The collision probability method in 1D part 2

Size: px
Start display at page:

Download "The collision probability method in 1D part 2"

Transcription

1 The collision probability method in 1D part 2 Alain Hébert alain.hebert@polymtl.ca Institut de génie nucléaire École Polytechnique de Montréal ENE611: Week 9 The collision probability method in 1D part 2 1/25

2 Content (week 9) 1 Calculation of 1D collision probabilities plane 2D geometry cylindrical 1D geometry spherical 1D geometry ENE611: Week 9 The collision probability method in 1D part 2 2/25

3 The collision probability method 1 Consider an infinite lattice of unit cells, each of them represented as i V i V i represents the infinite set of regions V i belonging to all the cells in the lattice The sources of secondary neutrons are uniform and equal to Q i on each region V i. The collision probabilityp ij,g is the probability for a neutron born uniformally and isotropically in any of the regions V i of the lattice to undergo its first collision in region V j of a unit cell or assembly. If the total cross section Σ(r) is constant and equal to Σ j in region V j, reduced CPs are (1) p ij = P ij Σ j = 1 4πV i V i d 3 r d 3 r e τ(s) V j s 2 where the optical path τ(s) is given by (2) τ(s) = s ds Σ(r s Ω). ENE611: Week 9 The collision probability method in 1D part 2 3/25

4 Plane 2D geometry 1 We will now study the case of a 2D geometry defined in the x y plane and homogeneous along the z axis. A cylinder or tube of infinite length is an example of such a geometry. In this case, it is possible to integrate analytically the integral transport equation along the axial angle θ. This angle is use to define the direction cosine of the particle relative to the z axis. z Ω r = (x,y,z) The direction of the particle is Ω = sinθ cosǫi+sinθ sinǫj +cosθk. Integration over θ is possible by taking the projection of each particle free path on the x y plane. We write θ y d 2 Ω = dθdǫ sinθ x ε (x,y) (3) τ(ρ) = τ(s) sinθ dρ = ds sinθ where ρ is the projection of s on the x y plane. ENE611: Week 9 The collision probability method in 1D part 2 4/25

5 Plane 2D geometry 2 We will limit ourself on the integration of the integral transport equation, defined on the domain of a unique unit cell. We use the relations r = r +sω and d 3 r = s 2 d 2 Ωds and obtain (4) p ij = 1 4πV i d 3 r V i 4π d 2 Ω dse τ(s) I j where the quantity I j is the set of points belonging simultaneously to the half straight line of origin r and direction Ω; to volume V j of the unit cell. With the help of figure, Eq. (4) can be rewritten as (5) p ij = 1 4πV i 2π dǫ d 2 r V i π dθ dρe I j τ(ρ) sinθ where V i now represents a surface in the x y plane and I j is the set of points belonging simultaneously to the half straight line of origin r and direction ǫ; to surface V j of the unit cell. ENE611: Week 9 The collision probability method in 1D part 2 5/25

6 Bickley functions 1 Bickley functions are defined as (6) with n 1. Ki n (x) = π/2 dθ sin n 1 θe x sinθ = π/2 dθ cos n 1 θe x cosθ Ki1(x) Ki2(x) Ki3(x) The following equations are relating Bickley functions of different orders: x x du Ki n (u) = Ki n+1 (x) Ki n+1 (x ),.5 Ki4(x) Ki5(x) and d dx Ki n(x) = Ki n 1 (x) x They can be evaluated efficiently using the matlab scriptakin. ENE611: Week 9 The collision probability method in 1D part 2 6/25

7 Plane 2D geometry 1 Equation (5) can be simplified by introducing the Bickley functions. We obtain (7) p ij = 1 2πV i 2π dǫ d 2 r dρki 1 [τ(ρ)]. V i I j Sets of integration lines, referred as tracks, are draw over the complete domain. Each set is characterized by a given angle ǫ and contains parallel tracks covering the domain. Tracks in a set can be separated by a constant distance h or can be placed at optimal locations, as depicted in sub-figures (a) and (b), respectively. Each track is used forward and backward, corresponding to angles ǫ and ǫ. Three-point formula h Three-point formula Three-point formula (a) Rectangular quadrature (b) Gaussian quadrature ENE611: Week 9 The collision probability method in 1D part 2 7/25

8 Plane 2D geometry 2 In the case of convex volumes i and j, Eq. (7) can be rewritten as (8) p ij = 1 2πV i 2π dǫ hmax h min dh lj dl dl Ki 1 (τ ij +Σ i l +Σ j l) if i j where τ ij is the optical path of the materials between regions i and j and (9) p ii = 1 2πV i 2π dǫ hmax h min dh dl l dl Ki 1 [Σ i (l l )]. y V i l l i l ij l j l' r V j r' h ε x ENE611: Week 9 The collision probability method in 1D part 2 8/25

