Public mailing list
If you are interested in discussions about current and future EOS development, you are invited to join the EOS developers mailing list at Google Groups.
If you are interested in discussions about current and future EOS development, you are invited to join the EOS developers mailing list at Google Groups.
I have just released version 0.1.1, which you can find here.
Changes since version 0.1 include:
Contributors of these changes are:
Thanks to a gratuitous donation of an iMac computer by Prof. Leo van Hemmen, we can now actively support building and using EOS on Mac OS X. We thank Professor van Hemmen very much for his donation!
The test hardware in use is limited to Mac OS 10.11 (El Capitan). We would be happy to receive reports about EOS builds on more recent Mac OS versions. The installation on MacOS via the Homebrew package manager is documented in the manual. The minimal commands necessary to build the most recent development version are
brew tap eos/eos
brew install --HEAD eos
In order to speed up build time of our TravisCI test cases, docker images
with the EOS build-time dependencies pre-installed are available over at
the docker hub in
eoshep/build-essentials.
These are used as for CI testing as of commit 21f61a28.
Even though it is a small annoyance that docker does not permit three-letter organization
names, hence the eoshep
name.
You can pull these images as you would pull any docker image using either
docker pull eoshep/build-essential:xenial
or
docker pull eoshep/build-essential:bionic
The source files for building these images are kept here. Please feel free to contribute your own docker files for whatever architecture you build EOS on.
While working on their publication EOS-2017-02, Tom Blake and Michal Kreps derived the full set of angular observables for the decay Λb → Λ ℓ+ ℓ- in the case of a polarised Λb baryon. They find a total of 34 angular observables compared to the 10 observables in the unpolarised case (compare the theory paper EOS-2014-01 and the fit to LHCb data in EOS-2016-02). The additional 24 observables can be classified as:
They modified the existing EOS code such that now all angular observables can be predicted. Their modifications have already been pushed to the master branch, and a corresponding tag has been pushed as well. A big thank you to Tom and Michal from my side for their contributions to EOS!