Neutron-Proton Collisions
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James Chadwick: Ahead of His Time
July 15, 2020 James Chadwick: ahead of his time Gerhard Ecker University of Vienna, Faculty of Physics Boltzmanngasse 5, A-1090 Wien, Austria Abstract James Chadwick is known for his discovery of the neutron. Many of his earlier findings and ideas in the context of weak and strong nuclear forces are much less known. This biographical sketch attempts to highlight the achievements of a scientist who paved the way for contemporary subatomic physics. arXiv:2007.06926v1 [physics.hist-ph] 14 Jul 2020 1 Early years James Chadwick was born on Oct. 20, 1891 in Bollington, Cheshire in the northwest of England, as the eldest son of John Joseph Chadwick and his wife Anne Mary. His father was a cotton spinner while his mother worked as a domestic servant. In 1895 the parents left Bollington to seek a better life in Manchester. James was left behind in the care of his grandparents, a parallel with his famous predecessor Isaac Newton who also grew up with his grandmother. It might be an interesting topic for sociologists of science to find out whether there is a correlation between children educated by their grandmothers and future scientific geniuses. James attended Bollington Cross School. He was very attached to his grandmother, much less to his parents. Nevertheless, he joined his parents in Manchester around 1902 but found it difficult to adjust to the new environment. The family felt they could not afford to send James to Manchester Grammar School although he had been offered a scholarship. Instead, he attended the less prestigious Central Grammar School where the teaching was actually very good, as Chadwick later emphasised. -
10. Collisions • Use Conservation of Momentum and Energy and The
10. Collisions • Use conservation of momentum and energy and the center of mass to understand collisions between two objects. • During a collision, two or more objects exert a force on one another for a short time: -F(t) F(t) Before During After • It is not necessary for the objects to touch during a collision, e.g. an asteroid flied by the earth is considered a collision because its path is changed due to the gravitational attraction of the earth. One can still use conservation of momentum and energy to analyze the collision. Impulse: During a collision, the objects exert a force on one another. This force may be complicated and change with time. However, from Newton's 3rd Law, the two objects must exert an equal and opposite force on one another. F(t) t ti tf Dt From Newton'sr 2nd Law: dp r = F (t) dt r r dp = F (t)dt r r r r tf p f - pi = Dp = ò F (t)dt ti The change in the momentum is defined as the impulse of the collision. • Impulse is a vector quantity. Impulse-Linear Momentum Theorem: In a collision, the impulse on an object is equal to the change in momentum: r r J = Dp Conservation of Linear Momentum: In a system of two or more particles that are colliding, the forces that these objects exert on one another are internal forces. These internal forces cannot change the momentum of the system. Only an external force can change the momentum. The linear momentum of a closed isolated system is conserved during a collision of objects within the system. -
12. Elastic Collisions A) Overview B) Elastic Collisions V
12. Elastic Collisions A) Overview In this unit, our focus will be on elastic collisions, namely those collisions in which the only forces that act during the collision are conservative forces. In these collisions, the sum of the kinetic energies of the objects is conserved. We will find that the description of these collisions is significantly simplified in the center of mass frame of the colliding objects. In particular, we will discover that, in this frame, the speed of each object after the collision is the same as its speed before the collision. B) Elastic Collisions In the last unit, we discussed the important topic of momentum conservation. In particular, we found that when the sum of the external forces acting on a system of particles is zero, then the total momentum of the system, defined as the vector sum of the individual momenta, will be conserved. We also determined that the kinetic energy of the system, defined to be the sum of the individual kinetic energies, is not necessarily conserved in collisions. Whether or not this energy is conserved is determined by the details of the forces that the components of the system exert on each other. In the last unit, our focus was on inelastic collisions, those collisions in which the kinetic energy of the system was not conserved. In particular non-conservative work was done by the forces that the individual objects exerted on each other during the collision. In this unit, we will look at examples in which the only forces that act during the collision are conservative forces. -
Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean Transformations