9 Cylindrical 1D geometry 1 In the case of 1D cylindrical geometry, the tracks are identical for any value of the angle ǫ. track 1 track 2 The tubular volumes are concave, making extra terms to appear. The corresponding geometry is depicted in figure. Two tracks are represented, both contributing to collision probability components p ij with i < j and p ii. Track 1 corresponds to the integration domain where region i is concave and track 2 corresponds to the integration domain where it is convex. In this figure, τ ij and τ ii are the optical paths of the materials located between regions i and j or between two instances of region i. Vj Vi l j l j τij l i τii r j-1/2 r l i-1/2 i r i+1/2 l i l j l j r j+1/2 ENE611: Week 9 The collision probability method in 1D part 2 9/25

10 Cylindrical 1D geometry 2 In this case, Eq. (8) can be rewritten as (1) p ij { = 2 ri 1/2 dh V i + lj dl dl ] + Ki 1 (τ ij +Σ i l +Σ j l) ri+1/2 r i 1/2 dh [ Ki 1 [(τ ij +τ ii +Σ i l i )+Σ i l +Σ j l] } lj dl dl Ki 1 (τ ij +Σ i l +Σ j l) if i < j where r i±1/2 are the radii bounding region i and Eq. (9) can be rewritten as { p ii = 2 ri 1/2 dh V i (11) + ri+1/2 r i 1/2 dh dl dl [2 dl Ki 1 [Σ i (l l )]+ l } l dl Ki 1 [Σ i (l l )] dl Ki 1 [τ ii +Σ i (l +l)] where the first and second terms are the contributions from tracks 1 and 2, respectively. ] ENE611: Week 9 The collision probability method in 1D part 2 1/25

11 Cylindrical 1D geometry 3 These equations can be simplified by introducing the following definitions: (12) C ij (τ ) = lj dl dl Ki 1 (τ +Σ i l +Σ j l) and (13) so that (14) D i = dl dl Ki 1 [Σ i (l l )] l { p ij = 2 ri 1/2 dh[c ij (τ ij +τ ii +Σ i l i )+C ij (τ ij )]+ V i if i < j, and ri+1/2 r i 1/2 dhc ij (τ ij ) } (15) { p ii = 2 ri 1/2 dh[2d i +C ii (τ ii )]+ V i ri+1/2 r i 1/2 dhd i }. ENE611: Week 9 The collision probability method in 1D part 2 11/25

12 Cylindrical 1D geometry 4 Integration in l and l is next performed, leading to the following relations: a)σ i andσ j : 1 [ C ij (τ ) = Ki 3 (τ ) Ki 3 (τ +Σ i l i ) Ki 3 (τ +Σ j l j ) Σ i Σ j ] + Ki 3 (τ +Σ i l i +Σ j l j ) b)σ i = andσ j : c)σ i andσ j = : C ij (τ ) = l i Σ j [Ki 2 (τ ) Ki 2 (τ +Σ j l j )] C ij (τ ) = l j Σ i [Ki 2 (τ ) Ki 2 (τ +Σ i l i )] d)σ i = Σ j = : C ij (τ ) = l i l j Ki 1 (τ ) ENE611: Week 9 The collision probability method in 1D part 2 12/25

13 Cylindrical 1D geometry 5 e)σ i : f)σ i = : D i = l i Σ i 1 Σ 2 i [Ki 3 () Ki 3 (Σ i l i )] D i = πl2 i 4. ENE611: Week 9 The collision probability method in 1D part 2 13/25

14 Cylindrical 1D geometry 6 The above relations are implemented in Matlab using the following two scripts: function f=cij_f(tau,sigi,sigj,segmenti,segmentj) if sigi = && sigj = f=(akin(3,tau)-akin(3,tau+sigi*segmenti)-... akin(3,tau+sigj*segmentj)+... akin(3,tau+sigi*segmenti+sigj*segmentj))/(sigi*sigj) ; elseif sigi == && sigj = f=(akin(2,tau)-akin(2,tau+sigj*segmentj))*segmenti/sigj ; elseif sigi = && sigj == f=(akin(2,tau)-akin(2,tau+sigi*segmenti))*segmentj/sigi ; else f=akin(1,tau)*segmenti*segmentj ; end function f=di_f(sig,segment) if sig = f=segment/sig-(akin(3,)-akin(3,sig*segment))/sigˆ2 ; else f=pi*segmentˆ2/4 ; end ENE611: Week 9 The collision probability method in 1D part 2 14/25

15 Tracking 1 The tracking of 1D cylindrical and spherical geometries is similar and can be generated with the same algorithm. A matlab scriptf=sybt1d(rad,lgsph,ngauss) is presented to produce a tracking object in these cases. The figure presents an example with I = 2 regions and K = 2 tracks per regions. Tracks 1 and 2 have two segments, identified as l 1 and l 2. Tracks 3 and 4 have only one segment, identified as l φ l 2 3 l 2 l 2 l 1 l 1 l 2 h 1 h 3 h 2 h 4 h ENE611: Week 9 The collision probability method in 1D part 2 15/25

