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:
Nikhef Colloquium: "What have Hadron-Hadron interactions to do with Neutron stars? Maybe nothing." (Laura Fabbieti)
What have Hadron-Hadron interactions to do with Neutron stars? Maybe nothing.50m
Abstract: Strange hadrons might play a rather crucial role in understanding the composition of the innermost part of neutron stars. Indeed among the many models attempting to describe the core of neutron stars many envisage the presence of strange hadrons. First Hypotheses saw the formation of a condensate composed of antikaons and neutrons as forming the neutron star cores, but the later discovery of extremely massive neutron stars currently disfavor this scenario. More recently Hyperons have been considered more suited candidates within these models but experimental confirmations are still needed. In this talk the tools offered by experiments at accelerators to verify the above-mentioned models will be presented. The state of the art knowledge in the field will be summarized and future perspectives discussed.