World Journal of Mechanics, 2020, 10, 154-165 https://www.scirp.org/journal/wjm ISSN Online: 2160-0503 ISSN Print: 2160-049X Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean Transformations Akihiro Ogura Laboratory of Physics, Nihon University, Matsudo, Japan How to cite this paper: Ogura, A. (2020) Abstract Collisions in Classical Mechanics in Terms of Mass-Momentum “Vectors” with Galilean We present the usefulness of mass-momentum “vectors” to analyze the colli- Transformations. World Journal of Mechan- sion problems in classical mechanics for both one and two dimensions with ics, 10, 154-165. Galilean transformations. The Galilean transformations connect the mass- https://doi.org/10.4236/wjm.2020.1010011 momentum “vectors” in the center-of-mass and the laboratory systems. We Received: August 28, 2020 show that just moving the two systems to and fro, we obtain the final states in Accepted: October 9, 2020 the laboratory systems. This gives a simple way of obtaining them, in contrast Published: October 12, 2020 with the usual way in which we have to solve the simultaneous equations. For Copyright © 2020 by author(s) and one dimensional collision, the coefficient of restitution is introduced in the Scientific Research Publishing Inc. center-of-mass system. This clearly shows the meaning of the coefficient of This work is licensed under the Creative restitution. For two dimensional collisions, we only discuss the elastic colli- Commons Attribution International sion case. We also discuss the case of which the target particle is at rest before License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ the collision. -
Definitions and Concepts for AQA Physics a Level
Definitions and Concepts for AQA Physics A Level Topic 4: Mechanics and Materials Breaking Stress: The maximum stress that an object can withstand before failure occurs. Brittle: A brittle object will show very little strain before reaching its breaking stress. Centre of Mass: The single point through which all the mass of an object can be said to act. Conservation of Energy: Energy cannot be created or destroyed - it can only be transferred into different forms. Conservation of Momentum: The total momentum of a system before an event, must be equal to the total momentum of the system after the event, assuming no external forces act. Couple: Two equal and opposite parallel forces that act on an object through different lines of action. It has the effect of causing a rotation without translation. Density: The mass per unit volume of a material. Efficiency: The ratio of useful output to total input for a given system. Elastic Behaviour: If a material deforms with elastic behaviour, it will return to its original shape when the deforming forces are removed. The object will not be permanently deformed. Elastic Collision: A collision in which the total kinetic energy of the system before the collision is equal to the total kinetic energy of the system after the collision. Elastic Limit: The force beyond which an object will no longer deform elastically, and instead deform plastically. Beyond the elastic limit, when the deforming forces are removed, the object will not return to its original shape. Elastic Strain Energy: The energy stored in an object when it is stretched. -
Bibliography of Low Energy Electron
Bibliography of Low Energy Electron Collision Cross Section Data United States Department of Commerce National Bureau of Standards Miscellaneous Publication 289 — THE NATIONAL BUREAU OF STANDARDS The National Bureau of Standards 1 provides measurement and technical information services essential to the efficiency and effectiveness of the work of the Nation's scientists and engineers. The Bureau serves also as a focal point in the Federal Government for assuring maximum application of the physical and engineering sciences to the advancement of technology in industry and commerce. To accomplish this mission, the Bureau is organized into three institutes covering broad program areas of research and services: THE INSTITUTE FOR BASIC STANDARDS . provides the central basis within the United States for a complete and consistent system of physical measurements, coordinates that system with the measurement systems of other nations, and furnishes essential services leading to accurate and uniform physical measurements throughout the Nation's scientific community, industry, and commerce. This Institute comprises a series of divisions, each serving a classical subject matter area: —Applied Mathematics—Electricity—Metrology—Mechanics—Heat—Atomic Physics—Physical Chemistry—Radiation Physics—Laboratory Astrophysics 2—Radio Standards Laboratory, 2 which includes Radio Standards Physics and Radio Standards Engineering—Office of Standard Refer- ence Data. THE INSTITUTE FOR MATERIALS RESEARCH . conducts materials research and provides associated materials services including mainly reference materials and data on the properties of ma- terials. Beyond its direct interest to the Nation's scientists and engineers, this Institute yields services which are essential to the advancement of technology in industry and commerce. This Institute is or- ganized primarily by technical fields: —Analytical Chemistry—Metallurgy—Reactor Radiations—Polymers—Inorganic Materials—Cry- ogenics 2—Materials Evaluation Laboratory-— Office of Standard Reference Materials. -
The Effects of Elastic Scattering in Neutral Atom Transport D
