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In order to enable an iCal export link, your account needs to have a 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.
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In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key 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 remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.
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Plenary Session 12
Place
Location: University of Warsaw, Faculty of Physics
Higgs-R2 inflation is a well-motivated model of inflation as it solves the unitarity issue of Higgs inflation, is consistent with the current CMB observation, and is within the scope of the near future B-mode observation. In this talk, I will first review these basic properties of Higgs-R2 inflation. I then show that the isocurvature mode, which is a mixture of the Higgs boson and the scalaron, ca
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Dynamical chiral symmetry breaking in a QCD-like hidden sector is used to generate the Planck mass and the electroweak scale including the heavy right-handed neutrino mass. A real scalar field transmits the energy scale of the hidden sector to the visible sectors, playing a role of inflaton in the early Universe. We discuss the inflationary dynamics and predictions for non-Gaussianity in our mode
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Presented by Dr. Mayumi AOKI
on
16/09/2023
at
12:30
U(1)Lμ−Lτ≡U(1)X model is anomaly free within the Standard Model (SM) fermion content, and can accommodate the muon (g−2) data for MZ′∼O(10−100) MeV and gX∼(4−8)×10−4. WIMP type thermal dark matter (DM) can be also introduced for MZ′∼2MDM, if DM pair annihilations into the SM particles occur only through the s-channel Z′ exchange. In this work, we show that this tight cor
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Presented by Prof. Pyungwon KO
on
16/09/2023
at
12:00
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