You are talking about the start of a process called "neutrino lasing" , for example:
We present a calculation of a neutrino decay scenario in the early Universe. The specific decay is $\nu_{2} \to \nu_{1} + \phi,$ where $phi$ is a boson. If there is a neutrino mass hierarchy, $m_{\nu_{e}} < m_{\nu_{\mu}} < m_{\nu_{\tau}}$, we show that it is possible to generate stimulated decay and effects similar to atomic lasing without invoking new neutrinos, even starting from identical neutrino distributions. Under the right circumstances the decay can be to very low momentum boson states thereby producing something similar to a Bose condensate, with possible consequences for structure formation. Finally, we argue that this type of decay may also be important other places in early Universe physics.
There are also lasing calculations for neutrinos in the sun, closely related to your question:
Applying the phenomenon of neutrino lasing in the solar interior, we show how the rate for the generic neutrino decay process $\nu -> fermion + boson$, can in principal be enhanced by many orders of magnitude over its normal decay rate. Such a large enhancement could be of import to neutrino-decay models invoked in response to the apparent deficit of electron neutrinos observed from the sun. The significance of this result to such models depends on the specific form of the neutrino decay, and the particle model within which it is embedded.
Note the date, 1994. At present mainstream physics accepts that neutrino oscillations, which have been seen in the lab also, explain the deficit of electron neutrinos, so this model is not validated,
The reason there is no attempt to study a lasing mechanism in the laboratory is due to the weak interaction of neutrinos with matter. To get a lazing action there should be a high probability for the secondary neutrinos to keep raising the level of new atoms,as with electromagnetic lasing, but the weak coupling constant is so much smaller than the electromagnetic that this cannot happen with weak interactions in the dinensions of matter on earth. The sun and the cosmological early times are the field for this study.
The weak coupling constant is also the reason why the decay times for unstable nuclei cannot be measurably affected by a neutrino starting a lasing inversion. The probability of a neutrino interacting with a nucleus is very small.
edit:
Has this behavior been excluded by experiment?
It cannot be excluded by experiment because of the very low probability of the interaction ( weak coupling constant. It might in the future be useful to model in cosmological observations.
Is this prohibited by theory/symmetries somehow?
no
Is this a real thing?
Real in physics means measurable. see answer to 1
What happens if we sub the neutrino for dark matter candidate particles?
it has been done by various models. example .