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
The establishment of the Lambda Cold Dark Matter paradigm in Cosmology has brought together physics on very diverse scales, with a mesmerizing variety of observational techniques and a unique theoretical effort. The consistency of this paradigm is today hindered by some tensions, either of internal consistency between datasets of different nature, or of seeming friction between theoretical predictions and observations. Observational and theoretical efforts are currently under way, in order to both understand the possible sources of systematics affecting the data, and to explain these frictions on theoretical grounds.
This workshop aims at bringing together the communities involved in this effort, building a bridge between observers and data analysists, theorists, and simulators, in order to address the following fundamental questions about the tensions in the CDM paradigm: Is the current tension in the determination of Hubble constant by different probes due to new physics, or to systematics? What are the real sources of the inconsistencies between theoretical predictions and observations at the smallest galactic scales? Is it a problem that we are seeing no new physics at LHC?
The ideal, two-fold, goal of the topical workshop is that of understanding whether tensions appearing on several scales are only episodical and disconnected from each other – and to which extent they are due to experimental systematics – or if they represent real cracks in the building of the ΛCDM. In the latter case, it remains to be assessed whether they are structural, thus hinting toward a major revision of our vision of the cosmological Universe, or they can be cured with minor modifications at different scales, separately.