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Minimal Left-Right Symmetric Model (mLRSM)

Updated 9 July 2026
  • mLRSM is a framework that extends the Standard Model by placing left- and right-handed fermions in analogous gauge multiplets and restoring parity at high energy.
  • It employs a bidoublet and triplet scalar sector to spontaneously break symmetry, generating heavy right-handed neutrino masses and realizing both type-I and type-II seesaw mechanisms.
  • The model offers concrete predictions for collider signals, low-energy observables, and cosmological phenomena such as leptogenesis and potential dark matter candidates.

The minimal Left-Right Symmetric Model (mLRSM) is a class of non-supersymmetric extensions of the Standard Model based on SU(3)c×SU(2)L×SU(2)R×U(1)BLSU(3)_c\times SU(2)_L\times SU(2)_R\times U(1)_{B-L}, or, in some electroweak-focused treatments, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}. Its defining idea is that left- and right-handed fermions are placed in analogous gauge multiplets and that parity PP or charge conjugation CC is restored at high energy and broken spontaneously. In the canonical formulation, the scalar sector contains a bidoublet Φ\Phi and triplets ΔL,ΔR\Delta_L,\Delta_R; ΔR0\langle \Delta_R^0\rangle breaks SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}, generates heavy right-handed neutrino masses, and gives rise to heavy gauge bosons WRW_R and ZRZ_R, while SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}0 generates electroweak symmetry breaking and Dirac fermion masses. The same structure underlies the type-I and type-II seesaw mechanisms, doubly charged scalars, right-handed currents, and a broad phenomenology spanning flavor physics, neutrinoless double beta decay, collider searches, leptogenesis, and dark matter model building (Dekens et al., 2021, Belfkir et al., 2023, Senjanovic et al., 2018).

1. Gauge principle and discrete left-right symmetry

In the canonical mLRSM, quarks and leptons occur in left- and right-handed doublets,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}1

with the standard assignments SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}2, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}3, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}4, and SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}5. Electric charge is fixed by

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}6

Because SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}7 is gauged, right-handed neutrinos are not optional; they are part of the gauge construction itself (Belfkir et al., 2023, Dekens et al., 2021, Borah et al., 2016).

The discrete left-right symmetry is implemented either as generalized parity SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}8 or generalized charge conjugation SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}9. Under PP0,

PP1

while under PP2,

PP3

These choices have direct consequences for the Yukawa sector: in the PP4-symmetric case the bidoublet Yukawas are Hermitian and PP5, whereas in the PP6-symmetric case they are symmetric and PP7 (Zhang et al., 2020, Chen et al., 4 Mar 2026).

A recurrent theme in the literature is that parity is exact only above the left-right breaking scale. After spontaneous breaking, the low-energy theory retains specific remnants of the high-energy symmetry. In the parity-symmetric mLRSM, for example, the right-handed CKM matrix is not independent; in the limit PP8, one has

PP9

with diagonal sign matrices CC0 and CC1. This relation is central to low-energy fits and to the predictivity of right-handed current phenomenology (Dekens et al., 2021).

2. Symmetry breaking and neutrino-mass structure

The canonical scalar sector contains

CC2

with

CC3

The vacuum structure is typically written as

CC4

with CC5 and CC6 tiny. The first stage,

CC7

is driven by CC8, and the second stage is electroweak breaking through the bidoublet vevs (Belfkir et al., 2023, Dekens et al., 2021, Kakoti et al., 2023).

Neutrino masses arise from the full CC9 neutral-fermion mass matrix,

Φ\Phi0

with Φ\Phi1 from Φ\Phi2, Φ\Phi3 from Φ\Phi4, and Φ\Phi5 from the bidoublet. In the seesaw limit one obtains

Φ\Phi6

or, in the notation frequently used in the literature,

Φ\Phi7

Thus the mLRSM realizes the type-II and type-I seesaw mechanisms in the same renormalizable gauge framework (Senjanovic et al., 2018, Zhang et al., 2020, Borah et al., 2016).

A distinctive property of the mLRSM is that the left-right symmetry constrains the Dirac sector strongly enough to reduce or remove the usual Casas–Ibarra ambiguity. In the Φ\Phi8-symmetric case, Φ\Phi9 is symmetric and can be written in terms of ΔL,ΔR\Delta_L,\Delta_R0 and ΔL,ΔR\Delta_L,\Delta_R1; in the type-I limit,

ΔL,ΔR\Delta_L,\Delta_R2

In the ΔL,ΔR\Delta_L,\Delta_R3-symmetric case, ΔL,ΔR\Delta_L,\Delta_R4 is Hermitian, and the mLRSM program described as “disentangling seesaw” shows that the Dirac mass matrix can be reconstructed analytically from light and heavy neutrino masses and mixings in the parity-conserving Yukawa limit. When parity is broken spontaneously, only the Hermitian part of ΔL,ΔR\Delta_L,\Delta_R5 remains independent, which still substantially reduces parameter freedom relative to the Standard Model seesaw (Senjanovic et al., 2018, Zhang et al., 2020).