16 Tracking 2 A K point Gauss-Jacobi quadrature is used The four tracks are obtained using rad=[.75.15] ; track=sybt1d(rad,false,2) ; track(i,j) is a 2D cell array containing I K elements, one per track. The i index refers to the tracks located in r i 1/2 < h < r i+1/2. The (i,j) th cell is also a cell array containing three elements: the weight w k of the track, the product w k cosφ, a 1D array of dimension I i+1 containing the track segments. The l 1 segment length of track 2 is l2=track{1,2}{3}(1) leading tol2 = Any lengthtrack{ik,il}{3}(1) corresponding to a segment that cross the h axis must be multiplied by 2. 2 l 2 l 1 1 l 2 l 1 4 l 2 φ 3 l 2 h 1 h 3 h 2 h 4 h ENE611: Week 9 The collision probability method in 1D part 2 16/25

17 Tracking 3 The following script will perform a numerical integration of p 11 in 1D cylindrical tube of radius rad and macroscopic total cross sectionsigt: function f=p11_cyl(rad,sigt) % compute the p11 component in 1D cylindrical geometry track=sybt1d(rad,false,5) ; val= ; for i=1:5 segment=2*track{1,i}{3}(1) ; if sigt = d=segment/sigt-(akin(3,)-akin(3,sigt*segment))/sigtˆ2 ; else d=pi*segmentˆ2/4 ; end val=val+track{1,i}{1}*d ; end f=val/(pi*radˆ2) ; ENE611: Week 9 The collision probability method in 1D part 2 17/25

18 Boundary conditions 1 The external boundary condition of a 1D cylindrical geometry is introduced by choosing an albedo β + set to zero for representing a voided boundary, or set to one for representing reflection of particles. The voided boundary condition is similar to the vacuum condition used for 1D slab geometry. The reflecting boundary condition is implemented in the context of the Wigner-Seitz approximation for lattice calculations in reactor physics. The Wigner-Seitz approximation consists of replacing the exact boundary with an equivalent cylindrical boundary, taking care to conserve the amount of moderator present in the cell. The correct condition in this case is the white boundary condition in which the particles are reflected with an isotropic angular distribution. Fuel Fuel ENE611: Week 9 The collision probability method in 1D part 2 18/25

19 Boundary conditions 2 The application of a white boundary condition is based on the transformation of the reduced collision probability matrix P = {p ij, i = 1,I and j = 1,I} corresponding to a vacuum boundary condition. We first compute the escape probability vector P is = {P is, i = 1,I}, a column vector whose components are obtained from (16) I P is = 1 p ij Σ j j=1 representing the probability for a neutron born in region i to escape from the unit cell without collision. The probability for a neutron entering in the unit cell by its boundary, with an isotropic angular distribution, to first collide in region i is represented by the component P Si. It is possible to show that (17) where S is the surface of the boundary. p Si = P Si Σ i = 4V i S P is ENE611: Week 9 The collision probability method in 1D part 2 19/25

20 Boundary conditions 3 The transmission probability P SS is therefore given as (18) P SS = 1 I p Si Σ i. i=1 The reduced collision probability matrix P = { p ij, i = 1,I and j = 1,I} corresponding to a white boundary condition can now be obtained using P = P+P is [ β + +(β + ) 2 P SS +(β + ) 3 P 2 SS +(β+ ) 4 P 3 SS +...] p Sj or, using a geometric progression, as (19) P = P+ β + 1 β + P SS P is p Sj. The collision probability matrix P can be scattering-reduced and used in the matrix flux equation of the CP method. ENE611: Week 9 The collision probability method in 1D part 2 2/25

21 Spherical 1D geometry 1 Computing the tracking and collision probabilities in 1D spherical geometry is similar to the cylindrical geometry case. The tracking is obtained by thesybt1d Matlab script The expression of reduced collision probabilities is written (2) p ij = 1 d 3 r V i V i I j dse τ(s) ENE611: Week 9 The collision probability method in 1D part 2 21/25

22 Spherical 1D geometry 2 which can be rewritten as (21) p ij = 2π V i { ri 1/2 dhh ] + e (τ ij+σ i l +Σ j l) + ri+1/2 r i 1/2 dhh lj dl dl } lj dl dl e (τ ij+σ i l +Σ j l) [ e [(τ ij+τ ii +Σ i l i )+Σ i l +Σ j l] if i < j where r i±1/2 are the radii bounding region i and (22) p ii = 2π V i + { ri 1/2 dhh ri+1/2 r i 1/2 dhh dl dl [2 l dl e [Σ i (l l l dl e [Σ i (l l )] } )] + dl e [τ ii+σ i (l +l)] where the first and second terms are the contributions from tracks 1 and 2, respectively. ] ENE611: Week 9 The collision probability method in 1D part 2 22/25

23 Spherical 1D geometry 3 These equations can be simplified by introducing the following definitions: (23) C ij (τ ) = lj dl dl e (τ +Σ i l +Σ j l) and (24) so that p ij = 2π V i (25) D i = dl l dl e Σ i (l l { ri 1/2 dhh[c ij (τ ij +τ ii +Σ i l i )+C ij (τ ij )]+ ) ri+1/2 r i 1/2 dhhc ij (τ ij ) } if i < j and (26) p ii = 2π V i { ri 1/2 dhh[2d i +C ii (τ ii )]+ ri+1/2 r i 1/2 dhhd i }. ENE611: Week 9 The collision probability method in 1D part 2 23/25

