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:
Nuclear structure investigations for fundamental symmetries and nuclear astrophysics1h
Modern nuclear physics experiments that probe different aspects of the atomic nuclei have the potential to answer diverse fundamental questions concerning nuclear interactions, perform precision tests of fundamental symmetries as well as provide critical nuclear structure information to understand astrophysical processes that produce the nuclei.
In this talk, I will first present some experimental studies that can potentially set stringent constraints on fundamental symmetries and nuclear structure models. In this context, I will present the results of a high-precision experiment performed to determine the superallowed branching ratio for the beta decay of 19Ne -->19F and as a consequence of this measurement a means to place stringent bounds on right-handed weak interactions. In the same spirit, I will discuss some results about the pairing properties of 136Ba that is important to be reproduced by nuclear structure models and hence allows to set important constrains on the calculated nuclear matrix elements for the 0vββ decay of 136Xe-->136Ba.
Finally, I will discuss about my current project which is designed to address crucial questions about the p-process nucleosynthesis that leads to the formation of about 35 stable proton rich nuclei. The modeling of this process needs several nuclear physics inputs but most importantly a better theoretical description of alpha-capture reactions rates in heavy nuclei and at very low energies. I will conclude this talk by brie y discussing our experimental campaign designed to address these crucial aspects.