The same structure persists in flavor-extended versions. In the modular ΔL,ΔR\Delta_L,\Delta_R6 realization, for example, the Yukawa couplings are replaced by modular forms ΔL,ΔR\Delta_L,\Delta_R7, the charged-lepton matrix is diagonal in the chosen basis, and both type-I and type-II dominant limits remain viable. In that construction the light-neutrino mass matrix is again organized as

ΔL,ΔR\Delta_L,\Delta_R8

with the same left-right logic but a different flavor origin (Kakoti et al., 2023).

3. Gauge and Higgs spectra

The breaking scale ΔL,ΔR\Delta_L,\Delta_R9 generates a heavy right-handed gauge sector. Across the literature, ΔR0\langle \Delta_R^0\rangle0 and ΔR0\langle \Delta_R^0\rangle1 masses are proportional to ΔR0\langle \Delta_R^0\rangle2, and the canonical triplet model often quotes

ΔR0\langle \Delta_R^0\rangle3

The same symmetry breaking also produces an extended Higgs sector containing neutral, singly charged, and doubly charged scalars (Heeck et al., 2015, Senjanovic et al., 2018).

The doubly charged states are especially characteristic. They arise as unavoidable components of ΔR0\langle \Delta_R^0\rangle4 and ΔR0\langle \Delta_R^0\rangle5, not as isolated additions: ΔR0\langle \Delta_R^0\rangle6 Their Yukawa couplings to leptons are directly tied to the neutrino sector, and in the ΔR0\langle \Delta_R^0\rangle7 realization one has ΔR0\langle \Delta_R^0\rangle8, with

ΔR0\langle \Delta_R^0\rangle9

In the collider regime where flavor-violating bidoublet scalars are heavy, the dominant decays are

SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}0

with partial width

SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}1

where SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}2 for identical leptons and SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}3 otherwise (Belfkir et al., 2023).

The neutral and singly charged states are constrained by flavor physics. In the triplet mLRSM, the FCNC-sensitive scalars SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}4 and SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}5 are typically taken at SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}6, SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}7, or SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}8 TeV to suppress flavor-changing neutral currents. This feeds directly into the doubly charged sector. A representative result is that for

SU(2)R×U(1)BLSU(2)_R\times U(1)_{B-L}9

the lowest possible mass of WRW_R0 is WRW_R1 GeV, whereas no unavoidable lower bound exists for WRW_R2 because its mass depends on the essentially free parameter WRW_R3 (Bambhaniya et al., 2014).

Collider studies reflect this structure. At the 14 TeV LHC, pair-produced doubly charged scalars yield clean same-sign dilepton signatures, and multilepton analyses in the MLRSM find that tri-lepton and four-lepton signals can be detected with WRW_R4 for doubly charged Higgs bosons up to approximately WRW_R5 GeV. At future hadron colliders, the heavy Higgs sector can be probed much more deeply; a conservative estimate in the TeV-scale type-I left-right seesaw setting gives sensitivity up to WRW_R6 TeV at a 100 TeV machine (Bambhaniya et al., 2013, Dev et al., 2016).

Muon-collider studies sharpen this program for the doubly charged sector. For a WRW_R7 collider at WRW_R8 TeV and WRW_R9, with ZRZ_R0 TeV, the channel

ZRZ_R1

is particularly clean, and the mixed final state ZRZ_R2 has the largest sensitivity because it is nearly background-free. Fully polarized initial muon beams can enhance the ZRZ_R3 signal by about a factor of 4 relative to ZRZ_R4 for a ZRZ_R5 TeV state and can roughly double the sensitivity in some cases (Belfkir et al., 2023).

Not every scalar-sector anomaly can be accommodated. In the specific analysis of the 750 GeV diphoton excess, the canonical minimal model admits a candidate ZRZ_R6, but the production is mixing-suppressed and the loop-induced ZRZ_R7 branching ratio is too small; even after including charged-scalar and ZRZ_R8 loops, the maximal ZRZ_R9 remains below SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}00 fb, far below the then-required SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}01 fb (Dasgupta et al., 2015).

