• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Syllabus of Instrumentation and Methods in Astroparticle Physics
Syllabus of Instrumentation and Methods in Astroparticle Physics

... 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 throughout the c ...
There is a theory which states that if ever for... Universe is for and why it is here it will...
There is a theory which states that if ever for... Universe is for and why it is here it will...

NAME: Quiz #5: Phys142 1. [4pts] Find the resulting current through
NAME: Quiz #5: Phys142 1. [4pts] Find the resulting current through

Higgs_1 - StealthSkater
Higgs_1 - StealthSkater

... Abdus Salam received the Nobel Prize in physics for unifying the weak subnuclear interaction with electromagnetism. The third fundamental force is called the strong nuclear force. It binds 3 quarks together to from the proton and the neutron. It is also responsible for causing protons and neutrons ...
Sample exam 2
Sample exam 2

... b) how long does it take in the lab frame? ...
Fulltext PDF
Fulltext PDF

... 11 The decay μ → eγ is therefore a good place to search for new physics beyond the Standard Model of Particle Physics. ...
Some properties of Thomson`s atom
Some properties of Thomson`s atom

... Some properties of Thomson’s atom In Thomson’s model for the Hydrogen atom, the positive charge e is uniformly distributed within a sfere of radius a0 . The electron, having charge −e, is considered to be a point particle and is located inside the sphere. a) Find the electric field and the potential ...
Particle accelerators
Particle accelerators

ppt - Infn
ppt - Infn

... c) Nuclear matrix elements (exploring better, and agreeing on, the reasons for the spread of calculated values, and deciding on the optimum way of performing the calculations, while pursuing vigorously also the application of the shell model). ...
Electrostatics HW 2 HW 4.2 1e- = -1.6x10
Electrostatics HW 2 HW 4.2 1e- = -1.6x10

... What can you conclude about the magnitude of the wool’s charge after the rubbing? Why? ...
Standard Model
Standard Model

... 1964 – Proposed by Murray Gell-Mann and George Zweig  Initially only three flavours of quarks: up, down and strange  A year later, another flavour was added: charm ...
Linear momentum and the impulse
Linear momentum and the impulse

... Next, we contemplate how to change the value of p for a particle. Obviously, the mass can not change and therefore to change p we must do it by changing v, i.e we must accelerate the particle. Newton’s second law gives Fnet = m dv/dt = d [mv]/dt = dp/dt. This becomes for a system of particles, Fextn ...
The Electron - Student Moodle
The Electron - Student Moodle

... mass of a proton or neutron), this means electrons are particles, and all of the equations that apply to motion of solid particles also apply to electrons. However, an electromagnetic wave is a wave of electricity, and electricity is made of electrons that are moving. This means that moving electron ...
Answers to Coursebook questions – Chapter J3
Answers to Coursebook questions – Chapter J3

... Parapositronium can decay into two photons whose spins are up and down, making a spin of zero. Orthopositronium can decay into three photons, where two photons have spin up and one has spin down, making a total spin of 1. It cannot, however, decay into a single photon because this would violate cons ...
Wave as particle 2
Wave as particle 2

... mass of two electrons ( 2me c 2 ) interact with the electric field of a nucleus, this photon may be turned into a pair of electron and positron. This process is called pair production through which energy gets turned into mass. Positron is the anti-particle of electron: it has the same mass as an el ...
Document
Document

... If the diagram can be cut in two by slicing only gluon lines (and not cutting open any external lines), the process is suppressed. Qualitatively OZI rule is related to the asymptotic freedom. ...
Cosmic calibration - TWiki
Cosmic calibration - TWiki

Prerequisites Level Year Number of Study Hours Course Code
Prerequisites Level Year Number of Study Hours Course Code

... This is an advanced course offered to the 8th level undergraduate senior students at the Jazan University. Particle and radiation interactions with matter, particle detectors, particle accelerators, particles zoo and the standard model are the main chapters to be covered in this course. The learning ...
Historical Introduction to the Elementary Particles
Historical Introduction to the Elementary Particles

... deflected by a magnet. This suggested that they carried electric charge; • 2. in fact, the direction of the curvature required that the charge be negative. • 3. It seemed, therefore, that these were not rays at all, but rather streams of particles. • 4. By passing the beam through electric and magne ...
Parts of an atom lesson
Parts of an atom lesson

