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I. Z. Rothstein

Publications and source records attributed to I. Z. Rothstein.

22 records · Page 2Linked to original sources

Closing the Windows on Mev Tau Neutrinos

In this note, we analyze various constraints on the ``visible'' decay modes of a massive $τ$ neutrino, $ν_τ\rightarrowν^\prime\,γ$ and $ν_τ\rightarrowν^\prime\, e^+ e^-$, where $ν^\prime$ is a light neutrino. The BEBC beam dump experiment provides model-independent constraints on these modes. The lifetime for the $ν^\prime\, e^+e^-$ mode is constrained to be $τ_{ν^\prime\, e^+e^-} \ge 0.18~(m_{ν_τ}/MeV)~sec.$ We point out that the same experiment implies a similar constraint on the $ν^\prime\,γ$ mode. This results in a new upper limit on the transition magnetic moment of $ν_τ$, $μ_{\rm tran} \le 1.1 \times 10^{-9} (MeV/m_{ν_τ})^2 μ_B $. Furthermore, a limit on the electric charge of $ν_τ$ may be obtained, $Q_{ν_τ} \le 4 \times 10^{-4}e$. Combining these constraints with those arising from supernova observations and primordial nucleosynthesis calculations, we show that these ``visible'' decays cannot be the dominant decay modes of the $τ$ neutrino.

hep-ph↗

Decoupling in Non-Perturbative Background Fields: the Thermal Sphaleron

Standard decoupling of heavy fermions may fail when there are non-perturbative variations in a scalar field which gives masses to the fermions. One situation of phenomenological relevance is the case of sphalerons in the presence of fermions at finite temperatures. The free energy of a simple model is determined using a non-perturbative technique to study the effect of fermions on the scalar field. The effects of quantum and thermal fermionic fluctuations on the free energy of the thermal sphaleron are calculated, including contributions from the gradients of the scalar field to all orders.

hep-ph↗

New Upper Limits on the Tau Neutrino Mass from Primordial Helium Considerations

In this paper we reconsider recently derived bounds on $MeV$ tau neutrinos, taking into account previously unaccounted for effects. We find that, assuming that the neutrino life-time is longer than $O(100~sec)$, the constraint $N_{eff}<3.6$ rules out $ν_τ$ masses in the range $0.5~(MeV)<m_{ν_τ}<35~(MeV)$ for Majorana neutrinos and $0.74~(MeV)<m_{ν_τ}<35~(MeV)$ for Dirac neutrinos. Given that the present laboratory bound is 35 MeV, our results lower the present bound to $0.5$ and $0.74$ for Majorana and Dirac neutrinos respectively.

hep-ph↗

Planck Scale Symmetry Breaking and Majoron Physics

Majoron models provide neutrino masses via the spontaneous breaking of a global $U(1)$ symmetry. However, it may be argued that all global symmetries will be explicitly violated by gravitational effects. We show that it is possible to preserve most of the usual features of majoron models by invoking $U(1)_{B-L}$ to be a gauge symmetry and adding a second singlet scalar field. The majoron gets a small model dependent mass. The couplings of majorons to neutrinos may be of ordinary strength or may be made arbitrarily weak. We discuss the cosmological and astrophysical consequences of majoron models in the context of a model dependent majoron mass and neutrino coupling. For an appropriate choice of parameters majorons can play the role of dark matter.

hep-ph↗