The Excitement of Neutrino Physics
... Stopping radiation with lead shielding: Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years ! ...
... Stopping radiation with lead shielding: Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years ! ...
VSharma-JC-2008-10
... What about interactions of high energy photons? What about neutral pions which decay very quickly (the mean lifetime is just 8×10-17 s, ct = 25 nm) to two photons? To answer these questions think about the evolution of the electromagnetic cascade ... For a deeper insight to the electromagnetic and h ...
... What about interactions of high energy photons? What about neutral pions which decay very quickly (the mean lifetime is just 8×10-17 s, ct = 25 nm) to two photons? To answer these questions think about the evolution of the electromagnetic cascade ... For a deeper insight to the electromagnetic and h ...
Electron Neutrino Sources from the Core of the Earth
... with their quantities adapted to 4 × 109 years ago, were uniformly distributed ..., it is quite possible that radioactive heating could produce fusion in a fraction of the age of the Earth.” Just as the solar neutrino flux [7] constitutes direct evidence of nuclear reactions within the Sun, an obser ...
... with their quantities adapted to 4 × 109 years ago, were uniformly distributed ..., it is quite possible that radioactive heating could produce fusion in a fraction of the age of the Earth.” Just as the solar neutrino flux [7] constitutes direct evidence of nuclear reactions within the Sun, an obser ...
REU Research Project: Simulating neutron interaction with the Super
... simulation to accepted physical data from neutrons. In a rare occurrence (~2% of a million events), the PMTs return an energy deposit value that is much larger than the initial beam energy. In 99% of these cases, the sum of all energy deposits in PMTs is equal to 793 keV. This process is the result ...
... simulation to accepted physical data from neutrons. In a rare occurrence (~2% of a million events), the PMTs return an energy deposit value that is much larger than the initial beam energy. In 99% of these cases, the sum of all energy deposits in PMTs is equal to 793 keV. This process is the result ...
Física Teórica de Partículas
... How to break the Flavour Code ? How to understand the pattern of fermion masses ! and mixing ? Are there more than one Higgs doublet ? Are neutrinos Majorana or Dirac Particles? Is there leptonic CP Violation, detectable in neutrino oscillations? What is the origin of the Baryon Asymmetry! of the Un ...
... How to break the Flavour Code ? How to understand the pattern of fermion masses ! and mixing ? Are there more than one Higgs doublet ? Are neutrinos Majorana or Dirac Particles? Is there leptonic CP Violation, detectable in neutrino oscillations? What is the origin of the Baryon Asymmetry! of the Un ...
Syllabus of Instrumentation and Methods in Astroparticle Physics
... Syllabus of Instrumentation and Methods in Astroparticle Physics The course is designed to introduce the experimental techniques and the data analysis methods of Particle Astrophysics. We will review special relativity and particle physics to remind or introduce basic concepts that will be used thro ...
... Syllabus of Instrumentation and Methods in Astroparticle Physics The course is designed to introduce the experimental techniques and the data analysis methods of Particle Astrophysics. We will review special relativity and particle physics to remind or introduce basic concepts that will be used thro ...
neutrinos: mysterious particles with fascinating features, which led to
... Gamma Ray Bursts, supernova explosions, etc. They are also produced inside the Earth (by decays), in our atmosphere (when cosmic rays hit it and trigger an air shower of secondary particles), and on the Earth, in particular in nuclear reactors. The latter provide ν̄-energies around 1 MeV, with a IV. ...
... Gamma Ray Bursts, supernova explosions, etc. They are also produced inside the Earth (by decays), in our atmosphere (when cosmic rays hit it and trigger an air shower of secondary particles), and on the Earth, in particular in nuclear reactors. The latter provide ν̄-energies around 1 MeV, with a IV. ...
Particle accelerators
... 100 million times greater than the energy reached with our accelerators. This is the energy of a 90 mph tennis ball compressed into a single proton ! ...
... 100 million times greater than the energy reached with our accelerators. This is the energy of a 90 mph tennis ball compressed into a single proton ! ...