24 Spherical 1D geometry 4 Integration in l and l is next performed, leading to the following relations: a)σ i andσ j : C ij (τ ) = 1 Σ i Σ j [ e τ e (τ +Σ i l i ) e (τ +Σ j l j ) +e (τ +Σ i l i +Σ j l j ) ] b)σ i = andσ j : c)σ i andσ j = : d)σ i = Σ j = : C ij (τ ) = l i Σ j [ e τ e (τ +Σ j l j ) ] C ij (τ ) = l j Σ i [ e τ e (τ +Σ i l i ) ] C ij (τ ) = l i l j e τ ENE611: Week 9 The collision probability method in 1D part 2 24/25

25 Spherical 1D geometry 5 e)σ i : f)σ i = : D i = l i Σ i 1 Σ 2 i [1 e Σ i l i ] D i = l2 i 2. ENE611: Week 9 The collision probability method in 1D part 2 25/25

The collision probability method in 1D part 1

The collision probability method in 1D part 1 The collision probability method in 1D part 1 Alain Hébert alain.hebert@polymtl.ca Institut de génie nucléaire École Polytechnique de Montréal ENE6101: Week 8 The collision probability method in 1D part

More information

Space-time kinetics. Alain Hébert. Institut de génie nucléaire École Polytechnique de Montréal.

Space-time kinetics. Alain Hébert. Institut de génie nucléaire École Polytechnique de Montréal. Space-time kinetics Alain Hébert alain.hebert@polymtl.ca Institut de génie nucléaire École Polytechnique de Montréal ENE613: Week 1 Space-time kinetics 1/24 Content (week 1) 1 Space-time kinetics equations

More information

Serco Assurance. Resonance Theory and Transport Theory in WIMSD J L Hutton

Serco Assurance. Resonance Theory and Transport Theory in WIMSD J L Hutton Serco Assurance Resonance Theory and Transport Theory in WIMSD J L Hutton 2 March 2004 Outline of Talk Resonance Treatment Outline of problem - pin cell geometry U 238 cross section Simple non-mathematical

More information

Discrete Euclidean Curvature Flows

Discrete Euclidean Curvature Flows Discrete Euclidean Curvature Flows 1 1 Department of Computer Science SUNY at Stony Brook Tsinghua University 2010 Isothermal Coordinates Relation between conformal structure and Riemannian metric Isothermal

More information

The multigroup Monte Carlo method part 1

The multigroup Monte Carlo method part 1 The multigroup Monte Carlo method part 1 Alain Hébert alain.hebert@polymtl.ca Institut de génie nucléaire École Polytechnique de Montréal ENE6103: Week 11 The multigroup Monte Carlo method part 1 1/23

More information

THREE-DIMENSIONAL INTEGRAL NEUTRON TRANSPORT CELL CALCULATIONS FOR THE DETERMINATION OF MEAN CELL CROSS SECTIONS

THREE-DIMENSIONAL INTEGRAL NEUTRON TRANSPORT CELL CALCULATIONS FOR THE DETERMINATION OF MEAN CELL CROSS SECTIONS THREE-DIMENSIONAL INTEGRAL NEUTRON TRANSPORT CELL CALCULATIONS FOR THE DETERMINATION OF MEAN CELL CROSS SECTIONS Carsten Beckert 1. Introduction To calculate the neutron transport in a reactor, it is often

More information

Extensions of the TEP Neutral Transport Methodology. Dingkang Zhang, John Mandrekas, Weston M. Stacey

Extensions of the TEP Neutral Transport Methodology. Dingkang Zhang, John Mandrekas, Weston M. Stacey Extensions of the TEP Neutral Transport Methodology Dingkang Zhang, John Mandrekas, Weston M. Stacey Fusion Research Center, Georgia Institute of Technology, Atlanta, GA 30332-0425, USA Abstract Recent

More information

Numerical methods part 2

Numerical methods part 2 Numerical methods part 2 Alain Hébert alain.hebert@polymtl.ca Institut de génie nucléaire École Polytechnique de Montréal ENE6103: Week 6 Numerical methods part 2 1/33 Content (week 6) 1 Solution of an

More information

PC4262 Remote Sensing Scattering and Absorption

PC4262 Remote Sensing Scattering and Absorption PC46 Remote Sensing Scattering and Absorption Dr. S. C. Liew, Jan 003 crslsc@nus.edu.sg Scattering by a single particle I(θ, φ) dφ dω F γ A parallel beam of light with a flux density F along the incident

More information

SEAFLOOR MAPPING MODELLING UNDERWATER PROPAGATION RAY ACOUSTICS

SEAFLOOR MAPPING MODELLING UNDERWATER PROPAGATION RAY ACOUSTICS 3 Underwater propagation 3. Ray acoustics 3.. Relevant mathematics We first consider a plane wave as depicted in figure. As shown in the figure wave fronts are planes. The arrow perpendicular to the wave

More information

xy 2 e 2z dx dy dz = 8 3 (1 e 4 ) = 2.62 mc. 12 x2 y 3 e 2z 2 m 2 m 2 m Figure P4.1: Cube of Problem 4.1.

