Changes between Version 16 and Version 17 of pSPSS


Ignore:
Timestamp:
Oct 20, 2022, 10:44:27 AM (2 years ago)
Author:
Jan Hajer
Comment:

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  • pSPSS

    v16 v17  
    1616
    1717The 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 states
     18Additionally, they introduce a small mass splitting [[latex($\Delta m$)]] between the two heavy neutrino mass eigenstates
    1919
    2020[[latex($m_{4/5}^{} = m_M^{} + \frac12 m_M^{} |\theta|^2 \mp \frac12 \Delta m$)]]
    2121
    2222where 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
     23The 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]]
     24At leading order, the oscillations between LNC and LNV processes induced by them can be described by
    2425
    2526[[latex($P^{\text{LNC}/\text{LNV}}_\text{osc}(\tau) = (1 \pm \cos\left(\Delta m \tau \right) \exp(-\lambda))/2$)]]
    2627
    27 where [[latex($\lambda$)]] captures the damping of the oscillations due to decoherence.[[BR]]
     28where [[latex($\lambda$)]] captures potential damping of the oscillations due to decoherence.[[BR]]
    2829Therefore, 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.
    2930