Physics, M.S. 1

Total Page：16

File Type：pdf, Size：1020Kb

Physics, M.S. 1 PHYSICS, M.S. DEPARTMENT OVERVIEW The Department of Physics has a strong tradition of graduate study and research in astrophysics; atomic, molecular, and optical physics; condensed matter physics; high energy and particle physics; plasma physics; quantum computing; and string theory. There are many facilities for carrying out world-class research (https://www.physics.wisc.edu/ research/areas/). We have a large professional staff: 45 full-time faculty (https://www.physics.wisc.edu/people/staff/) members, afﬁliated faculty members holding joint appointments with other departments, scientists, senior scientists, and postdocs. There are over 175 graduate students in the department who come from many countries around the world. More complete information on the graduate program, the faculty, and research groups is available at the department website (http:// www.physics.wisc.edu). Research specialties include: THEORETICAL PHYSICS Astrophysics; atomic, molecular, and optical physics; condensed matter physics; cosmology; elementary particle physics; nuclear physics; phenomenology; plasmas and fusion; quantum computing; statistical and thermal physics; string theory. EXPERIMENTAL PHYSICS Astrophysics; atomic, molecular, and optical physics; biophysics; condensed matter physics; cosmology; elementary particle physics; neutrino physics; experimental studies of superconductors; medical physics; nuclear physics; plasma physics; quantum computing; spectroscopy. M.S. DEGREES The department offers the master science degree in physics, with two named options: Research and Quantum Computing. The M.S. Physics-Research option (http://guide.wisc.edu/graduate/physics/ physics-ms/physics-research-ms/) is non-admitting, meaning it is only available to students pursuing their Ph.D. The M.S. Physics-Quantum Computing option (http://guide.wisc.edu/graduate/physics/physics-ms/ physics-quantum-computing-ms/) (MSPQC Program) is a professional master's program in an accelerated format designed to be completed in one calendar year..

Copy Link

Recommended publications

Statistics of a Free Single Quantum Particle at a Finite
STATISTICS OF A FREE SINGLE QUANTUM PARTICLE AT A FINITE TEMPERATURE JIAN-PING PENG Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China Abstract We present a model to study the statistics of a single structureless quantum particle freely moving in a space at a finite temperature. It is shown that the quantum particle feels the temperature and can exchange energy with its environment in the form of heat transfer. The underlying mechanism is diffraction at the edge of the wave front of its matter wave. Expressions of energy and entropy of the particle are obtained for the irreversible process. Keywords: Quantum particle at a finite temperature, Thermodynamics of a single quantum particle PACS: 05.30.-d, 02.70.Rr 1 Quantum mechanics is the theoretical framework that describes phenomena on the microscopic level and is exact at zero temperature. The fundamental statistical character in quantum mechanics, due to the Heisenberg uncertainty relation, is unrelated to temperature. On the other hand, temperature is generally believed to have no microscopic meaning and can only be conceived at the macroscopic level. For instance, one can define the energy of a single quantum particle, but one can not ascribe a temperature to it. However, it is physically meaningful to place a single quantum particle in a box or let it move in a space where temperature is well-defined. This raises the well-known question: How a single quantum particle feels the temperature and what is the consequence? The question is particular important and interesting, since experimental techniques in recent years have improved to such an extent that direct measurement of electron dynamics is possible.1,2,3 It should also closely related to the question on the applicability of the thermodynamics to small systems on the nanometer scale.4 We present here a model to study the behavior of a structureless quantum particle moving freely in a space at a nonzero temperature.
