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NEWS
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Version 1.0 :
~~~~~~~~~~~~~
first public version
Version 1.1 :
~~~~~~~~~~~~~
Bugs fixed in kolmogoroff fields:
- correct destructor
- define a Bmax() and a _fBmax
Bug fixed in env1d:
When a source density is defined then _fXmax is 1.01*Density->Xmax(),
which gives a non-zero value for a uniform density.
Bug fixed in particlepropa/photon:
- Correction of _fTime by adding lTcorr in CheckDetection (particlepropa).
- Compute EM cascade propagation distance with accurate observer geometry.
Bug fixed:
- slight memory leak in TSophiaInteraction
- important memory leak in DINT (synchrotron tables)
Bug fixed in sourcedensity: name of the .fits source density file to
be read by cfitsio >= 3.
Slight improvment to avoid problems in some extreme configurations:
- RK integrator modification.
- secondary pair production photons are propagated only when
_fTimeStep >= 0.1*IntegratorMinTimeStep
Slight improvments in configuration files parsing:
Test number of sources
Feature added, continuous, uniform source density in 1D:
Can specify Xmin (in order to easily modelize the effect of the
position of nearest source)
Feature added in the output of photons:
prints out "Source_Energy" in EeV, in order to know the injection energy
of the primary nucleon that generated the photon. Mostly useful in 3D
(in 1D, when only a "grid" of EM showers are propagated, this field is
arbitrarily set to 0)
Feature added: test of the 1D approximation for the EM cascade
if the flag <CutCascade_MagField /> is set within the <Interactions>
marker, the following is applied within DINT: At each step all the e+/-
with an energy E_e < E_c are removed from the cascade, where E_c is
obtained by comparing t_larmor, t_synch, and t_ics. This allows to
estimate the error which is made on the point-source flux due to
the 1D approximation of the EM cascade.
New installation procedure: using configure
Version 1.2 :
~~~~~~~~~~~~~
Tested on MacOSX Intel and SL4 (GNU compiler)
Small bug corrected, in previous improvments in nucleon.cc
Bug fixed to compile with MacOS using configure
Slight improvment: a null radio background is implemented; the
default radio being "Obs"
Slight improvment: the parameter "A" to cut the EM cascade by comparing
the Larmor radius and loss timescales can be set directly from the
XML file.
Slight improvment: the number of crowns of boxes around which one looks
for observers in the case of a neutrino may be set by hand to any value
in the neutrino.h file.
Feature added: primary photons can be propagated in 1D
Feature added: possibility to include a probability to follow the
secondary photons generated by pair production. By following only a
fraction of these EM cascades and then reweighting the results this
allows to gain some CPU in 3D configurations.
Version 1.3 :
~~~~~~~~~~~~~
Slight improvment: use of Hep PDT particle codes in the output to determine
particle types.
Feature added: ROOT output is now possible.