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Physlib.Particles.BeyondTheStandardModel.RHN.AnomalyCancellation.Ordinary.Basic

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definition

ACC system for the Standard Model with nn right-handed neutrinos

#SM

The definition SMRHN.SM(n)\text{SMRHN.SM}(n) constructs an Anomaly Cancellation Condition (ACC) system for the Standard Model (SM) extended by nn right-handed neutrinos (RHN), excluding hypercharge. This system is defined over the charge space V=SMνCharges(n)V = \text{SM}\nu\text{Charges}(n), which assigns rational charges to the standard fermions and the nn additional neutrinos. The system consists of: 1. Three linear anomaly cancellation equations: the gravitational anomaly (accGrav\text{accGrav}), the SU(2)SU(2) gauge anomaly (accSU2\text{accSU2}), and the SU(3)SU(3) gauge anomaly (accSU3\text{accSU3}). 2. Zero quadratic anomaly cancellation equations. 3. A single cubic anomaly cancellation equation (accCube\text{accCube}) corresponding to the U(1)U(1) cubic gauge anomaly.

theorem

The gravitational anomaly accGrav\text{accGrav} vanishes for linear solutions of SMRHN.SM(nn)

#gravSol

For any linear solution SS of the Anomaly Cancellation Condition (ACC) system for the Standard Model with nn right-handed neutrinos (without hypercharge), the gravitational anomaly cancellation condition accGrav\text{accGrav} evaluated on SS is satisfied, i.e., accGrav(S)=0\text{accGrav}(S) = 0.

theorem

accSU2(S)=0\text{accSU2}(S) = 0 for Linear Solutions in the SMRHN ACC System

#SU2Sol

For any linear solution SS of the anomaly cancellation system for the Standard Model with nn right-handed neutrinos (without hypercharge), the SU(2)SU(2) gauge anomaly equation accSU2\text{accSU2} evaluated at SS is zero.

theorem

Linear solutions in SMRHN satisfy accSU3=0\text{accSU3} = 0

#SU3Sol

In the anomaly cancellation condition (ACC) system for the Standard Model with nn right-handed neutrinos, let SS be a linear solution (a charge vector satisfying the linear anomaly equations). Then the SU(3)SU(3) gauge anomaly cancellation equation, denoted as accSU3\text{accSU3}, evaluates to zero for SS: accSU3(S)=0\text{accSU3}(S) = 0

theorem

Solutions to the SM with nn RHN satisfy the cubic anomaly equation accCube(S)=0\text{accCube}(S) = 0

#cubeSol

In the Anomaly Cancellation Condition (ACC) system for the Standard Model extended with nn right-handed neutrinos, let SS be a valid solution to the system (i.e., S(SM n).SolsS \in (\text{SM } n).\text{Sols}). Then, the U(1)U(1) cubic gauge anomaly cancellation equation accCube\text{accCube} evaluated at the charge assignment SS is equal to zero.

definition

Construction of a linear solution from charges satisfying accGrav\text{accGrav}, accSU2\text{accSU2}, and accSU3\text{accSU3}

#chargeToLinear

For the anomaly cancellation system (SM n)(SM \ n) representing the Standard Model with nn right-handed neutrinos, this function takes a charge assignment S(SM n).ChargesS \in (SM \ n).\text{Charges} and proofs that SS satisfies the three linear anomaly cancellation conditions (ACCs): 1. The gravitational anomaly: accGrav(S)=0\text{accGrav}(S) = 0 2. The SU(2)SU(2) gauge anomaly: accSU2(S)=0\text{accSU2}(S) = 0 3. The SU(3)SU(3) gauge anomaly: accSU3(S)=0\text{accSU3}(S) = 0 It returns SS as an element of (SM n).LinSols(SM \ n).\text{LinSols}, the space of charges that satisfy all linear ACCs in the system.

definition

Inclusion of linear solutions into quadratic solutions for (SM n)(SM \ n)

#linearToQuad

In the context of the Anomaly Cancellation Condition (ACC) system for the Standard Model with nn right-handed neutrinos (denoted as (SM n)(SM \ n)), this function maps a linear solution S(SM n).LinSolsS \in (SM \ n).\text{LinSols} to a quadratic solution S(SM n).QuadSolsS \in (SM \ n).\text{QuadSols}. A linear solution is a charge assignment that satisfies the gravitational, SU(2)SU(2), and SU(3)SU(3) anomaly cancellation equations. Because the (SM n)(SM \ n) system is defined with zero quadratic anomaly equations, any charge vector SS that satisfies the linear conditions is vacuously a solution to the quadratic conditions.