The effects of elastic scattering in neutral atom transport D. N. Ruzic Citation: Phys. Fluids B 5, 3140 (1993); doi: 10.1063/1.860651 View online: http://dx.doi.org/10.1063/1.860651 View Table of Contents: http://pop.aip.org/resource/1/PFBPEI/v5/i9 Published by the American Institute of Physics. Related Articles Dissociation mechanisms of excited CH3X (X = Cl, Br, and I) formed via high-energy electron transfer using alkali metal targets J. Chem. Phys. 137, 184308 (2012) Efficient method for quantum calculations of molecule-molecule scattering properties in a magnetic field J. Chem. Phys. 137, 024103 (2012) Scattering resonances in slow NH3–He collisions J. Chem. Phys. 136, 074301 (2012) Accurate time dependent wave packet calculations for the N + OH reaction J. Chem. Phys. 135, 104307 (2011) The k-j-j′ vector correlation in inelastic and reactive scattering J. Chem. Phys. 135, 084305 (2011) Additional information on Phys. Fluids B Journal Homepage: http://pop.aip.org/ Journal Information: http://pop.aip.org/about/about_the_journal Top downloads: http://pop.aip.org/features/most_downloaded Information for Authors: http://pop.aip.org/authors Downloaded 23 Dec 2012 to 192.17.144.173. Redistribution subject to AIP license or copyright; see http://pop.aip.org/about/rights_and_permissions The effects of elastic scattering in neutral atom transport D. N. Ruzic University of Illinois, 103South Goodwin Avenue, Urbana Illinois 61801 (Received 14 December 1992; accepted21 May 1993) Neutral atom elastic collisions are one of the dominant interactions in the edge of a high recycling diverted plasma. Starting from the quantum interatomic potentials, the scattering functions are derived for H on H ‘, H on Hz, and He on Hz in the energy range of 0. -
Energy Considerations in Collisions How It Works
L-8 (M-7) I. Collisions II. Work and Energy • Momentum: an object of mass m, moving with velocity v has a momentum p = m v. • Momentum is an important and useful concept that is used to analyze collisions – The colliding objects exert strong forces on each other over relatively short time intervals – Details of the forces are usually not known, but the forces acting on the objects are equal in magnitude and opposite in direction (3rd law) – The law of conservation of momentum which follows from Newton’s 2nd and 3rd laws, allows us to predict what happens in collisions 1 2 I. Physics of collisions: Law of Conservation of Momentum conservation of momentum • A consequence of Newton’s Newton’s Cradle 3rd law is that if we add the • The concept of momentum is very useful momentum of both objects when discussing how 2 objects interact. before a collision, it is the same as the momentum of • Suppose two objects are on a collision the two objects immediately course. AB after the collision. • We know their masses and speeds before • The law of conservation of momentum and the law of they collide conservation of energy are During the short time of • The momentum concept helps us to two of the fundamental laws of nature. the collision, the effect of predict what will happen after they collide. gravity is not important. 3 4 Momentum conservation in a two-body collision, Energy considerations in collisions How it works. v • Objects that are in motion have kinetic energy: v B, before A, before KE = ½ m v2 (Note that KE does not depend on before B collision A the direction of the object’s motion) more on this . -
Collisions and Momentum
1 Collisions and Momentum Introduction: The important vector quantities in physics are the momentum and force. Force is defined as the time rate of change of the momentum. The momentum (p) of an object is given by the product of its mass (a scalar) and its velocity (a vector): p = m v Since the force is the rate of change of the momentum, we would expect that if the force is zero, then the momentum would remain constant. This is the basis for Newton’s first law of motion. We also find that in the case of a collision between two objects of different momenta, the total momentum, which is the vector sum of the momenta of the two individual objects, will not change as a result of the collision if no external force is acting on the objects. If you have ever played billiards, you probably made good use of this rule. This is the rule of conservation of momentum. Another quantity in physics is the kinetic energy (K.E.), a scalar quantity defined as: 1 2 K.E. = 2 mv The kinetic energy is one half the mass multiplied by the velocity squared. An elastic collision is a collision where the total kinetic energy (the sum of the energies of the colliding objects) is conserved (the same both before and after the collision). An inelastic collision is one where the kinetic energy is not conserved. (It is important to remember that in both kinds of collisions the total energy of the colliding objects is conserved.) In this experiment we will study the collision of two steel balls to test the law of conservation of momentum and to test the elasticity of such a collision by comparing the kinetic energies of the balls before and after the collision. -
Ultra-Cold Collisions and Evaporative Cooling of Caesium in a Magnetic Trap
