In order to enable an iCal export link, your account needs to have an API key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
Additionally to having an API key associated with your account, exporting private event information requires the usage of a persistent signature. This enables API URLs which do not expire after a few minutes so while the setting is active, anyone in possession of the link provided can access the information. Due to this, it is extremely important that you keep these links private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately create a new key pair on the 'My Profile' page under the 'HTTP API' and update the iCalendar links afterwards.
Permanent link for public information only:
Permanent link for all public and protected information:
02.430 (Mainz Institute for Theoretical Physics, Johannes Gutenberg University)
Mainz Institute for Theoretical Physics, Johannes Gutenberg University
Staudingerweg 9 / 2nd floor, 55128 Mainz
After the discovery of the Higgs boson, the SM of particle physics is theoretically complete, nevertheless it leaves many questions unanswered. Most important of those are the naturalness of the electroweak scale, the nature of dark matter, the origin of matter in the Universe and the structure of flavor.
Experimentally, data from Run 2 of the LHC will give us a good idea of what can be expected from the experiments in the long run: by the summer of 2017 either there will already be a discovery of new physics or some significant deviations from SM expectations, or one will have to start facing the fact that new physics might remain invisible at 13/14 TeV hadron colliders. At the same time the Xenon 1T experiment will push the frontier of Dark Matter direct detection closer towards the neutrino floor, Planck legacy results will be known, and the first data of Belle II might be on their way. In addition, the physics cases for future colliders like FCC, CepC, SppC will already be well studied at that point. This makes 2017 an ideal time to pause and to critically reassess the status of new physics in light of these anticipated new results and to brainstorm about new ideas by bringing together experts from all areas of BSM physics. Potential discoveries will be analyzed in particular regarding their impact on naturalness, dark matter and flavor. In the absence of convincing new signals, we will discuss new strategies to uncover natural models of the electroweak scale, like the MSSM and composite Higgs models, or whether they should be abandoned in favour of more elusive "neutral naturalness" scenarios like relaxion and twin Higgs.