4. Low-energy observables, flavor, and lepton-number violation

Low-energy precision observables are among the sharpest probes of the mLRSM. A global analysis of the parity-symmetric model matched to SMEFT and then to low-energy effective operators includes mesonic, neutron, and nuclear SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}02 decay, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}03 and SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}04 observables in the strange and bottom sectors, and EDMs of nucleons, nuclei, and atoms. In the version with a Peccei–Quinn solution to the strong CP problem, this fit yields

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}05

while in the SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}06-symmetric model without a Peccei–Quinn mechanism the corresponding bound is

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}07

The same analysis requires the additional scalar fields to be a few times heavier than the right-handed gauge bosons. It also finds that TeV-scale SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}08 bosons can alleviate some tension in first-row CKM unitarity tests, but a full solution is disfavored once other observables are included (Dekens et al., 2021).

In the SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}09-symmetric case, the strong-CP sector is tightly correlated with spontaneous symmetry breaking. After symmetry breaking,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}10

and the neutron EDM bound implies

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}11

This relation explains why EDM data dominate the no-PQ fit and why the phenomenology differs sharply between PQ and non-PQ realizations (Dekens et al., 2021).

Neutrinoless double beta decay is another central diagnostic. In the mLRSM the relevant amplitudes are not independent because the same seesaw mechanism ties together SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}12, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}13, and active-heavy mixing. The standard classification distinguishes the SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}14, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}15, and SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}16 channels. A general analysis shows that, if no fine-tuned cancellation is involved in the light-neutrino contribution, a new-physics-dominated signal is expected mainly from the SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}17 channel. An important exception occurs when the right-handed neutrino spectrum is hierarchical,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}18

in which case the SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}19 channel can dominate (Huang et al., 2013).

Allowing both type-I and type-II seesaw contributions changes the viable parameter space substantially. In the general type-I+II analysis of SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}20, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}21, and SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}22, the mLRSM admits more allowed parameter space than the pure type-I or pure type-II limits, and the doubly charged scalar masses SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}23 are allowed to be smaller than the heaviest right-handed neutrino mass SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}24, contrary to earlier expectations based on individual seesaw dominance (Borah et al., 2016).

A particularly constrained corner of parameter space emerges in the type-II seesaw limit with negligible left-right mixing. There, a sub-GeV sterile neutrino can survive all current collider, meson-decay, supernova, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}25, and cosmological constraints only in a narrow window: SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}26 In that study, the use of effective-field-theory SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}27 amplitudes together with updated nuclear matrix elements makes future tonne-scale SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}28 searches the exclusive probe of the remaining corridor (Li et al., 21 Aug 2025).

5. Cosmological applications: baryogenesis and dark matter

The mLRSM is frequently used as a predictive setting for thermal leptogenesis because left-right symmetry fixes much of the neutrino Dirac sector. In the regime where left-right symmetry remains unbroken in the lepton Yukawa sector, the neutrino Dirac matrix is determined by neutrino masses, heavy-neutrino masses, and the lepton mixing matrix SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}29, so the CP phases needed for leptogenesis can reside entirely in the low-energy PMNS sector. Numerical Boltzmann analyses in the thermal unflavored regime,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}30

find that the observed baryon asymmetry SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}31 is achievable in both type-I-dominated and mixed type-I+II scenarios, for both heavy-neutrino decay and triplet-decay leptogenesis, and that in several cases the Dirac phase SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}32 alone can generate the correct magnitude and sign (Zhang et al., 2020).

A later parity-based analysis sharpened this statement. With generalized parity, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}33, and if the right-handed mixing matrix SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}34 is taken real, the hermiticity constraints favor CP-conserving Majorana phases,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}35

so that SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}36 becomes the sole source of asymmetry. In that setting all four standard leptogenesis scenarios can reproduce the observed baryon asymmetry in specific regions of parameter space, with strong dependence on the neutrino mass ordering and the lightest neutrino mass (Chen et al., 4 Mar 2026).

Dark-matter model building in the mLRSM proceeds along several distinct tracks. A minimal extension by fermion multiplets

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}37

with triplet SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}38 and quintuplet SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}39 cases emphasized, yields stable TeV-scale dark matter without any ad hoc stabilizing symmetry. Stability comes either from the remnant

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}40

under which all fermions are odd and all bosons are even, or from accidental stability in the Minimal Dark Matter sense. Because left-right exchange symmetry enforces a common Majorana mass SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}41, this construction introduces only one new free parameter. For the canonical mass relation SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}42, the observed relic abundance can be reproduced for TeV-scale masses provided roughly

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}43

(Heeck et al., 2015).

A more economical but highly tuned alternative uses no new fields at all and identifies the dark matter candidate with the neutral real component of the right-handed triplet,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}44

This scenario requires an extreme hierarchy

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}45

together with

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}46

suppressed scalar mixing, and typically

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}47

to satisfy X-ray bounds. The construction is described as fully minimal because no new fields are added, but it is also explicitly described as somewhat fine-tuned (Dev et al., 24 Jan 2025).