Ultra-cold Collisions and Evaporative Cooling of Caesium in a Magnetic Trap Angharad Mair Thomas A thesis submitted in partial fulfilment of the requirements for the degree of Doctor of Philosophy at the University of Oxford Jesus College University of Oxford Hilary Term 2004 Abstract Ultra-cold Collisions and Evaporative Cooling of Caesium in a Magnetic Trap Angharad Mair Thomas, Jesus College, Oxford University DPhil Thesis, Hilary Term 2004 Caesium-133 atoms have been evaporatively cooled in a magnetic trap to tem- peratures as low as 8 nK producing a final phase-space density within a factor of 4 of that required for the onset of Bose-Einstein condensation. At the end of the forced radio-frequency evaporation, 1500 atoms in the F = 3; mF = ¡3 state remain in the magnetic trap. A decrease in the one-dimensional evaporative cool- ing efficiency at very low temperatures is observed as the trapped sample enters the collisionally thick (hydrodynamic) regime. Different evaporation trajectories are experimentally studied leading to a greater understanding of one-dimensional evaporation, inelastic collisions and the hydrodynamic regime. A theoretical sim- ulation accurately reproduces the experimental data and indicates that the reduc- tion in the evaporative cooling efficiency as the cloud enters the hydrodynamic regime is the main obstacle to the realization of Bose-Einstein condensation in the F = 3; mF = ¡3 state. In addition, we report measurements of the two-body inelastic collision rate coefficient for caesium atoms as a function of magnetic field and collision energy. The positions of three previously identified resonances are confirmed, with reduced uncertainties, at magnetic fields of 108.87(6), 118.46(3) and 133.52(3) Gauss. -
Section 7: BASIC NUCLEAR CONCEPTS
BPA BASIC NUCLEAR CONCEPTS Section 7: BASIC NUCLEAR CONCEPTS In this section, we present a basic description of atomic nuclei, the stored energy contained within them, their occurrence and stability Basic Nuclear Concepts EARLY DISCOVERIES [see also Section 2] Radioactivity - discovered in 1896 by Henri Becquerel. Types of radiation observed: alpha ( ) rays (4He nuclei); beta ( ) rays (electrons) ; gamma ( ) rays (photons) Proposed atomic models: built of positively and negatively charged components. - Planetary model: Light electrons (-charge) orbiting a massive nucleus (+charge): - 'Plum pudding' model (J. J. Thompson): In this model, electrons are embedded but free to move in an extended region of positive charge filling the entire volume of the atom. Thompson found it difficult to develop this model. For example he could not account for the patterns of discrete wavelengths in light emitted from excited atoms. In the early 1900s, Rutherford and co-workers, by performing experiments scattering particles off gold, confirmed the planetary model with a small, massive nucleus at its centre. The problem of the stability of such an atom was realized early on but not explained until the development of quantum mechanics [see Section 3]. Discovery of the neutron 1932 – The neutron was identified by James Chadwick from observations of the effects of radiation emitted when beryllium is bombarded with alpha particles. This gave the basic nuclear framework (Heisenberg, Majorana and Wigner) that the nucleus consists of nucleons (neutrons and protons) held together by a strong, short-range binding force, with a strength independent of the type of nucleon. Nuclear size and density Scattering experiments showed that the nuclear radius varies as cube root of the mass number A, 1/3 i.e. -
From the Natural Transmutations of Uranium to Its Artificial Fission
O T T O H AH N From the natural transmutations of uranium to its artificial fission Nobel Lecture, December 13, 1946 The year 1946 marked a jubilee in the history of the chemical element, ura- nium. Fifty years earlier, in the spring of 1896, Henri Becquerel had discov- ered the remarkable radiation phenomena of this element, which were at that time grouped together under the name of radioactivity. For more than 100 years, uranium, discovered by W. H. Klaproth in 1789, had had a quiet existence as a somewhat rare but not particularly interesting element. After its inclusion in the Periodic System by D. Mendeleev and Lothar Meyer, it was distinguished from all the other elements in one partic- ular respect: it occupied the highest place in the table of the elements. As yet, however, that did not have any particular significance. We know today that it is just this position of uranium at the highest place of the then known chemical elements which gives it the important properties by which it is distinguished from all other elements. The echo of Becquerel’s fundamental observations on the radioactivity of uranium in scientific circles was at first fairly weak. Two years later, how- ever, they acquired an exceptional importance when the Curies succeeded in separating from uranium minerals two active substances, polonium and ra- dium, of which the latter appeared to be several million times stronger than the same weight of uranium. It was only a few years before the first surprising property of this "ra- diating" substance was explained.