[Show full text]
An Original Way of Teaching Geometrical Optics C. Even
Learning through experimenting: an original way of teaching geometrical optics C. Even1, C. Balland2 and V. Guillet3 1 Laboratoire de Physique des Solides, CNRS, Université Paris-Sud, Université Paris-Saclay, F-91405 Orsay, France 2 Sorbonne Universités, UPMC Université Paris 6, Université Paris Diderot, Sorbonne Paris Cite, CNRS-IN2P3, Laboratoire de Physique Nucléaire et des Hautes Energies (LPNHE), 4 place Jussieu, F-75252, Paris Cedex 5, France 3 Institut d’Astrophysique Spatiale, CNRS, Université Paris-Sud, Université Paris-Saclay, F- 91405 Orsay, France E-mail : [email protected] Abstract Over the past 10 years, we have developed at University Paris-Sud a first year course on geometrical optics centered on experimentation. In contrast with the traditional top-down learning structure usually applied at university, in which practical sessions are often a mere verification of the laws taught during preceding lectures, this course promotes “active learning” and focuses on experiments made by the students. Interaction among students and self questioning is strongly encouraged and practicing comes first, before any theoretical knowledge. Through a series of concrete examples, the present paper describes the philosophy underlying the teaching in this course. We demonstrate that not only geometrical optics can be taught through experiments, but also that it can serve as a useful introduction to experimental physics. Feedback over the last ten years shows that our approach succeeds in helping students to learn better and acquire motivation and autonomy. This approach can easily be applied to other fields of physics. Keywords : geometrical optics, experimental physics, active learning 1. Introduction Teaching geometrical optics to first year university students is somewhat challenging, as this field of physics often appears as one of the less appealing to students.
[Show full text]
Physics 357 – Thermal Physics - Spring 2005
Physics 357 – Thermal Physics - Spring 2005 Contact Info MTTH 9-9:50. Science 255 Doug Juers, Science 244, 527-5229, [email protected] Office Hours: Mon 10-noon, Wed 9-10 and by appointment or whenever I’m around. Description Thermal physics involves the study of systems with lots (1023) of particles. Since only a two-body problem can be solved analytically, you can imagine we will look at these systems somewhat differently from simple systems in mechanics. Rather than try to predict individual trajectories of individual particles we will consider things on a larger scale. Probability and statistics will play an important role in thinking about what can happen. There are two general methods of dealing with such systems – a top down approach and a bottom up approach. In the top down approach (thermodynamics) one doesn’t even really consider that there are particles there, and instead thinks about things in terms of quantities like temperature heat, energy, work, entropy and enthalpy. In the bottom up approach (statistical mechanics) one considers in detail the interactions between individual particles. Building up from there yields impressive predictions of bulk properties of different materials. In this course we will cover both thermodynamics and statistical mechanics. The first part of the term will emphasize the former, while the second part of the term will emphasize the latter. Both topics have important applications in many fields, including solid-state physics, fluids, geology, chemistry, biology, astrophysics, cosmology. The great thing about thermal physics is that in large part it’s about trying to deal with reality.
[Show full text]
Typical Course Sequence for Physics/Astronomy
