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:
Prof. Laura Fabbietti - "Terrestrial experiments to understand what is inside neutron stars"
Main Auditorium (MPP)
Max-Planck-Institut für Physik
Föhringer Ring 6
Many physicists would like to know what is inside neutron stars (NS). Others would be already very happy if they could understand how two and three baryons interact with better accuracy than available today. The two things are intertwined since the two and three body hadron interaction determines the equation of state, hence how pressure and energy depend on density, for every hadron system. Different hypotheses can be made about the content of NS. The scenarios vary from pure dense neutron matter, to mixtures of neutrons and strange hadrons up to quark matter. Each hypothesis, provided that the interaction among the constituents is well known, leads to an equation of state and to a precise mass to radius relationship for the NS. This way, observations of masses and radii for NS can test different hypotheses. A new method is proposed to exploit particle production at accelerator experiments to substitute scattering experiments among different hadron species. This idea can also open up the possibility of studying three body interactions among hadrons. First results from the HADES and ALICE collaborations, two experiments at very different beam energies, will be shown and the potential of the method will be discussed.