived slice of the CMSSM · Introduction · 0.82
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As a starting point it is beneficial to recall the geometric or field theoretic origin of the shift symmetry within the orbifold constructions of [ref] as discussed in [ref] .
A Shift Symmetry in the Higgs Sector: Experimental Hints and Stringy Realizations · Introduction and Summary · 0.99
Discussion
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