TYPICAL COURSE SEQUENCE FOR PHYSICS/ASTRONOMY Odd Year Entry Freshman Year Fall Spring PHYS-141 Mechanics/Thermal 3 PHYS-142 E & M/Waves 3 PHYS-141L Experimental Physics I 1 PHYS-142L Experimental Physics II 1 PHYS-190 Freshman Seminar 1 MATH-132 Calculus II 4 MATH-131 Calculus I 4 CORE-115 Core 5 CORE-110 Core 5 CC Christ College 8 CC Christ College 8 Total (with Core) 14 Total (with Core) 13 Total (with CC) 17 Total (with CC) 16 Sophomore Year Fall Spring PHYS-243 Modern Physics 3 PHYS-245 Experimental Physics III 1 PHYS-281/281L Electricity/Electronics 3 PHYS-246 Data Reduction and Error... 1 MATH-253 Calculus III 4 PHYS-250 Mechanics 3 CS-157 Algorithms & Programming 3 ASTR-221 Observational Astronomy 1 ASTR-253 Astrophysics - Galaxies 3 MATH-260/270 Linear Alg/Diff Equations 4 MATH-264/270 Linear Alg/Diff Equations 6 Total 13 Total 13 Junior Year Fall Spring PHYS-345 Experimental Physics IV 1 PHYS-422 Quantum Mechanics II 3 PHYS-371 Electromagnetic Fields 3 PHYS-430 Nuclear Physics 3 PHYS-421 Quantum Mechanics I 3 PHYS-430L Nuclear Physics Lab 1 ASTR-252 Astrophysics - Stars 3 Total 7 Total 10 Senior Year Fall Spring PHYS-360 Thermal Physics 3 PHYS-372 Electromagnetic Waves 3 PHYS-381 Advanced Mechanics 3 PHYS-440 Condensed Matter Physics 3 PHYS-440 Condensed Matter Physics 3 PHYS-445 Senior Research 1 PHYS-445 Senior Research 1 MATH-330 Partial Diff. Eq. 3 MATH-334 Complex Variables 3 Total 13 Total 10 Page 1 TYPICAL COURSE SEQUENCE FOR PHYSICS/ASTRONOMY Even Year Entry Freshman Year Fall Spring PHYS-141 Mechanics/Thermal 3 PHYS-142 E & M/Waves 3 PHYS-141L Experimental Physics I 1 PHYS-142L Experimental Physics II 1 PHYS-190 Freshman Seminar 1 MATH-132 Calculus II 4 MATH-131 Calculus I 4 CORE-115 Core 5 CORE-110 Core 5 CC Christ College 8 CC Christ College 8 Total (with Core) 14 Total (with Core) 13 Total (with CC) 17 Total (with CC) 16 Sophomore Year Fall Spring PHYS-243 Modern Physics 3 PHYS-245 Experimental Physics III 1 PHYS-281 Electricity/Electronics 3 PHYS-250 Mechanics 3 MATH-253 Calculus III 4 PHYS-246 Data Reduction and Error..
[Show full text]
Experimental Physics I PHYS 3250/3251
Syllabus Experimental Physics I PHYS 3250/3251 Course Description: Introduction to experimental modern physics, measurement of fundamental constants, repetition of crucial experiments of modern physics (Stern Gerlach, Zeeman effect, photoelectric effect, etc.) Course Objectives: The objective of this course is introduce you to the proper methods for conducting controlled physics experiments, including the acquisition, analysis and physical interpretation of data. The course involves experiments which illustrate the principles of modern physics, e.g. the quantum nature of charge and energy, etc. Succinct, journal-style reports will be the primary output for each experiment, with at least one additional presentation (oral and/or poster) required. Text: An Introduction to Error Analysis, 2nd Edition, J.R. Taylor, ISBN 0-935702-75-X. Additional documentation for any assigned experiments will be supplied as needed. Learning Outcomes: At the conclusion of this course, students will be able to: 1) Assemble and document a relevant bibliography for a physics experiment. 2) Prepare a journal-style manuscript using scientific typesetting software. 3) Plan and conduct experimental measurements in physics while employing proper note-taking methods. 4) Calculate uncertainties for physical quantities derived from experimental measurements. Clemson Thinks2: What is Critical Thinking? This course is designed to be part of the Clemson Thinks2 (CT2) program. “Critical thinking is reasoned and reflective judgment applied to solving problems or making decisions about what to believe or what to do. Critical thinking gives reasoned consideration to defining and analyzing problems, identifying and evaluating options, inferring likely outcomes and probable consequences, and explaining the reasons, evidence, methods and standards used in making those analyses, inferences and evaluations.
