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Physics 121 Exam Sheet - BYU Physics and Astronomy
Physics 121 Exam Sheet - BYU Physics and Astronomy

Physics_AP_A_Evans_Day_39_Period_4
Physics_AP_A_Evans_Day_39_Period_4

Presentation
Presentation

Applications of gamma spectrometry
Applications of gamma spectrometry

Homework 1 Solution
Homework 1 Solution

Nuclear Force and Weak Interaction
Nuclear Force and Weak Interaction

Structure of Physics
Structure of Physics

The Atom
The Atom

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Summary Notes Template

... information and use available evidence to assess the contributions made by Heisenberg and Pauli to the development of atomic theory ...
PerturbationTheory
PerturbationTheory

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Core Idea PS2 Motion and Stability: Forces and Interactions How
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... exerted force (friction, elastic pushes and pulls) electric, magnetic, and gravitational forces magnets (push or pull at a distance) size (of the forces) properties of the objects forces between two magnets (depend on their orientation relative to each other) gravitational force of Earth ...
Classes of Particles - Liberty Union
Classes of Particles - Liberty Union

... during the junior or senior years since many players will not have completed them before encountering the subject matter at tournaments. One high-yield area of physics to study is the nomenclature of various groups of particles. Some conventions: The mass of particles is usually given in mega-electr ...
QCD and Nuclei
QCD and Nuclei

... approaching from below, hadronic interactions become very weak Assume between the PT point and the “flash point” (at which hadrons become strongly interacting), hadrons flow “freely” with little interaction Brown Rule (after Bethe): Set equal to zero! ...
The Strong interaction or the mystery of the nucleus - Pierre
The Strong interaction or the mystery of the nucleus - Pierre

...  This theory is similar than quantum electrodynamics with the major differences being:  The strong interaction only acts at short distance scale, binding all elements that have a strong charge together  The force become weaker as the energy increases  Asymptotic freedom: allows for quark collisi ...
Nuclear Probabilities
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... In Beta- decay, a neutron emits an electron and antineutrino and becomes a proton. We can see this occur if we consider the neutron to consist of 2 down quarks and 1 up quark. The extra energy in the unstable isotope undergoing the decay is converted into a neutrino / anti-neutrino pair. One of the ...
Exact factorization of the time-dependent electron
Exact factorization of the time-dependent electron

... of the BO approximation. Yet, this is “just” an approximation, and some of the most fascinating phenomena of condensed-matter physics, like superconductivity, appear in the regime where the BO approximation is not valid. This raises the question: If one were to solve the Schrödinger equation of the ...
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Work – Energy Principle

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Aluminum Isotope symbol 13 protons 13 neutrons 10 electrons

... Atomic mass is calculated using the mass of the protons and neutrons. Most of the mass resides in the nucleus. The electrons are so light that it would take approximately 2000 of them to equal the mass of l proton or neutron. Therefore we don’t really need them to calculate the mass of the atom. Ato ...
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PowerPoint 演示文稿

... While uranium-235 is the naturally occuring fissionable isotope, there are other isotopes which can be induced to fission by neutron bombardment. Plutonium-239 is also fissionable by bombardment with slow neutrons, and both it and uranium-235 have been used to make nuclear fission bombs. Plutonium-2 ...
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PROBLEMS conservation of energy/energy/work 1.A)How much

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HW6.2: Work, Energy and Power

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Elementary Particles Fundamental forces in Nature
Elementary Particles Fundamental forces in Nature

... Soon after the quark theory was proposed, it was suggested that quarks have another property, called color, or color charge. Unlike other quantum numbers, color takes on three values. Real particles must be colorless; this explains why only 3-quark and quark–antiquark configurations are seen. Color ...
Chapter 30 - Mosinee School District
Chapter 30 - Mosinee School District

... Although produced by the strong interaction, they do not decay into particles that interact via the strong interaction, but instead into particles that interact via weak interactions ...
Fundamental Forces of Nature
Fundamental Forces of Nature

... One of the four fundamental forces, the weak interaction involves the exchange of the intermediate vector bosons, the W and the Z. Since the mass of these particles is on the order of 80 GeV, the uncertainty principle dictates a range of about 1018meters which is about 0.1% of the diameter of a prot ...
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Nuclear force



The nuclear force (or nucleon–nucleon interaction or residual strong force) is the force between protons and neutrons, subatomic particles that are collectively called nucleons. The nuclear force is responsible for binding protons and neutrons into atomic nuclei. Neutrons and protons are affected by the nuclear force almost identically. Since protons have charge +1 e, they experience a Coulomb repulsion that tends to push them apart, but at short range the nuclear force is sufficiently attractive as to overcome the electromagnetic repulsive force. The mass of a nucleus is less than the sum total of the individual masses of the protons and neutrons which form it. The difference in mass between bound and unbound nucleons is known as the mass defect. Energy is released when nuclei break apart, and it is this energy that used in nuclear power and nuclear weapons.The nuclear force is powerfully attractive between nucleons at distances of about 1 femtometer (fm, or 1.0 × 10−15 metres) between their centers, but rapidly decreases to insignificance at distances beyond about 2.5 fm. At distances less than 0.7 fm, the nuclear force becomes repulsive. This repulsive component is responsible for the physical size of nuclei, since the nucleons can come no closer than the force allows. By comparison, the size of an atom, measured in angstroms (Å, or 1.0 × 10−10 m), is five orders of magnitude larger. The nuclear force is not simple, however, since it depends on the nucleon spins, has a tensor component, and may depend on the relative momentum of the nucleons.A quantitative description of the nuclear force relies on partially empirical equations that model the internucleon potential energies, or potentials. (Generally, forces within a system of particles can be more simply modeled by describing the system's potential energy; the negative gradient of a potential is equal to the vector force.) The constants for the equations are phenomenological, that is, determined by fitting the equations to experimental data. The internucleon potentials attempt to describe the properties of nucleon–nucleon interaction. Once determined, any given potential can be used in, e.g., the Schrödinger equation to determine the quantum mechanical properties of the nucleon system.The discovery of the neutron in 1932 revealed that atomic nuclei were made of protons and neutrons, held together by an attractive force. By 1935 the nuclear force was conceived to be transmitted by particles called mesons. This theoretical development included a description of the Yukawa potential, an early example of a nuclear potential. Mesons, predicted by theory, were discovered experimentally in 1947. By the 1970s, the quark model had been developed, which showed that the mesons and nucleons were composed of quarks and gluons. By this new model, the nuclear force, resulting from the exchange of mesons between neighboring nucleons, is a residual effect of the strong force.
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