Suitable for undergraduate and graduate physics students, this unique textbook provides an ideal entry point into particle, nuclear, and astroparticle physics and presents the modern concepts, theories, and experiments that explain the elementary constituents and basic forces of the universe.
Suitable for undergraduate and graduate physics students, this unique textbook provides an ideal entry point into particle, nuclear, and astroparticle physics and presents the modern concepts, theories, and experiments that explain the elementary constituents and basic forces of the universe.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Francesco Terranova has been working in collider and neutrino physics for 25 years giving significant contributions to the DELPHI experiment at LEP (direct evidence of triple gauge couplings), the construction and data analysis of OPERA (first observation of tau neutrino appearance in a long-baseline experiment), and CUORE (search for neutrinoless double-beta decay with bolometers). In 2015, he proposed the concept of 'monitored neutrino beam' and is currently Co-Spokesperson of the CERN NP06/ENUBET experiment. Since 2018 he has worked in DUNE, the US flagship project in neutrino physics, which studies CP violation in neutrinos and multi-messenger physics.
Inhaltsangabe
1: Setting the scene 2: Scattering and decay 3: Measurements in particle physics 4: Accelerators and colliders 5: Symmetries and antimatter 6: Electromagnetic interactions 7: The modern theory of strong interactions 8: Flavor symmetries and the quark models 9: From QCD to nuclear physics 10: Weak interactions 11: Radioactivity and cosmic engines 12: The electroweak theory 13: At the forefront of the Standard Model Free
1: Setting the scene 2: Scattering and decay 3: Measurements in particle physics 4: Accelerators and colliders 5: Symmetries and antimatter 6: Electromagnetic interactions 7: The modern theory of strong interactions 8: Flavor symmetries and the quark models 9: From QCD to nuclear physics 10: Weak interactions 11: Radioactivity and cosmic engines 12: The electroweak theory 13: At the forefront of the Standard Model Free
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