[Show full text]
Modern Experimental Physics Introduction for Physics 401 Students
Modern Experimental Physics Introduction for Physics 401 students Spring 2014 Eugene V. Colla • Goals of the course • Experiments • Teamwork • Schedule and assignments • Your working mode Physics 401 Spring 2013 2 • Primary: Learn how to “do” research Each project is a mini-research effort How are experiments actually carried out Use of modern tools and modern analysis and data-recording techniques Learn how to document your work • Secondary: Learn some modern physics Many experiments were once Nobel-prize-worthy efforts They touch on important themes in the development of modern physics Some will provide the insight to understand advanced courses Some are just too new to be discussed in textbooks Physics 401 Spring 2013 3 Primary. Each project is a mini-research effort Step1. Preparing: • Sample preparation • Wiring the setup • Testing electronics Preparing the samples for ferroelectric measurements Courtesy of Emily Zarndt & Mike Skulski (F11) Standing waves resonances in Second Step2. Taking data: Sound experiment If problems – go back to Courtesy of Mae Hwee Teo and Step 1. Vernie Redmon (F11) Physics 401 Spring 2013 4 Primary. Each project is a mini-research effort Plot of coincidence rate for 22Na against the angle between detectors A and B. The fit is a Step3. Data Analysis Gaussian function centred at If data is “bad” or not 179.30° with a full width at half maximum (FWHM) of 14.75°. enough data point – go back to Step 2 Courtesy of Bi Ran and Thomas Woodroof Author#1 and Author#2 Step4. Writing report and preparing the talk Physics 401 Spring 2013 5 Primary.
[Show full text]
On the Shoulders of Giants: a Brief History of Physics in Göttingen
1 6 ON THE SHO UL DERS OF G I A NTS : A B RIEF HISTORY OF P HYSI C S IN G Ö TTIN G EN On the Shoulders of Giants: a brief History of Physics in Göttingen 18th and 19th centuries Georg Ch. Lichtenberg (1742-1799) may be considered the fore- under Emil Wiechert (1861-1928), where seismic methods for father of experimental physics in Göttingen. His lectures were the study of the Earth's interior were developed. An institute accompanied by many experiments with equipment which he for applied mathematics and mechanics under the joint direc- had bought privately. To the general public, he is better known torship of the mathematician Carl Runge (1856-1927) (Runge- for his thoughtful and witty aphorisms. Following Lichtenberg, Kutta method) and the pioneer of aerodynamics, or boundary the next physicist of world renown would be Wilhelm Weber layers, Ludwig Prandtl (1875-1953) complemented the range of (1804-1891), a student, coworker and colleague of the „prince institutions related to physics proper. In 1925, Prandtl became of mathematics“ C. F. Gauss, who not only excelled in electro- the director of a newly established Kaiser-Wilhelm-Institute dynamics but fought for his constitutional rights against the for Fluid Dynamics. king of Hannover (1830). After his re-installment as a profes- A new and well-equipped physics building opened at the end sor in 1849, the two Göttingen physics chairs , W. Weber and B. of 1905. After the turn to the 20th century, Walter Kaufmann Listing, approximately corresponded to chairs of experimen- (1871-1947) did precision measurements on the velocity depen- tal and mathematical physics.
[Show full text]
Physics Ph.D
THE UNIVERSITY OF VERMONT PHYSICS PH.D. PHYSICS PH.D. consists of a Ph.D. dissertation proposal given after the start of a dissertation research project. All students must meet the Requirements for the Doctor of Philosophy Degree (http:// Requirements for Advancement to Candidacy for the catalogue.uvm.edu/graduate/degreerequirements/ Degree of Doctor of Philosophy requirementsforthedoctorofphilosophydegree/). Successful completion of all required courses and the comprehensive exam. OVERVIEW The Department of Physics offers research opportunities in theoretical and experimental condensed matter physics, astronomy and astrophysics, and soft condensed matter physics and biophysics. SPECIFIC REQUIREMENTS Requirements for Admission to Graduate Studies for the Degree of Doctor of Philosophy Undergraduate majors in physics are considered for admission to the program. Satisfactory scores on the Graduate Record Examination (general) are required. Minimum Degree Requirements 75 credits, including: 6 Core Graduate Courses PHYS 301 Mathematical Physics 3 PHYS 311 Advanced Dynamics 3 PHYS 313 Electromagnetic Theory 3 PHYS 323 Contemporary Physics 3 PHYS 362 Quantum Mechanics II 3 PHYS 365 Statistical Mechanics 3 All of these courses must be completed with a grade B or better within the first 2 years of graduate study. To accommodate the needs of the specific subfields in physics such as astrophysics, biological physics, condensed- matter physics and materials physics, 3 elective courses (9 credits) have to be chosen to fulfill the breadth requirement with a grade of B or higher. Elective courses must be completed within the first 3 years of the program, as the fourth year (and beyond if needed) should be dedicated to progress towards the Ph.D.
