Conveners
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes: Automatized One-Loop Matching of BSM Models
- Javier Fuentes-Martin (Universidad de Granada)
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
Keynotes
- There are no conveners in this block
-
Patrizia De Simone (INFN e Laboratori Nazionali di Frascati (IT)), Patrizia De Simone (Istituto Nazionale Fisica Nucleare (IT))27/03/2023, 08:30
-
Luka Santelj (Jozef Stefan Institute)27/03/2023, 09:00
-
Bernat Capdevila (IFAE)27/03/2023, 09:30
-
Chaoyi Lyu27/03/2023, 10:30
-
Prof. Prafulla Behera (Indian Institute of Technology Madras (IN))27/03/2023, 11:00
-
Syuhei Iguro (Nagoya University)27/03/2023, 11:30
-
Navid Khandan Rad27/03/2023, 19:15
-
Alberto Lusiani (Scuola Normale Superiore and INFN, sezione di Pisa)28/03/2023, 08:30
After the 0.46 ppm measurement in 2021, the Muon g-2 experiment at FNAL aims at measuring the muon anomaly with a 0.23 precision in 2023 and later with a precision matching the design of 0.14 ppm.
Go to contribution page -
Dominik Stockinger (IPPP Durham)28/03/2023, 09:00
-
Martin Hoferichter28/03/2023, 09:45
-
Gernot Eichmann28/03/2023, 18:15
The anomalous magnetic moment (g-2) of the muon continues to be one of the most promising places to look for evidence of new physics. First measurements at Fermilab have confirmed the previous Brookhaven result and slightly increased the tension with the Standard Model prediction to 4.2 standard deviations. The theoretical value is the sum of QED, electroweak and QCD contributions, where the...
Go to contribution page -
Greg Landsberg (Brown University (US))29/03/2023, 08:30
-
Bruce Mellado Garcia (University of Wisconsin)29/03/2023, 09:15
-
Javier Fuentes-Martin (Universidad de Granada)29/03/2023, 11:00
-
Tomer Volansky (Tel Aviv University (IL))30/03/2023, 08:30
-
Dr Pilar Coloma (Instituto de Fisica Teorica UAM/CSIC)30/03/2023, 09:00
-
Thomas Schwetz30/03/2023, 09:30
-
Joshua Ruderman (Princeton University), Joshua Thomas Ruderman (NYU)30/03/2023, 10:30
-
Alejandro Ibarra30/03/2023, 11:00
The flux of high energy neutrinos and photons produced in active galactic nuclei could get attenuated when they propagate through the dark matter spike around their central black hole. Using measurements of the neutrino and the gamma-ray fluxes from TXS 0506+056 and from NGC 1068 by IceCube and the Fermi-LAT we derive new constraints on the dark matter-neutrino and the dark matter-photon...
Go to contribution page -
Felix Kahlhoefer (Karlsruhe Institute of Technology)30/03/2023, 11:30
-
Diego Guadagnoli (LAPTh Annecy)30/03/2023, 19:30
-
Eung Jin Chun31/03/2023, 08:30
-
Pedro Klaus Schwaller (Mainz University)31/03/2023, 09:00
-
Dr Vivian Poulin (LUPM, CNRS & U. de Montpellier, France)
-
Alejandro Ibarra