Changes between Version 16 and Version 17 of pSPSS
- Timestamp:
- Oct 20, 2022, 10:44:27 AM (2 years ago)
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pSPSS
v16 v17 16 16 17 17 The additional lepton number violating (LNV) interactions must be small in order to generate light neutrino masses.[[BR]] 18 Additionally, they introduce a small mass splitting [[latex($\Delta m$)]] between the two heavy neutrino mass eigen 18 Additionally, they introduce a small mass splitting [[latex($\Delta m$)]] between the two heavy neutrino mass eigenstates 19 19 20 20 [[latex($m_{4/5}^{} = m_M^{} + \frac12 m_M^{} |\theta|^2 \mp \frac12 \Delta m$)]] 21 21 22 22 where the contribution with the active sterile mixing parameter [[latex($\theta = m_D / m_M$)]] with [[latex($m_D = y_1 v$)]] and [[latex($v\simeq174 \text{ GeV}$)]] appears already in the LNC case.[[BR]] 23 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 23 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.[[BR]] 24 At leading order, the oscillations between LNC and LNV processes induced by them can be described by 24 25 25 26 [[latex($P^{\text{LNC}/\text{LNV}}_\text{osc}(\tau) = (1 \pm \cos\left(\Delta m \tau \right) \exp(-\lambda))/2$)]] 26 27 27 where [[latex($\lambda$)]] captures thedamping of the oscillations due to decoherence.[[BR]]28 where [[latex($\lambda$)]] captures potential damping of the oscillations due to decoherence.[[BR]] 28 29 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. 29 30