[Show full text]
Department of Physics and Geosciences 1
Department of Physics and Geosciences 1 Department of Physics and Geosciences Contact Information Chair: Brent Hedquist Phone: 361-593-2618 Email: [email protected] Building Name: Hill Hall Room Number: 113 The Department of Physics and Geosciences serves the needs of three types of students: 1. those majoring in geology or physics and those minoring in geography, geology, GIS, geophysics, or physics 2. technical or pre-professional students; and 3. students who take physics and geoscience courses out of interest or to satisfy science requirements. The department seeks to prepare students who are majoring in geology or physics; minoring in geography, geology, Geographic Information Systems (GIS), geophysics, or physics to compete with graduates from other institutions for industrial and governmental positions, follow a career in science education, or pursue a higher level degree. It does this through fundamental courses in the respective disciplines and through specialized programs in GIS, energy, hydrogeology, groundwater modeling, certification in GIS, certification in Geophysics, and certification in nuclear power plant (NPP) operations. For students in technical areas, the department endeavors to provide the background necessary for success in their chosen profession. For non-technical majors, the department strives to enlighten students concerning some of the basic realities of our universe and to instill in them an appreciation of the methods of scientific inquiry and the impact of science on our modern world. In addition to our undergraduate degrees and minors, we also offer an interdisciplinary graduate program in Petrophysics. Students majoring or minoring in the Department of Physics and Geosciences should plan the course work so that it will best support their career and educational goals.
[Show full text]
Case Western Reserve University
CASE WESTERN RESERVE UNIVERSITY DEPARTMENT OF PHYSICS Cleveland, Ohio 44106-7079 http://physics.cwru.edu General University Information TOEFL requirements President: Barbara Snyder The TOEFL exam is required for students from non-English- Dean of Graduate School: Charles E. Rozek speaking countries. University website: http://www.cwru.edu PBT score: 557 Control: Private iBT score:90 Setting: Urban Other admissions information Total Faculty: 2,745 Additional requirements: No minimum acceptable GRE score is Total number of Students: 9,837 specified. Total number of Graduate Students: 5,610 Undergraduate preparation assumed: Taylor, Classical Mechan- ics; Griffiths, Electrodynamics; Kittel, Thermal Physics; Grif- Department Information fiths, Quantum Mechanics; or equivalent textbooks; one or Department Chairman: Kathleen Kash, Chair two years of advanced laboratory courses. Department Contact: Corbin E. Covault, Director of the Graduate Program Total full-time faculty:25 TUITION Total number of full-time equivalent positions:22 Tuition year 2012–13: Full-Time Graduate Students:60 Tuition for out-of-state residents First-Year Graduate Students:12 Full-time students: $27,828 annual Female First-Year Students:3 Part-time students: $1,546 per credit Total Post Doctorates:15 Credit hours per semester to be considered full-time:9 Deferred tuition plan: Yes Department Address Health insurance: Available at the cost of $1,452 per year. Rockefeller Building Academic term: Semester 2076 Adelbert Road Number of first-year students who receive full tuition
[Show full text]
Module Code SP-1203 Module Title Thermal Physics and Optics Degree