definition

Full solution from a quadratic solution satisfying accCube=0\text{accCube} = 0

#quadToAF

For the Standard Model with nn right-handed neutrinos, let SS be a vector of rational charges that satisfies the linear and quadratic anomaly cancellation conditions (ACCs). Given a proof hchc that SS also satisfies the cubic anomaly cancellation equation, accCube(S)=0\text{accCube}(S) = 0, this function constructs a complete anomaly-free solution S(SM n).SolsS \in (\text{SM } n).\text{Sols}.

definition

Construction of a quadratic solution from charges satisfying accGrav\text{accGrav}, accSU2\text{accSU2}, and accSU3\text{accSU3}

#chargeToQuad

For the anomaly cancellation system of the Standard Model with nn right-handed neutrinos (denoted (SM n)(SM \ n)), this function takes a charge assignment S(SM n).ChargesS \in (SM \ n).\text{Charges} and proofs that SS satisfies the three linear anomaly cancellation conditions (ACCs): 1. The gravitational anomaly: accGrav(S)=0\text{accGrav}(S) = 0 2. The SU(2)SU(2) gauge anomaly: accSU2(S)=0\text{accSU2}(S) = 0 3. The SU(3)SU(3) gauge anomaly: accSU3(S)=0\text{accSU3}(S) = 0 It returns SS as an element of (SM n).QuadSols(SM \ n).\text{QuadSols}, the space of charges satisfying both linear and quadratic ACCs. Since the (SM n)(SM \ n) system is defined with zero quadratic anomaly equations, any charge vector satisfying the linear conditions is vacuously a solution to the quadratic sector.

definition

Construction of an anomaly-free solution from charges satisfying linear and cubic ACCs

#chargeToAF

In the context of the Standard Model with nn right-handed neutrinos (without hypercharge), let S(SM n).ChargesS \in (\text{SM } n).\text{Charges} be a vector of rational charges. Given proofs that SS satisfies the three linear anomaly cancellation conditions—the gravitational anomaly accGrav(S)=0\text{accGrav}(S) = 0, the SU(2)SU(2) anomaly accSU2(S)=0\text{accSU2}(S) = 0, and the SU(3)SU(3) anomaly accSU3(S)=0\text{accSU3}(S) = 0—and the cubic anomaly cancellation condition accCube(S)=0\text{accCube}(S) = 0, this function constructs an element of (SM n).Sols(\text{SM } n).\text{Sols}, representing a complete anomaly-free solution. This construction utilizes the fact that the system has no quadratic anomaly constraints, so satisfying the linear and cubic conditions is sufficient for a full solution.

definition

Anomaly-free solution from a linear solution satisfying accCube=0\text{accCube} = 0

#linearToAF

In the context of the Anomaly Cancellation Condition (ACC) system for the Standard Model with nn right-handed neutrinos (denoted as (SM n)(\text{SM } n)), let SS be a linear solution (S(SM n).LinSolsS \in (\text{SM } n).\text{LinSols}). A linear solution is a charge assignment that satisfies the three linear anomaly equations: the gravitational anomaly, the SU(2)SU(2) gauge anomaly, and the SU(3)SU(3) gauge anomaly. Given a proof hchc that SS also satisfies the cubic anomaly cancellation equation accCube(S)=0\text{accCube}(S) = 0, this function constructs a complete anomaly-free solution S(SM n).SolsS \in (\text{SM } n).\text{Sols}. This construction is possible because the (SM n)(\text{SM } n) system has no quadratic anomaly constraints.

definition

Permutation group action on the ACC system SMRHN.SM(n)\text{SMRHN.SM}(n)

#perm

For a given number of right-handed neutrinos nNn \in \mathbb{N}, the definition SMRHN.SM.perm(n)\text{SMRHN.SM.perm}(n) constructs a group action of the permutation group (typically acting on fermion generations or the nn additional neutrinos) on the charge space of the Anomaly Cancellation Condition (ACC) system SMRHN.SM(n)\text{SMRHN.SM}(n). This action is shown to leave the four primary anomaly equations invariant: the three linear anomalies—gravitational (accGrav\text{accGrav}), SU(2)SU(2) (accSU2\text{accSU2}), and SU(3)SU(3) (accSU3\text{accSU3})—and the cubic U(1)U(1) anomaly (accCube\text{accCube}). Since there are no quadratic anomalies in this system, the invariance is trivially satisfied for that category.