20 double BR_mu_e_gamma = (alph*pow(mMU,5) * ((*(allcoeff_me[
LO])) * (*(allcoeff_me[
LO])).conjugate()).abs() / (2.99598e-19) );
33 double BR_mu_e_gamma = (alph*pow(mMU,5) * ((*(allcoeff_me[
LO])) * (*(allcoeff_me[
LO])).conjugate()).abs() / (2.99598e-19) );
34 return log10(BR_mu_e_gamma);
46 double BR_mu_e_gamma = (alph*pow(mMU,5) * ((*(allcoeff_me[
LO])) * (*(allcoeff_me[
LO])).conjugate()).abs() / (2.99598e-19) );
47 double BR_mu_e_gamma_obs=4.2e-13;
48 double BR_mu_e_gamma_exp=5.3e-13;
49 double ntos=1.64485362695147;
51 return (1+(BR_mu_e_gamma-BR_mu_e_gamma_obs)/BR_mu_e_gamma_exp)*ntos;
63 double BR_tau_mu_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_tm[
LO])) * (*(allcoeff_tm[
LO])).conjugate()).abs() / (2.26735e-12) );
64 return BR_tau_mu_gamma;
76 double BR_tau_mu_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_tm[
LO])) * (*(allcoeff_tm[
LO])).conjugate()).abs() / (2.26735e-12) );
77 return log10(BR_tau_mu_gamma);
89 double BR_tau_mu_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_tm[
LO])) * (*(allcoeff_tm[
LO])).conjugate()).abs() / (2.26735e-12) );
90 double BR_tau_mu_gamma_obs=4.4e-8;
91 double BR_tau_mu_gamma_exp=8.2e-8;
92 double ntos=1.64485362695147;
94 return (1+(BR_tau_mu_gamma-BR_tau_mu_gamma_obs)/BR_tau_mu_gamma_exp)*ntos;
106 double BR_tau_mu_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_tm[
LO])) * (*(allcoeff_tm[
LO])).conjugate()).abs() / (2.26735e-12) );
107 double BR_tau_mu_gamma_obs=1.0e-9;
108 double BR_tau_mu_gamma_exp=1.0e-9;
109 double ntos=1.64485362695147;
111 return (1+(BR_tau_mu_gamma-BR_tau_mu_gamma_obs)/BR_tau_mu_gamma_exp)*ntos;
123 double BR_tau_e_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_te[
LO])) * (*(allcoeff_te[
LO])).conjugate()).abs() / (2.26735e-12) );
124 return BR_tau_e_gamma;
136 double BR_tau_e_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_te[
LO])) * (*(allcoeff_te[
LO])).conjugate()).abs() / (2.26735e-12) );
137 return log10(BR_tau_e_gamma);
149 double BR_tau_e_gamma = (alph*pow(mTAU,5) * ((*(allcoeff_te[
LO])) * (*(allcoeff_te[
LO])).conjugate()).abs() / (2.26735e-12) );
150 double BR_tau_e_gamma_obs=3.3e-8;
151 double BR_tau_e_gamma_exp=9.8e-8;
152 double ntos=1.64485362695147;
154 return (1+(BR_tau_e_gamma-BR_tau_e_gamma_obs)/BR_tau_e_gamma_exp)*ntos;
gslpp::vector< gslpp::complex > ** ComputeCoeffli_lj_gamma(int li_lj)
Computes the Wilson coefficient for the process .
const double & getMass() const
A get method to access the particle mass.
Robs_mu_e_gamma(const StandardModel &SM_i)
Calculates the upper limit ratio of the process .
Robs_tau_e_gamma(const StandardModel &SM_i)
Calculates the upper limit ratio of the process .
Robs_tau_mu_gamma_BelleII(const StandardModel &SM_i)
Calculates the upper limit ratio of the process .
Robs_tau_mu_gamma(const StandardModel &SM_i)
Calculates the upper limit ratio of the process .
A model class for the Standard Model.
const Particle & getLeptons(const QCD::lepton p) const
A get method to retrieve the member object of a lepton.
LeptonFlavour * getMyLeptonFlavour() const
const double getAle() const
A get method to retrieve the fine-structure constant .
A class for a model prediction of an observable.
const StandardModel & SM
A reference to an object of StandardMode class.
log_meg(const StandardModel &SM_i)
Calculates the value of the process .
log_teg(const StandardModel &SM_i)
Calculates the value of the process .
log_tmg(const StandardModel &SM_i)
Calculates the value of the process .
mu_e_gamma(const StandardModel &SM_i)
Calculates the value of the process .
tau_e_gamma(const StandardModel &SM_i)
Calculates the value of the process .
tau_mu_gamma(const StandardModel &SM_i)
Calculates the value of the process .