REVIEW
Solitons in the supersymmetric extensions of the Standard Model
High Energy Physics - Phenomenology · Submitted 9 Apr 1997 · 16 references
Pith's verdict: The trilinear-coupling argument for generic MSSM Q-balls is correct and consequential; the gaps are mostly expositional, except for the cosmology, which is deferred to an in-preparation paper.
T0 · AI review
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Referee report
The paper
The paper claims
Every supersymmetric version of the Standard Model contains stable Q-balls: lumps of squark and slepton field that carry baryon number, lepton number, or electric charge.
The reading
What carries the argument
The carrying object is the multi-flavor Q-ball: a coherent lump of several charged scalar fields rotating in their internal $U(1)$ with angular velocities proportional to their charges. Its existence is decided by Coleman's criterion, the requirement that $2U(phi)/sum_k q_k phi_k^2$ have a minimum at nonzero field, and its shape is the three-dimensional Euclidean bounce of the effective potential $hat{U}_omega$ obtained by Legendre transforming on the charge. The mechanism that does the work in the MSSM is the tri-linear coupling $yA H_1 Phi varphi$ between the Higgs and a left-handed squark or slepton doublet together with its right-handed singlet; a cubic term of either sign in the potential makes the ratio fall away from the origin, so the criterion is satisfied for arbitrarily small coupling strength.
Extended reading notes
Core claim
The paper's claim is that non-topological solitons with nonzero baryon number, lepton number, and electric charge are generic to supersymmetric extensions of the Standard Model, not special to particular parameter choices. The derivation runs through Coleman's existence condition, which requires that $2U(1, ...)/8$ be minimized at some nonzero field configuration; the paper generalizes this to several fields with different charges and shows that the fields in the soliton rotate in internal space with velocities proportional to their charges, $phi_k(x,t) = e^{i q_k omega t} phi_k(x)$. Minimizing the energy at fixed charge then reduces to finding a bounce in the modified potential $hat{U}_omega(phi) = U(phi) - (1/2)omega^2 sum_k q_k^2 |phi_k|^2$ in three Euclidean dimensions. For large charge the soliton is a thin-walled ball with mass $M_Q = Q sqrt{2U(phi_0)/sum_k q_k phi_{k,0}^2}$, below the mass of the lightest constituent particle whenever the minimum is global, which is what makes it stable. For small charge the thin-wall picture fails and a thick-wall treatment gives Q-beads with masses and radii expanded in a small parameter; the paper states there is no classical lower bound on the charge. Applied to the MSSM, the tri-linear couplings $yA H_1 Phi varphi$ that every supersymmetric model must contain make the origin of the ratio unstable, so a stable soliton with a given lepton or baryon number always exists.
Load-bearing premise
The claim that every supersymmetric model contains these solitons rests on at least one squark or slepton having a nonzero tri-linear coupling, and on a simplified scalar potential that neglects the Higgs vacuum expectation value still capturing the relevant MSSM field content; the paper acknowledges both points and argues neither can fail in a realistic model.
Editorial extensions
If this is right
- Every supersymmetric extension of the Standard Model contains solitons carrying baryon number, lepton number, or electric charge, so their existence does not constrain model parameters the way a model-specific prediction would.
- Large B- and L-balls are stable against decay into their own scalar constituents but still evaporate slowly into quarks and leptons from their surface, at a rate set by the surface area rather than the volume because the interior fermion sea fills to the Fermi pressure.
- A Q-ball that survives down to temperatures of order the QCD scale leaves behind a bound lump of quark matter, so heavy nuclei of matter and antimatter with mass number of order the soliton charge can be present at the time standard nucleosynthesis begins.
- Small solitons of unit charge can be absolutely stable through combinations of conservation laws alone, for example an electrically neutral, SU(2)-singlet, spin-zero bead with lepton number one, making them candidates for dark matter.
- A soliton carrying both baryon and lepton number interacts as a leptoquark, which gives it a distinctive signature if such objects can ever be produced in a collider.
Reading between the lines
- The argument is a structural one: it says the soliton sector is a generic feature fixed by the symmetries and the presence of cubic couplings, so searching for these objects is a test of low-energy supersymmetry as a class rather than of any particular mass spectrum.
- If the beads really are stable dark matter, their number density is set by the same statistical fluctuation mechanism the paper cites for large balls, which suggests that the small-charge end of the spectrum, not the large-charge end, is where the cosmological abundance is decided.
- The quark-matter remnant picture implies that a population of evaporating solitons would leave a signature in the primordial abundance of heavy elements and in the light-element ratios, which is a place where an independent handle on the soliton abundance could come from.
- The paper's own caveat that quantum corrections can modify the semiclassical result at unit charge suggests that a lattice or functional computation of the Q=1 bead mass would be the sharpest way to test whether the dark-matter candidate survives.
Original abstract
All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons of the Q-ball type which may have non-zero baryon and lepton numbers, as well as the electric charge. These solitons can be produced in the early Universe, can affect the nucleosynthesis, and can lead to a variety of other cosmological consequences.
