Physics: Intro to Nuclear Physics Notes
The four forces in the universe: gravity, strong force, weak force, electromagnetism
Gravity is attraction between objects
Gravity is only significant for very large objects
Electromagnetism Creates magnetism
Holds chemical bonds together
Creates electricity
Strong & weak Forces act in the nucleus of the atom
The Strong Force
The glue that binds the nucleus together
When you release the energy in the nucleus, you get a nuclear bomb and nuclear energy
Fission
Very large unstable nuclei can fall apart or can be split
Purpose is to create large amounts of energy
Nuclear Chain Reaction
Neutron is added making the atom unstable
Atom falls apart
Loss of mass and release of energy
Utilized in WW2 and nuclear power plants
Fusion
Occurs under high pressure and temperature
Small nuclei combine to form large nuclei
Cannot be controlled
The Sun turns hydrogen into helium
Heavier elements are made in supernovas and in star collisions
Huge amounts of energy are released by fusion
Used in hydrogen bomb (not WW 2 Bomb) and stars
Albert Einstein determined that a small amount of mass contains a large amount of energy
Equation: E+mc^2
The amount of mass lost when the WW2 Bombs dropped on Japan: 0.7 grams
The amount of mass the Sun converts to energy each second: 5 million tons
The amount of years till the Sun runs out of fuel (hydrogen): 5 billion years
The Weak Force
Takes place in the nucleus
The weak force is Radioactive BETA decay
A neutron turns into a proton and an electron
Beta decay is responsible for
Irritating hydrogen in fusion stars
Plate tectonics
Carbon 14 dating of organic objects
Carbon Dating
Cosmic rays cause all living things to be radioactive
Used to date items up to 60,000 years old
Amount of atomic bombs tested on Earth: 2,000
Wave Particle Duality
Light can behave like a wave or a particle
Light is a transverse wave
Light does not need a medium
Light also travels in particles called photons
Young’s Double Slit Experiment showed that light can behave as both a particle and a wave
Two waves combine form an interference wave
Spectroscopy
Elements can be identified by their atomic spectrum
Each type of light corresponds to a specific energy
Visible light spectrum in order from least to greatest energy “ROY-G-BIV” Highest energy is violet, lowest energy is red
Higher orbits have higher energy
When jumping from a low level to a higher level you add energy
When falling from a higher level to a lower level you remove energy
Photons are emitted from the atom when an electron falls in energy
The color of the photon emitted is related to the amount of energy released
Spectroscopy: dispersion of light into its available spectrum
the two types of spectra: continuous, discrete
In a continuous spectrum, light is composed of a wide unbroken range of colors
Materials that create a continuous spectrum: stars and galaxies
A discrete spectrum only has lines at very distinct colors
Every element and chemical has a different emission spectrum
The Photoelectric Effect
Einstein won the Nobel Prize in 1921for the photoelectric effect
The photoelectric effect: the emission of electrons when electromagnetic radiation (light) falls on an object
Three things that happen during the photoelectric effect:
A light photon hits an object
Energy transfers from the photon to the object
If the energy is great enough an electron will be ejected by the object
The threshold frequency is the minimum energy required to eject an electron
If energy is below the threshold frequency, no emission
If energy is equal to or greater than the threshold frequency, electron emitted
Only the frequency determines the energy
The amount of light (intensity) does not matter
Different substances have different thresholds
Different light has different energy