... 3. Electrons – Negative particles in region around nucleus. N P ...
Presentazione di PowerPoint
Presentazione di PowerPoint

Cosmic Rays - High Energy Physics at Wayne State
Cosmic Rays - High Energy Physics at Wayne State

... 1) Even though they decay, they have sufficiently long lifetime such that the more energetic muons reach sea level before decaying 2) Unlike electrons (which are much lighter) they do not interact with atomic fields so easily The neutrinos interact only weakly, so they easily reach sea level (and co ...
4.2 - Science with Mrs. Vaness
4.2 - Science with Mrs. Vaness

Experiment to measure the Charge to Mass Ratio of Electrons 1AN
Experiment to measure the Charge to Mass Ratio of Electrons 1AN

MuNew Sesaps (1) WM
MuNew Sesaps (1) WM

... case of the stopped muons - of the emitted electron (in arbitrary units), tallying these events afterwards. We will graph the cosmic ray energy of unspecified particles passing through our detector, as well as the energy of stopped muons, with which they enter the detector, and of decay electrons, a ...
< 1 ... 188 189 190 191 192 193 194 195 196 ... 202 >

Lepton



A lepton is an elementary, half-integer spin (spin 1⁄2) particle that does not undergo strong interactions, but is subject to the Pauli exclusion principle. The best known of all leptons is the electron, which is directly tied to all chemical properties. Two main classes of leptons exist: charged leptons (also known as the electron-like leptons), and neutral leptons (better known as neutrinos). Charged leptons can combine with other particles to form various composite particles such as atoms and positronium, while neutrinos rarely interact with anything, and are consequently rarely observed.There are six types of leptons, known as flavours, forming three generations. The first generation is the electronic leptons, comprising the electron (e−) and electron neutrino (νe); the second is the muonic leptons, comprising the muon (μ−) and muon neutrino (νμ); and the third is the tauonic leptons, comprising the tau (τ−) and the tau neutrino (ντ). Electrons have the least mass of all the charged leptons. The heavier muons and taus will rapidly change into electrons through a process of particle decay: the transformation from a higher mass state to a lower mass state. Thus electrons are stable and the most common charged lepton in the universe, whereas muons and taus can only be produced in high energy collisions (such as those involving cosmic rays and those carried out in particle accelerators).Leptons have various intrinsic properties, including electric charge, spin, and mass. Unlike quarks however, leptons are not subject to the strong interaction, but they are subject to the other three fundamental interactions: gravitation, electromagnetism (excluding neutrinos, which are electrically neutral), and the weak interaction. For every lepton flavor there is a corresponding type of antiparticle, known as antilepton, that differs from the lepton only in that some of its properties have equal magnitude but opposite sign. However, according to certain theories, neutrinos may be their own antiparticle, but it is not currently known whether this is the case or not.The first charged lepton, the electron, was theorized in the mid-19th century by several scientists and was discovered in 1897 by J. J. Thomson. The next lepton to be observed was the muon, discovered by Carl D. Anderson in 1936, which was classified as a meson at the time. After investigation, it was realized that the muon did not have the expected properties of a meson, but rather behaved like an electron, only with higher mass. It took until 1947 for the concept of ""leptons"" as a family of particle to be proposed. The first neutrino, the electron neutrino, was proposed by Wolfgang Pauli in 1930 to explain certain characteristics of beta decay. It was first observed in the Cowan–Reines neutrino experiment conducted by Clyde Cowan and Frederick Reines in 1956. The muon neutrino was discovered in 1962 by Leon M. Lederman, Melvin Schwartz and Jack Steinberger, and the tau discovered between 1974 and 1977 by Martin Lewis Perl and his colleagues from the Stanford Linear Accelerator Center and Lawrence Berkeley National Laboratory. The tau neutrino remained elusive until July 2000, when the DONUT collaboration from Fermilab announced its discovery.Leptons are an important part of the Standard Model. Electrons are one of the components of atoms, alongside protons and neutrons. Exotic atoms with muons and taus instead of electrons can also be synthesized, as well as lepton–antilepton particles such as positronium.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report