Module code SP-1203 Module Title Thermal Physics and Optics Degree/Diploma Bachelor of Science (Applied Physics) Type of Module Major Core Modular Credits 4 Total student workload 10 hours/week Contact hours 4 hours/week Prerequisite A-level Physics or equivalent Anti-requisite SP-1303 Thermal Physics and Optics Aims This module aims to provide students with a logical presentation of the basic concepts and principles of thermal physics and optics in physics and strengthen the understanding of the concepts and principles through a range of real-life applications. Learning Outcomes: On successful completion of this module, a student will be expected to be able to: Lower order : 30% - recognise the three phases of matter: solid, liquid and gas, how their properties depends on thermal motion and the forces between atoms and molecules - describe the fundamental concepts related to various forms of energy: internal, enthalpy, entropy, free internal energy and free enthalpy - describe the basic concept of thermal equilibrium - describe the basic phenomena due to light matter interaction. Middle order : 60% - describe polarization and the properties of polarizing components - describe the concept of quantum nature of light and discuss the limitations of classical optics, derive the thermodynamic temperature scale from the operation of an ideal Carnot heat engine -recognise the fundamental limits for the efficiency of heat engine Higher order: 10% - describe interferometer principles and its applications. - describe and apply the basic principles of geometrical optics. - describe the kinetic theory of gases and how this theory can be applied to what is actually observed in real gases - explain and use laws of thermodynamics to solve simple problems related with heat and work changes to practical systems.
[Show full text]
Research in High Energy Physics
,*•'••' Annual Technical Progress Report and FY 1997 Budget Request for DOE Grant DE-FG03-94ER40833 to The U.S. Department of Energy San Francisco Operations Office from The University of Hawaii Honolulu, Hawaii 96822 Title of Project: RESEARCH IN HIGH ENERGY PHYSICS December 1, 1993 to November 30, 1998 (FY94-FY98) Principal Investigators Stephen L. Olsen Xerxes Tata Experimental Physics Theoretical Physics G<: fun DOCUMENT IS UMJTO ASTER Contents 1 Introduction 2 1.1 Overview 2 1.1.1 Background 3 1.1.2 Recent Accomplishments 4 1.1.3 Personnel Changes 5 2 Accelerator-Based Experiments 6 2.1 The BELLE Experiment 6 2.1.1 Physics Motivation 6 2.1.2 The BELLE Detector 7 2.1.3 Hawaii Participation in BELLE 10 2.1.4 BELLE Equipment Budget 18 2.1.5 Detector Integration 19 2.1.6 Budget 19 2.1.7 Publications 19 2.2 The BES Experiment 21 2.2.1 V' Physics 21 2.2.2 Xc Physics 31 2.2.3 Charm Physics: measurement of fz>a and fn 34 2.2.4 CODEMAN 35 2.2.5 The BES upgrade 35 2.2.6 Recent BES publications: 38 2.3 The CLEO-II Experiment 41 2.3.1 Studies of inclusive B Meson decays 41 2.3.2 Search for the process b —• s gluon 42 2.3.3 Exclusive hadronic B decays 45 ii DISCLAIMER Portions of this document may be illegible in electronic image products. Images are produced from the best available original document 2.3.4 Determination of CKM matrix elements 47 2.3.5 Bs - Bs Mixing 47 2.3.6 Doubly Cabibbo-suppressed D° meson decay and D° — D° mixing 48 2.3.7 CLEO II particle ID 49 2.3.8 Reviews of B Physics 51 2.4 The DO Experiment 53 2.4.1 Top Mass Fitting 53 2.4.2 Hawaii analyses to extract the top mass 56 2.4.3 Another pseudolikelihood fit 58 2.4.4 Optimal cuts 59 2.4.5 HT analysis 62 2.4.6 Personnel 64 2.4.7 Other Activities 64 2.4.8 Future Plans 64 2.4.9 Publications 64 2.5 The AMY Experiment .
[Show full text]