xy 2 e 2z dx dy dz = 8 3 (1 e 4 ) = 2.62 mc. 12 x2 y 3 e 2z 2 m 2 m 2 m Figure P4.1: Cube of Problem 4.1. Problem 4.1 A cube m on a side is located in the first octant in a Cartesian coordinate system, with one of its corners at the origin. Find the total charge contained in the cube if the charge density

More information

2. The Steady State and the Diffusion Equation

2. The Steady State and the Diffusion Equation 2. The Steady State and the Diffusion Equation The Neutron Field Basic field quantity in reactor physics is the neutron angular flux density distribution: Φ( r r, E, r Ω,t) = v(e)n( r r, E, r Ω,t) -- distribution

More information

Electromagnetic Field Theory (EMT)

Electromagnetic Field Theory (EMT) Electromagnetic Field Theory (EMT) Lecture # 9 1) Coulomb s Law and Field Intensity 2) Electric Fields Due to Continuous Charge Distributions Line Charge Surface Charge Volume Charge Coulomb's Law Coulomb's

More information

1. ELECTRIC CHARGES AND FIELDS

1. ELECTRIC CHARGES AND FIELDS 1. ELECTRIC CHARGES AND FIELDS 1. What are point charges? One mark questions with answers A: Charges whose sizes are very small compared to the distance between them are called point charges 2. The net

More information

Lesson 9: Multiplying Media (Reactors)

Lesson 9: Multiplying Media (Reactors) Lesson 9: Multiplying Media (Reactors) Laboratory for Reactor Physics and Systems Behaviour Multiplication Factors Reactor Equation for a Bare, Homogeneous Reactor Geometrical, Material Buckling Spherical,

More information

Applied Nuclear Physics (Fall 2006) Lecture 19 (11/22/06) Gamma Interactions: Compton Scattering

Applied Nuclear Physics (Fall 2006) Lecture 19 (11/22/06) Gamma Interactions: Compton Scattering .101 Applied Nuclear Physics (Fall 006) Lecture 19 (11//06) Gamma Interactions: Compton Scattering References: R. D. Evans, Atomic Nucleus (McGraw-Hill New York, 1955), Chaps 3 5.. W. E. Meyerhof, Elements

More information

Integrals in cylindrical, spherical coordinates (Sect. 15.7)

Integrals in cylindrical, spherical coordinates (Sect. 15.7) Integrals in clindrical, spherical coordinates (Sect. 15.7 Integration in spherical coordinates. Review: Clindrical coordinates. Spherical coordinates in space. Triple integral in spherical coordinates.

More information

Lesson 8: Slowing Down Spectra, p, Fermi Age

Lesson 8: Slowing Down Spectra, p, Fermi Age Lesson 8: Slowing Down Spectra, p, Fermi Age Slowing Down Spectra in Infinite Homogeneous Media Resonance Escape Probability ( p ) Resonance Integral ( I, I eff ) p, for a Reactor Lattice Semi-empirical

More information

Optical Imaging Chapter 5 Light Scattering

Optical Imaging Chapter 5 Light Scattering Optical Imaging Chapter 5 Light Scattering Gabriel Popescu University of Illinois at Urbana-Champaign Beckman Institute Quantitative Light Imaging Laboratory http://light.ece.uiuc.edu Principles of Optical

More information

Problem Solving 1: Line Integrals and Surface Integrals

Problem Solving 1: Line Integrals and Surface Integrals A. Line Integrals MASSACHUSETTS INSTITUTE OF TECHNOLOY Department of Physics Problem Solving 1: Line Integrals and Surface Integrals The line integral of a scalar function f ( xyz),, along a path C is

More information

Chapter 21: Gauss law Tuesday September 13 th. Gauss law and conductors Electrostatic potential energy (more likely on Thu.)

Chapter 21: Gauss law Tuesday September 13 th. Gauss law and conductors Electrostatic potential energy (more likely on Thu.) Chapter 21: Gauss law Tuesday September 13 th LABS START THIS WEEK Quick review of Gauss law The flux of a vector field The shell theorem Gauss law for other symmetries A uniformly charged sheet A uniformly

More information

Chapter 1 The Electric Force

Chapter 1 The Electric Force Chapter 1 The Electric Force 1. Properties of the Electric Charges 1- There are two kinds of the electric charges in the nature, which are positive and negative charges. - The charges of opposite sign

More information

Maxwell s equations for electrostatics

Maxwell s equations for electrostatics Maxwell s equations for electrostatics October 6, 5 The differential form of Gauss s law Starting from the integral form of Gauss s law, we treat the charge as a continuous distribution, ρ x. Then, letting

More information

Nuclear Reactor Physics I Final Exam Solutions

Nuclear Reactor Physics I Final Exam Solutions .11 Nuclear Reactor Physics I Final Exam Solutions Author: Lulu Li Professor: Kord Smith May 5, 01 Prof. Smith wants to stress a couple of concepts that get people confused: Square cylinder means a cylinder

More information

Lesson 6: Diffusion Theory (cf. Transport), Applications

Lesson 6: Diffusion Theory (cf. Transport), Applications Lesson 6: Diffusion Theory (cf. Transport), Applications Transport Equation Diffusion Theory as Special Case Multi-zone Problems (Passive Media) Self-shielding Effects Diffusion Kernels Typical Values

More information

Simple benchmark for evaluating self-shielding models

Simple benchmark for evaluating self-shielding models Simple benchmark for evaluating self-shielding models The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation As Published Publisher

More information

51. General Surface Integrals

51. General Surface Integrals 51. General urface Integrals The area of a surface in defined parametrically by r(u, v) = x(u, v), y(u, v), z(u, v) over a region of integration in the input-variable plane is given by d = r u r v da.

