Elementary Particles - Modern Physics - Lecture Slides, Slides of Physics

A great and very useful lecture on Modern Physics. These lecture slides include: Elementary Particles, Building Blocks of Matter, Positron, Antiparticles, Feynman Diagram, Fundamental Interactions, Graviton, Classification of Elementary Particles, Higgs Boson, Mesons, Particles and Lifetimes, Additional Conservation Laws, Strangeness, Hypercharge, Quarks

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14.1 Early Discoveries
14.2 The Fundamental Interactions
14.3 Classification of Elementary Particles
14.4 Conservation Laws and Symmetries
14.5 Quarks
14.6 The Families of Matter
14.7 Beyond the Standard Model
14.8 Accelerators
Elementary Particles
If I could remember the names of all these particles, I’d be a botanist.
- Enrico Fermi
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Download Elementary Particles - Modern Physics - Lecture Slides and more Slides Physics in PDF only on Docsity!

 14.1 Early Discoveries

 14.2 The Fundamental Interactions

 14.3 Classification of Elementary Particles

 14.4 Conservation Laws and Symmetries

 14.5 Quarks

 14.6 The Families of Matter

 14.7 Beyond the Standard Model

 14.8 Accelerators

Elementary Particles

If I could remember the names of all these particles, I’d be a botanist.

  • Enrico Fermi

Elementary Particles

 We began our study of subatomic physics in Chapter 12. We investigated the nucleus in Chapters 12 and 13. We now delve deeper, because finding answers to some of the basic questions about nature is a foremost goal of science:  What are the basic building blocks of matter?What is inside the nucleus?What are the forces that hold matter together?How did the universe begin?Will the universe end, and if so, how and when?

14.1: Early Discoveries

In 1930 the known elementary particles were the proton, the electron, and the photon.  Thomson identified the electron in 1897, and Einstein’s work on the photoelectric effect can be said to have defined the photon (originally called a quantum ) in 1905. The proton is the nucleus of the hydrogen atom.  Despite the rapid progress of physics in the first couple of decades of the twentieth century, no more elementary particles were discovered until 1932, when Chadwick proved the existence of the neutron, and Carl Anderson identified the positron in cosmic rays.

The Positron

 Dirac in 1928 introduced the relativistic theory of the electron when he combined quantum mechanics with relativity.  He found that his wave equation had negative, as well as positive, energy solutions.  His theory can be interpreted as a vacuum being filled with an infinite sea of electrons with negative energies.  If enough energy is transferred to the “sea”, an electron can be ejected with positive energy leaving behind a hole that is the positron , denoted by e + .

Cosmic Rays

 Cosmic rays are highly energetic particles, mostly

protons, that cross interstellar space and enter the

Earth’s atmosphere, where their interaction with

particles creates cosmic “showers” of many

distinct particles.

Positron-Electron Interaction

 The ultimate fate of positrons (antielectrons) is

annihilation with electrons.

 After a positron slows down by passing through

matter, it is attracted by the Coulomb force to an

electron, where it annihilates through the reaction

Yukawa’s Meson

 The Japanese physicist Hideki Yukawa had the idea of developing a quantum field theory that would describe the force between nucleons analogous to the electromagnetic force.  To do this, he had to determine the carrier or mediator of the nuclear strong force analogous to the photon in the electromagnetic force which he called a meson (derived from the Greek word meso meaning “middle” due to its mass being between the electron and proton masses).

 Yukawa’s meson , called a pion (or pi-meson or π- meson), was identified in 1947 by C. F. Powell (1903–

  1. and G. P. Occhialini (1907–1993)  Charged pions have masses of 140 MeV/ c 2 , and a neutral pion π 0 was later discovered that has a mass of 135 MeV/ c 2 , a neutron and a proton.

Yukawa’s Meson

Figure 14.3: A Feynman diagram indicating the exchange of a pion (Yukawa’s meson) between a neutron and a proton.

The Fundamental Interactions

 We have learned that the fundamental forces act through the exchange or mediation of particles according to the quantum theory of fields. The exchanged particle in the electromagnetic interaction is the photon. All particles having either electric charge or a magnetic moment (and also the photon) interact with the electromagnetic interaction. The electromagnetic interaction has very long range.

The Fundamental Interactions

 In the 1960s Sheldon Glashow, Steven Weinberg,

and Abdus Salam (Nobel Prize for Physics, 1979)

predicted that particles, which they called W (for

weak) and Z, should exist that are responsible for

the weak interaction.

 This theory, called the electroweak theory, unified

the electromagnetic and weak interactions much as

Maxwell had unified electricity and magnetism into

the electromagnetic theory a hundred years earlier.

The Graviton

 It has been suggested that the particle responsible for the gravitational interaction be called a graviton.  The graviton is the mediator of gravity in quantum field theory and has been postulated because of the success of the photon in quantum electrodynamics theory.  It must be massless, travel at the speed of light, have spin 2, and interact with all particles that have mass- energy.  The graviton has never been observed because of its extremely weak interaction with objects.

The Fundamental Interactions

14.3: Classification of Elementary Particles

 We discussed in Chapter 9 that articles with half-

integral spin are called fermions and those with

integral spin are called bosons.

 This is a particularly useful way to classify

elementary particles because all stable matter in the

universe appears to be composed, at some level, of

constituent fermions.

Bosons and Fermions

 Photons, gluons, W

±

, and the Z are called gauge

bosons and are responsible for the strong and

electroweak interactions.

 Gravitons are also bosons, having spin 2.

 Fermions exert attractive or repulsive forces on each

other by exchanging gauge bosons, which are the

force carriers.