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
All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons of the Q-ball type which may have non-zero baryon and lepton numbers, as well as the electric charge. These solitons can be produced in the early Universe, can affect the nucleosynthesis, and can lead to a variety of other cosmological consequences.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons of the Q-ball type which may have non-zero baryon and lepton numbers, as well as the electric charge. | result 0.90 | 0.25 | 0.75 | asserted 0.63 |
| s1 | These solitons can be produced in the early Universe, can affect the nucleosynthesis, and can lead to a variety of other cosmological consequences. | interpretation 0.91 | 0.17 | 0.17 | hedged possibility 0.85 |
What was examined, and what was not
- arXiv listing abstract v2
- full text
- figures and tables
- references and citing sentences
- relations to other papers
- P abstract
- S sections
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References
How later papers used it
88 later papers cite it
4 later papers by other authors are listed below: 4 used its method or tool.
Uses its method or tool 4 of 5 papers with this label
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The Hamiltonian for this theory is [equation] To determine if this system admits Q-ball solutions, we introduce a Lagrange multiplier $ω$, as in Ref. [ref] , that enforces charge conservation upon minimisation with respect to it: [equation] where $j^0$ is the zeroth component of the Noether current density given in Eq. [ref].
Multi-Field Q-balls with Real Scalars (2021) · Minimising the Energy in a Sector of Fixed Charge · 0.99
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The Hamiltonian, coincident with the energy, for this theory is [equation] To determine the states with the lowest energy for a given charge, we employ the method of Ref. [ref] .
Non-Canonical Q-balls (2021) · The Minimisation Procedure · 1.00
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The Hamiltonian for this theory is [equation] To determine if this system admits Q-ball solutions, we introduce a set of Lagrange multipliers, ${ω_k}$, similar to Ref. [ref] , that each enforce charge conservation upon minimisation with respect to them: [equation] where $j^0_k$ is the zeroth component of the Noether current density associated to the $k$-th $U(1)$ symmetry given in Eq. [ref].
Q-balls with Multiple Charges and Cores (2022) · Minimising the Energy in a Sector of Fixed Charge · 0.96
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Used the method of Lagrange multipliers from this paper to minimize the total energy for a fixed Noether charge.
Higgs Assisted Q-balls from Pseudo-Nambu-Goldstone Bosons (2017) · 0.99 · paraphrased: the licence does not allow quoting
How the literature uses it
82 arXiv papers cite this in 123 sentences
Papers citing it · 66 sentences without a confident label
Builds on it 3 papers
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These results are readily generalised to models with multiple scalar fields using Ref. [ref] .
Solitonic supersymmetry restoration · Q-balls in metastable vacua · 0.96
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The thin-wall limit for multi-field Q-balls was first considered in Ref. [ref] for the case of one complex scalar and one real scalar.[It should be noted that in Ref. [ref] , the case of multiple charged scalars – and no real scalars – was analysed for thin-wall Q-balls.] For completeness, we include the analysis for multiple real scalars here.
Multi-Field Q-balls with Real Scalars · Thin-Wall Q-balls · 0.97
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In the multi-field case, an argument similar to the one around Efunctional indicates that we should seek a Q-ball solution of the form [ref] ϕ_I(x) = f_I(r) e^i q_I t , and the existence condition now is that min\(V(|f_I|)∑_I q_I f^2_I\) is reached at f_I ≠0 .
Non-topological solitons and quasi-solitons · Flat directions in MSSM · 0.98
Uses its method or tool 5 papers
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The Hamiltonian for this theory is [equation] To determine if this system admits Q-ball solutions, we introduce a Lagrange multiplier $ω$, as in Ref. [ref] , that enforces charge conservation upon minimisation with respect to it: [equation] where $j^0$ is the zeroth component of the Noether current density given in Eq. [ref].
Multi-Field Q-balls with Real Scalars · Minimising the Energy in a Sector of Fixed Charge · 0.99
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The Hamiltonian, coincident with the energy, for this theory is [equation] To determine the states with the lowest energy for a given charge, we employ the method of Ref. [ref] .
Non-Canonical Q-balls · The Minimisation Procedure · 1.00
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To search for the formation of Q-balls from the scalar field $φ$, one needs to find the solution that minimizes the energy [ref] [equation] where $ω$ is a Lagrangian multiplier, and $j^0$ is the time component of the Noether current of the field $φ$ defined in Eq. [ref], namely [equation]
A Unified Fermionic Origin for Density-Driven Waterfall Inflation and its Multi-Messenger Signatures · Q-balls from inflaton fragmentation · 0.84
Cites it as support 1 paper
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This has been confirmed by perturbative analysis as well as detailed numerical simulations [ref] .
PQ-ball and its Real Scalar Analogue in an Expanding Universe · Evolution of averaged field value · 0.97
Cites it as background 41 papers
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Another important consequence of the AD mechanism is the formation of Q-balls [ref] .
Lepton Asymmetric Universe · Lepton asymmetry from L-ball · 0.84
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In such regions, the oscillation of the AD field experiences spatial instabilities and fragments into non-topological solitons called Q-balls [ref] .
Supermassive black hole formation from Affleck-Dine mechanism with suppressed clustering on large scales · Introduction · 0.80
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Now we turn to the cosmological effect of Q balls [ref] , which are potential obstacles in this scenario.
Higgs, Moduli Problem, Baryogenesis and Large Volume Compactifications · Affleck-Dine baryogenesis in high-scale SUSY breaking · 0.93
Discussion
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