More information

MCRT L10: Scattering and clarification of astronomy/medical terminology

MCRT L10: Scattering and clarification of astronomy/medical terminology MCRT L10: Scattering and clarification of astronomy/medical terminology What does the scattering? Shape of scattering Sampling from scattering phase functions Co-ordinate frames Refractive index changes

More information

Monte Carlo Radiation Transfer I

Monte Carlo Radiation Transfer I Monte Carlo Radiation Transfer I Monte Carlo Photons and interactions Sampling from probability distributions Optical depths, isotropic emission, scattering Monte Carlo Basics Emit energy packet, hereafter

More information

The Dancoff correction. in various geometries. /. Carlvik, B. Pershagen

The Dancoff correction. in various geometries. /. Carlvik, B. Pershagen AE-16 The Dancoff correction in various geometries /. Carlvik, B. Pershagen AKTIEBOLAGET ATOMENERGI STOCKHOLM SWEDEN 1959 AE-16 The Dancoff correction in various geometries I. Carhik, B. Persbagen Summary;

More information

Introduction to Condensed Matter Physics

Introduction to Condensed Matter Physics Introduction to Condensed Matter Physics Diffraction I Basic Physics M.P. Vaughan Diffraction Electromagnetic waves Geometric wavefront The Principle of Linear Superposition Diffraction regimes Single

More information

Note: Each problem is worth 14 points except numbers 5 and 6 which are 15 points. = 3 2

Note: Each problem is worth 14 points except numbers 5 and 6 which are 15 points. = 3 2 Math Prelim II Solutions Spring Note: Each problem is worth points except numbers 5 and 6 which are 5 points. x. Compute x da where is the region in the second quadrant between the + y circles x + y and

More information

PHYS 390 Lecture 23 - Photon gas 23-1

PHYS 390 Lecture 23 - Photon gas 23-1 PHYS 39 Lecture 23 - Photon gas 23-1 Lecture 23 - Photon gas What's Important: radiative intensity and pressure stellar opacity Text: Carroll and Ostlie, Secs. 9.1 and 9.2 The temperature required to drive

More information

SENIOR_ 2017_CLASS_12_PHYSICS_ RAPID REVISION_1_ DERIVATIONS IN FIRST FIVE LESSONS Page 1

SENIOR_ 2017_CLASS_12_PHYSICS_ RAPID REVISION_1_ DERIVATIONS IN FIRST FIVE LESSONS Page 1 INDIAN SCHOOL MUSCAT Department of Physics Class XII Rapid Revision -1 DERIVATIONS IN FIRST FIVE LESSONS 1) Field due to an infinite long straight charged wire Consider an uniformly charged wire of infinite

More information

3 Chapter. Gauss s Law

3 Chapter. Gauss s Law 3 Chapter Gauss s Law 3.1 Electric Flux... 3-2 3.2 Gauss s Law (see also Gauss s Law Simulation in Section 3.10)... 3-4 Example 3.1: Infinitely Long Rod of Uniform Charge Density... 3-9 Example 3.2: Infinite

More information

14.1. Multiple Integration. Iterated Integrals and Area in the Plane. Iterated Integrals. Iterated Integrals. MAC2313 Calculus III - Chapter 14

14.1. Multiple Integration. Iterated Integrals and Area in the Plane. Iterated Integrals. Iterated Integrals. MAC2313 Calculus III - Chapter 14 14 Multiple Integration 14.1 Iterated Integrals and Area in the Plane Objectives Evaluate an iterated integral. Use an iterated integral to find the area of a plane region. Copyright Cengage Learning.

More information

Math 3435 Homework Set 11 Solutions 10 Points. x= 1,, is in the disk of radius 1 centered at origin

Math 3435 Homework Set 11 Solutions 10 Points. x= 1,, is in the disk of radius 1 centered at origin Math 45 Homework et olutions Points. ( pts) The integral is, x + z y d = x + + z da 8 6 6 where is = x + z 8 x + z = 4 o, is the disk of radius centered on the origin. onverting to polar coordinates then

More information

Instructions: No books. No notes. Non-graphing calculators only. You are encouraged, although not required, to show your work.