The thermal history of right-handed neutrino dark matter can require entropy dilution. A systematic study of diluted dark matter in the mLRSM finds that the spontaneous left-right breaking scale must be above PeV to accommodate the observed relic abundance in generic cases, and that cosmology provides the most sensitive probes of the scenario. When the dilutor is a heavier right-handed neutrino, it can be much lighter and lie near the electroweak scale, but large-scale-structure constraints on energetic secondary dark matter impose

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}48

This makes the viable parameter space highly structured (Nemevšek et al., 2023).

Inflationary extensions can also be formulated within left-right symmetry. In the spontaneous SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}49-parity-breaking construction, a parity-odd singlet SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}50 plays the role of the inflaton, parity breaking occurs at roughly SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}51 GeV, and the induced left-triplet vev obeys

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}52

For the sample parameter choice

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}53

the model gives

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}54

That work explicitly connects inflationary observables, neutrino masses, and leptogenesis within the left-right framework (0705.0068).

6. Variants, scope of “minimality,” and ongoing interpretation

A persistent source of confusion is that the designation mLRSM is not used for a single universal scalar sector. The literature contains several closely related constructions, each called minimal because it adopts the smallest field content compatible with a specific symmetry-breaking pattern, neutrino-mass mechanism, or ultraviolet realization. This usage suggests that “minimality” in left-right symmetry is objective-dependent rather than unique (Siringo, 2012, 0911.0710, Anchordoqui et al., 2016).

Realization Defining content Characteristic consequence
Canonical triplet mLRSM SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}55, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}56, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}57 Type-I+II seesaw; doubly charged scalars; SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}58
Simplest non-supersymmetric doublet model SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}59, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}60, no bidoublet With one intermediate scale, SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}61 GeV and heavy gauge bosons above SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}62 TeV
Classically conformal doublet version Bidoublet SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}63 plus SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}64, no mass terms at tree level Coleman–Weinberg breaking can generate a few-TeV left-right scale
Spontaneous SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}65-parity-breaking version Parity-odd singlet SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}66 plus SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}67 Separates parity breaking from SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}68 breaking and supports inflation
Intersecting D-brane realization SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}69, bi-doublet plus SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}70 doublets Neutrinos are Dirac at renormalizable level; SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}71 above about SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}72 TeV not ruled out
Modular SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}73 realization Canonical LR gauge sector with SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}74 modular symmetry No flavons; Yukawas arise from modular forms

The simplest non-supersymmetric doublet model is especially distinct. It contains only two scalar doublets SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}75 and SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}76, no bidoublet, and treats the parity-breaking scale SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}77 as the only intermediate threshold between the electroweak scale and unification. In a one-loop analysis with measured low-energy couplings, this yields

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}78

that is,

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}79

with an almost sterile right-handed neutrino around SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}80 TeV below that scale (Siringo, 2012).

The classically conformal version instead removes explicit mass terms from the scalar potential and generates scales through radiative symmetry breaking. In a representative numerical example it gives

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}81

where SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}82 is the scalon. That framework emphasizes dimensional transmutation and the possibility that electroweak symmetry breaking is triggered by left-right breaking (0911.0710).

The intersecting D-brane construction changes the scalar logic more radically. Because SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}83 triplets with SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}84 are not available in the minimal open-string setup, left-right breaking uses SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}85 doublets with SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}86 rather than triplets. Majorana masses are then suppressed by higher-dimensional effects, neutrinos are Dirac at renormalizable level, and the model predicts a SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}87 with comparable leptonic and hadronic branching fractions. In that setup, gauge bosons with masses

SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}88

are not ruled out independent of SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}89 (Anchordoqui et al., 2016).

The modular-symmetric mLRSM retains the canonical gauge and scalar structure but replaces flavons by modular forms. In that realization SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}90 to SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}91, both type-I and type-II dominance are viable, and the predicted sums of neutrino masses remain within current cosmological bounds. This line of work preserves the usual triplet-based seesaw while minimizing the flavor sector (Kakoti et al., 2023).

Taken together, these variants delimit the modern meaning of the mLRSM. In one sense, the term refers narrowly to the bidoublet-plus-triplets theory that underlies most collider, flavor, and neutrino analyses. In a broader sense used across the literature, it denotes the smallest left-right-symmetric completion compatible with a chosen ultraviolet or phenomenological requirement. The resulting theory space is unified by gauged SU(2)L×SU(2)R×U(1)BLSU(2)_L\times SU(2)_R\times U(1)_{B-L}92, right-handed weak interactions, and spontaneous breaking of left-right symmetry, but not by a single universally accepted minimal scalar content (Dekens et al., 2021, Siringo, 2012, Anchordoqui et al., 2016).

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