Scattering amplitudes can be extracted from time-ordered n-point functions by means of the well known LSZ reduction formula, even in non-perturbative Quantum Field Theories, such as Quantum Chromod
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 | "la Caixa" Foundation Fellowships Ceremony | 105 researchers will develop their projects in Spain and Portugal thanks to the 65 fellowships granted within the framework of the INPhINIT doctoral program and the 40 fellowships from the Junior Leader postdoctoral program. |
 | The IFT holds NASA’s Fermi-LAT collaboration meeting for the first time in Spain | From March 11th to the 15th at the Instituto de Física Teórica UAM-CSIC. |
 | Nearly fifty high school students explore particle physics at the IFT | Thanks to a new edition of the 'Hands-on Particle Physics' Masterclass |
 | New measurement of cosmic distances in the Dark Energy Survey gives clues about the nature of dark energy |
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 | Institutional visit of the CSIC President to the CFTMAT | Eloísa del Pino, President of the CSIC, has addressed the research and technical staff and held various meetings with the management teams of both centers, IFT and ICMAT. |
 | Talk by Juan García-Bellido about new perspectives in modern cosmology | The outreach talk will take place on Tuesday, February 20, at 7:00 PM at the Ramón Areces Foundation - Auditorium. Address: Calle Vitruvio, 5, 28006, Madrid. |
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Upcoming Events
May 21, 2024
11:30am to 12:30pm
The nature of the dark matter in the Universe is among the longest and most important outstanding problems in all of modern physics.
May 21, 2024
2:00pm to 3:00pm
Join the IFT cosmology/gravity journal club at https://benty-fields.com to vote for papers and volunteer to present them.
May 22, 2024
11:30am to 12:30pm
"I will give a brief introductory presentation on the topic of symmetry-protected topological (SPT) phases [mainly in (1+1)D], with an emphasis on the relevant concepts, including the definition of
May 23, 2024
3:00pm to 4:00pm
Dark matter (DM) below a GeV is motivated by some cosmological histories and possibly by anomalies in data. Leading detectors cannot easily test it, due to its small kinetic energy.
May 30, 2024
3:00pm to 4:15pm
We present a chiral non-abelian dark sector model that features a spontaneous $SU(3)\times SU(2) \rightarrow SU(3)$ symmetry breaking and results in the formation of dark mesons, $\pi_D$, and baryo
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