Instructions: No books. No notes. Non-graphing calculators only. You are encouraged, although not required, to show your work. Exam 3 Math 850-007 Fall 04 Odenthal Name: Instructions: No books. No notes. Non-graphing calculators only. You are encouraged, although not required, to show your work.. Evaluate the iterated integral

More information

Tutorial on Surface Ricci Flow, Theory, Algorithm and Application

Tutorial on Surface Ricci Flow, Theory, Algorithm and Application Tutorial on Surface Ricci Flow, Theory, Algorithm and Application 1 1 Department of Computer Science University of New York at Stony Brook Graduate Summer School: Computer Vision, IPAM, UCLA Collaborators

More information

6. LIGHT SCATTERING 6.1 The first Born approximation

6. LIGHT SCATTERING 6.1 The first Born approximation 6. LIGHT SCATTERING 6.1 The first Born approximation In many situations, light interacts with inhomogeneous systems, in which case the generic light-matter interaction process is referred to as scattering

More information

Graduate Written Examination Spring 2014 Part I Thursday, January 16th, :00am to 1:00pm

Graduate Written Examination Spring 2014 Part I Thursday, January 16th, :00am to 1:00pm Graduate Written Examination Spring 2014 Part I Thursday, January 16th, 2014 9:00am to 1:00pm University of Minnesota School of Physics and Astronomy Examination Instructions Part 1 of this exam consists

More information

Introduction and Vectors Lecture 1

Introduction and Vectors Lecture 1 1 Introduction Introduction and Vectors Lecture 1 This is a course on classical Electromagnetism. It is the foundation for more advanced courses in modern physics. All physics of the modern era, from quantum

More information

Downloaded from

Downloaded from Question 1.1: What is the force between two small charged spheres having charges of 2 10 7 C and 3 10 7 C placed 30 cm apart in air? Repulsive force of magnitude 6 10 3 N Charge on the first sphere, q

More information

Answer sheet: Final exam for Math 2339, Dec 10, 2010

Answer sheet: Final exam for Math 2339, Dec 10, 2010 Answer sheet: Final exam for Math 9, ec, Problem. Let the surface be z f(x,y) ln(y + cos(πxy) + e ). (a) Find the gradient vector of f f(x,y) y + cos(πxy) + e πy sin(πxy), y πx sin(πxy) (b) Evaluate f(,

More information

Multiple Choice. Compute the Jacobian, (u, v), of the coordinate transformation x = u2 v 4, y = uv. (a) 2u 2 + 4v 4 (b) xu yv (c) 3u 2 + 7v 6

Multiple Choice. Compute the Jacobian, (u, v), of the coordinate transformation x = u2 v 4, y = uv. (a) 2u 2 + 4v 4 (b) xu yv (c) 3u 2 + 7v 6 .(5pts) y = uv. ompute the Jacobian, Multiple hoice (x, y) (u, v), of the coordinate transformation x = u v 4, (a) u + 4v 4 (b) xu yv (c) u + 7v 6 (d) u (e) u v uv 4 Solution. u v 4v u = u + 4v 4..(5pts)

More information

Solutions: Homework 7

Solutions: Homework 7 Solutions: Homework 7 Ex. 7.1: Frustrated Total Internal Reflection a) Consider light propagating from a prism, with refraction index n, into air, with refraction index 1. We fix the angle of incidence

More information

f dr. (6.1) f(x i, y i, z i ) r i. (6.2) N i=1

f dr. (6.1) f(x i, y i, z i ) r i. (6.2) N i=1 hapter 6 Integrals In this chapter we will look at integrals in more detail. We will look at integrals along a curve, and multi-dimensional integrals in 2 or more dimensions. In physics we use these integrals

More information

Geometrical models for spheroidal cosmological voids

Geometrical models for spheroidal cosmological voids Geometrical models for spheroidal cosmological voids talk by: Osvaldo M. Moreschi collaborator: Ezequiel Boero FaMAF, Universidad Nacional de Córdoba, Instituto de Física Enrique Gaviola (IFEG), CONICET,

More information

UNIVERSITY OF CALIFORNIA - SANTA CRUZ DEPARTMENT OF PHYSICS PHYS 110A. Homework #6. Benjamin Stahl. February 17, 2015

UNIVERSITY OF CALIFORNIA - SANTA CRUZ DEPARTMENT OF PHYSICS PHYS 110A. Homework #6. Benjamin Stahl. February 17, 2015 UNIVERSITY OF CALIFORNIA - SANTA CRUZ DEPARTMENT OF PHYSICS PHYS A Homework #6 Benjamin Stahl February 7, 5 GRIFFITHS, 5.9 The magnetic field at a point, P, will be found for each of the steady current

More information

ANTENNAS. Vector and Scalar Potentials. Maxwell's Equations. E = jωb. H = J + jωd. D = ρ (M3) B = 0 (M4) D = εe

ANTENNAS. Vector and Scalar Potentials. Maxwell's Equations. E = jωb. H = J + jωd. D = ρ (M3) B = 0 (M4) D = εe ANTENNAS Vector and Scalar Potentials Maxwell's Equations E = jωb H = J + jωd D = ρ B = (M) (M) (M3) (M4) D = εe B= µh For a linear, homogeneous, isotropic medium µ and ε are contant. Since B =, there

More information

Math Exam IV - Fall 2011

Math Exam IV - Fall 2011 Math 233 - Exam IV - Fall 2011 December 15, 2011 - Renato Feres NAME: STUDENT ID NUMBER: General instructions: This exam has 16 questions, each worth the same amount. Check that no pages are missing and

More information

One side of each sheet is blank and may be used as scratch paper.

