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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…
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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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The recent issue from @micheledoro #5147 shows the need for a more flexible class for the `PrimaryFlux` class, which allows different spectra files for input.
Currently there are three different opt…
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The scales and lower/upper bounds of some parameters (eg mass of neutrinos and omega_b) do not match experimental errors, resulting in crazy values during MCMCs.
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We can report the L2 and max norm of the error in the trace of the particles' density matrices.
Currently, for each particle the flavor vector length L is calculated from `N_ab`, the matrix storing…
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The `Particle` class has an unused `tex` property for typesetting particle names. Let's fill this out for concrete classes. It would be especially nice if we can do this implicitly in some cases, e.g.…
fionn updated
6 years ago
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Sophia occasionally crashes with
`sophiaevent: theta < -1.D0: -1.0000067840120266`
reported by @DavidWit
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The characterizations of ultra-relativistic degrees of freedom/massless neutrino density in CLASS differs from that of CAMB, where N_ur does not equal N_eff - number of massive neutrinos. Instead, N_u…
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My understanding is that current and future surveys are/will be able to probe the neutrino mass hierarchy. It would make sense to allow for not just three massive neutrinos with identical masses.
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I am running a 1D simulation with injected Helium particles from a source redshift evolution and with relevant interactions for energy loss. The simulation fails with following Exception error saying …