Elementary Particle Physics
... imagine that we aim a beam of highly energetic protons towards a target also consisting of protons (can be realised as a tank of liquid hydrogen). If the target is thin, a large number of protons in the incoming beam will just pass through the target, while a few will react with target particles. Th ...
... imagine that we aim a beam of highly energetic protons towards a target also consisting of protons (can be realised as a tank of liquid hydrogen). If the target is thin, a large number of protons in the incoming beam will just pass through the target, while a few will react with target particles. Th ...
Review 4
... USE ENERGY EQUATIONS IF YOU ARE ASKED FOR VELOCITY IN TERMS OF POSITION, OR POSITION IN TERMS OF VELOCITY! Note that the equations W Fx|| and P Fv|| are equivalent to W F|| x and P F|| v and W Fx cos ...
... USE ENERGY EQUATIONS IF YOU ARE ASKED FOR VELOCITY IN TERMS OF POSITION, OR POSITION IN TERMS OF VELOCITY! Note that the equations W Fx|| and P Fv|| are equivalent to W F|| x and P F|| v and W Fx cos ...
4. Star formation 4.1 Jeans` criterion
... • Hence gravitational energy is radiated away on a thermal (Kelvin) timescale, tK~107 – 108 y. • Star remains close to hydrostatic equilibrium so we can continue to use Virial theorem. AS 3003 ...
... • Hence gravitational energy is radiated away on a thermal (Kelvin) timescale, tK~107 – 108 y. • Star remains close to hydrostatic equilibrium so we can continue to use Virial theorem. AS 3003 ...
CHAPTER 2 The nucleus and radioactive decay - Cin
... = 7.7423 MeV) as a function of mass number, e.g. EB/A. Except for mass numbers below ~20 u, it can be seen that EB/A is remarkably constant, lying between 7 and 10 MeV per nucleon. This feature indicates that the binding energy increases approximately linearly with mass number. Another feature of th ...
... = 7.7423 MeV) as a function of mass number, e.g. EB/A. Except for mass numbers below ~20 u, it can be seen that EB/A is remarkably constant, lying between 7 and 10 MeV per nucleon. This feature indicates that the binding energy increases approximately linearly with mass number. Another feature of th ...
Notes in pdf format
... • Conservation laws are very important • They are also useful for solving Problems • We have talked about several of them: Energy conservation Linear momentum conservation Angular momentum conservation ...
... • Conservation laws are very important • They are also useful for solving Problems • We have talked about several of them: Energy conservation Linear momentum conservation Angular momentum conservation ...
Friday`s Slides
... Which, if any, of your responses to questions 1, 2, 3, or 4 would change if the magnitude of F1 was twice as great as the magnitude of F2 ? ...
... Which, if any, of your responses to questions 1, 2, 3, or 4 would change if the magnitude of F1 was twice as great as the magnitude of F2 ? ...
Cosmology - RHIG - Wayne State University
... The evolution of luminous matter Standard model is symmetric. All degrees of freedom are massless. Electro-weak symmetry breaking via Higgs field (Dm of W, Z, g) Mechanism to generate current quark masses (but does not explain their magnitude) ...
... The evolution of luminous matter Standard model is symmetric. All degrees of freedom are massless. Electro-weak symmetry breaking via Higgs field (Dm of W, Z, g) Mechanism to generate current quark masses (but does not explain their magnitude) ...
Binary evolution in a nutshell
... Here we made the assumption that the fraction of the stellar mass available for hydrogen fusion is the same for all stars. In reality, this factor will vary; it is ∼ 0.15 for the Sun, but may be much larger for more massive stars, for example because they have convective cores and can mix material f ...
... Here we made the assumption that the fraction of the stellar mass available for hydrogen fusion is the same for all stars. In reality, this factor will vary; it is ∼ 0.15 for the Sun, but may be much larger for more massive stars, for example because they have convective cores and can mix material f ...
Force and Newton Laws
... • For every reaction, there is an equal and opposite reaction. • Forces always occur in pairs when acting on an object. Second object of two objects will exert a force equal to the force the first object originally exerted. • Never act on the same object or could be combined. (same magnitude but opp ...
... • For every reaction, there is an equal and opposite reaction. • Forces always occur in pairs when acting on an object. Second object of two objects will exert a force equal to the force the first object originally exerted. • Never act on the same object or could be combined. (same magnitude but opp ...
CHAPTER 2: Special Theory of Relativity
... Note that we are free to interpret what is K and what is K’, so we need concepts of proper time and length ...
... Note that we are free to interpret what is K and what is K’, so we need concepts of proper time and length ...