Version 15 (modified by 2 years ago) ( diff ) | ,
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pSPSS
: Phenomenological symmetry protected seesaw scenario
The motivation and implementation of the pSPSS
is discussed in
- Antusch, J. Hajer, and J. Rosskopp. ‘Simulating lepton number violation caused by heavy neutrino-antineutrino oscillations at colliders’ (2022).
Please cite this publication when you use the pSPSS
model file.
Model description
The pSPSS
describes the interactions of a pseudo-Dirac pair of two Majorana degrees of freedom $N_1$
$N_2$
In the lepton number conserving (LNC) limit the interactions of the symmetry protected seesaw scenario (SPSS) with the Standard Model are
$\mathcal L_\text{SPSS}^L = \overline N_i \, i\!\! \not\! \partial N_i - y_{\alpha1} \widetilde H^\dagger \bar \ell_\alpha N_1^c - \overline N_1 m_M^{} N_2^c + \text{H.c.}$
The additional lepton number violating (LNV) interactions must be small in order to generate light neutrino masses.
Additionally, they introduce a small mass splitting $\Delta m$
$m_{4/5}^{} = m_M^{} + \frac12 m_M^{} |\theta|^2 \mp \frac12 \Delta m$
where the contribution with the active sterile mixing parameter $\theta = m_D / m_M$
$m_D = y_1 v$
$v\simeq174 \text{ GeV}$
The smallness of the LNV interactions ensures unobservable collider effects, with the exception of heavy neutrino-antineutrino oscillations since these are a macroscopic interference effect
$P^{\text{LNC}/\text{LNV}}_\text{osc}(\tau) = (1 \pm \cos\left(\Delta m \tau \right) \exp(-\lambda))/2$
where $\lambda$
Therefore, the details of the seesaw model besides the generated mass splitting can be neglected when simulating pseudo-Dirac heavy neutrinos as long as the neutrino-antineutrino oscillations are taken into account.
FeynRules implementation
The FeynRules model file contains in addition to the Standard Model parameter as free parameter the heavy neutrino
- Majorana mass
$m_M$
Mmaj
- mass splitting
$\Delta M$
deltaM
- mixing parameter
$\theta_\alpha$
theta1
,theta2
,theta3
- damping parameter
$\lambda$
damping
MadGraph patch
In order to generate events with heavy neutrino-antineutrino oscillations it is necessary to patch the [pSPSS]/bin/internal/common_run_interface.py
file in MadGraph using
mass_splitting = param_card.get_value('PSPSS', 2) damping = param_card.get_value('PSPSS', 6) for event in lhe: leptonnumber = 0 write_event = True for particle in event: if particle.status == 1: if particle.pid in [11, 13, 15]: leptonnumber += 1 elif particle.pid in [-11, -13, -15]: leptonnumber -= 1 for particle in event: id = particle.pid width = param_card['decay'].get((abs(id),)).value if width: if id in [8000011, 8000012]: tau0 = random.expovariate(width / cst) if 0.5 * (1 + math.exp(=damping)*math.cos(mass_splitting * tau0 / cst)) >= random.random(): write_event = (leptonnumber == 0) else: write_event = (leptonnumber != 0) vtim = tau0 * c else: vtim = c * random.expovariate(width / cst) if vtim > threshold: particle.vtim = vtim # write this modify event if write_event: output.write(str(event)) output.write('</LesHouchesEvents>\n') output.close()
which must replace the original code
for event in lhe: for particle in event: id = particle.pid width = param_card['decay'].get((abs(id),)).value if width: vtim = c * random.expovariate(width/cst) if vtim > threshold: particle.vtim = vtim #write this modify event output.write(str(event)) output.write('</LesHouchesEvents>\n') output.close()
The small mass splitting can cause problems in the automatic calculation of the decay width.
One way to fix this problem is by replacing the argument of the square root of the return value of the function calculate_apx_psarea
in the file [MadGraph]/mg5decay/decay_objects.py
by its absolute value.
Attachments (2)
- pSPSS.fr (27.9 KB ) - added by 10 months ago.
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pSPSS_UFO.zip
(64.9 KB
) - added by 10 months ago.
UFO folder
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