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Hello. I have been playing around with your code. It is very well-organised and easy to use - so thank you!
I've just encountered one thing I can't figure out. I modified the Planck example in the…
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Only a fraction of the high-energy gamma-rays, cosmic rays, and neutrinos have origins which can be associated with astronomical sources. One two Galactic accelerators up to PeV energies, and one extr…
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I recently developed an idea that we can still preserve neutrino oscillations without neutrino mass.
The first thing to explain it the direct neutrino mass experiments. Review papers showed that th…
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Hi there
The class background module returns the growth factor D(z) and f(z) = dlnD/dlna for dust universe. Is there a function (perhaps in perturbation module) that returns the scale-dependant gro…
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Methods like calling TJPCov and using the internal gaussian seem to be quite unstable leading to non-positive definite matrices and breaking the cholesky decomposition.
I haven't yet found a way to…
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only possible anti matter reactor will use neutrinos instead of heat or other things because most of energy released is neutrinos
only neutronium in supernova cores can capture neutrino and cause boo…
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Hi,
I have tried to reproduce pisa results with my own code using vanilla prob3++ and just including detector systematics. I attach the 90% CL contours.
After inspecting the spectra for a few b…
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[I'm raising this because it's clearly a huge issue, and I'm not 100% sure if it's going to be covered. Is anybody on "Galaxies" here?]
Dark matter consists of 25% of the Universe, gets studied a l…
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The polarization vector of the primary lepton seems to be set to -1 (antiparallel to the momentum vector), regardless of the energy of the lepton ([based on this code](https://github.com/GENIE-MC/Gene…
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When I use gmkspl in generating the reaction cross section for neutrinos and nuclides, I get a GSL error as follows:
### Error in : Error 4 in $ROOTSYS/GSL-src/monte/vegas.c at 128 : xu must be gre…