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:
MLL-Kolloquium: Dr. Takashi Toma (Physik Department, TUM): Radiative Generation of Neutrino Masses and Dark Matter
Lecture Hall (ground floor west) (LMU building, Am Coulombwall 1, Garching)
Lecture Hall (ground floor west)
LMU building, Am Coulombwall 1, Garching
Small non-zero neutrino masses and the existence of dark matter in the universe are required from experiments, but both are not explained in the Standard Model. The canonical seesaw mechanism is the simplest approach to generate the small neutrino masses. However, a dark matter candidate has to be introduced independently in order to explain some astronomical observations. The mechanism of generating neutrino masses through radiative corrections is an alternative possibility for solving the two different issues simultaneously. I will introduce some representative models and discuss their phenomenological implications. In addition, I will also point out some deficiencies of these models and consider further extensions to resolve them.