One side of each sheet is blank and may be used as scratch paper. Math 244 Spring 2017 (Practice) Final 5/11/2017 Time Limit: 2 hours Name: No calculators or notes are allowed. One side of each sheet is blank and may be used as scratch paper. heck your answers whenever

More information

Neutron reproduction. factor ε. k eff = Neutron Life Cycle. x η

Neutron reproduction. factor ε. k eff = Neutron Life Cycle. x η Neutron reproduction factor k eff = 1.000 What is: Migration length? Critical size? How does the geometry affect the reproduction factor? x 0.9 Thermal utilization factor f x 0.9 Resonance escape probability

More information

CANONICAL EQUATIONS. Application to the study of the equilibrium of flexible filaments and brachistochrone curves. By A.

CANONICAL EQUATIONS. Application to the study of the equilibrium of flexible filaments and brachistochrone curves. By A. Équations canoniques. Application a la recherche de l équilibre des fils flexibles et des courbes brachystochrones, Mem. Acad. Sci de Toulouse (8) 7 (885), 545-570. CANONICAL EQUATIONS Application to the

More information

Analysis of Scattering of Radiation in a Plane-Parallel Atmosphere. Stephanie M. Carney ES 299r May 23, 2007

Analysis of Scattering of Radiation in a Plane-Parallel Atmosphere. Stephanie M. Carney ES 299r May 23, 2007 Analysis of Scattering of Radiation in a Plane-Parallel Atmosphere Stephanie M. Carney ES 299r May 23, 27 TABLE OF CONTENTS. INTRODUCTION... 2. DEFINITION OF PHYSICAL QUANTITIES... 3. DERIVATION OF EQUATION

More information

Physics 208, Spring 2016 Exam #3

Physics 208, Spring 2016 Exam #3 Physics 208, Spring 206 Exam #3 A Name (Last, First): ID #: Section #: You have 75 minutes to complete the exam. Formulae are provided on an attached sheet. You may NOT use any other formula sheet. You

More information

NEUTRAL PARTICLE TRANSPORT IN PLASMA EDGE USING TRANSMISSION/ESCAPE PROBABILITY (TEP) METHOD

NEUTRAL PARTICLE TRANSPORT IN PLASMA EDGE USING TRANSMISSION/ESCAPE PROBABILITY (TEP) METHOD NEUTRAL PARTICLE TRANSPORT IN PLASMA EDGE USING TRANSMISSION/ESCAPE PROBABILITY (TEP) METHOD A Dissertation Presented to The Academic Faculty By Dingkang Zhang In Partial Fulfillment of the Requirements

More information

Chapter 22. Dr. Armen Kocharian. Gauss s Law Lecture 4

Chapter 22. Dr. Armen Kocharian. Gauss s Law Lecture 4 Chapter 22 Dr. Armen Kocharian Gauss s Law Lecture 4 Field Due to a Plane of Charge E must be perpendicular to the plane and must have the same magnitude at all points equidistant from the plane Choose

More information

ROTATING RING. Volume of small element = Rdθbt if weight density of ring = ρ weight of small element = ρrbtdθ. Figure 1 Rotating ring

ROTATING RING. Volume of small element = Rdθbt if weight density of ring = ρ weight of small element = ρrbtdθ. Figure 1 Rotating ring ROTATIONAL STRESSES INTRODUCTION High centrifugal forces are developed in machine components rotating at a high angular speed of the order of 100 to 500 revolutions per second (rps). High centrifugal force

More information

Sections minutes. 5 to 10 problems, similar to homework problems. No calculators, no notes, no books, no phones. No green book needed.

Sections minutes. 5 to 10 problems, similar to homework problems. No calculators, no notes, no books, no phones. No green book needed. MTH 34 Review for Exam 4 ections 16.1-16.8. 5 minutes. 5 to 1 problems, similar to homework problems. No calculators, no notes, no books, no phones. No green book needed. Review for Exam 4 (16.1) Line

More information

PhD Qualifying Exam Nuclear Engineering Program. Part 1 Core Courses

PhD Qualifying Exam Nuclear Engineering Program. Part 1 Core Courses PhD Qualifying Exam Nuclear Engineering Program Part 1 Core Courses 9:00 am 12:00 noon, November 19, 2016 (1) Nuclear Reactor Analysis During the startup of a one-region, homogeneous slab reactor of size

More information

Multiple Integrals and Vector Calculus: Synopsis

Multiple Integrals and Vector Calculus: Synopsis Multiple Integrals and Vector Calculus: Synopsis Hilary Term 28: 14 lectures. Steve Rawlings. 1. Vectors - recap of basic principles. Things which are (and are not) vectors. Differentiation and integration

More information

MATH 52 FINAL EXAM SOLUTIONS

MATH 52 FINAL EXAM SOLUTIONS MAH 5 FINAL EXAM OLUION. (a) ketch the region R of integration in the following double integral. x xe y5 dy dx R = {(x, y) x, x y }. (b) Express the region R as an x-simple region. R = {(x, y) y, x y }

More information

FLUX OF VECTOR FIELD INTRODUCTION

FLUX OF VECTOR FIELD INTRODUCTION Chapter 3 GAUSS LAW ntroduction Flux of vector field Solid angle Gauss s Law Symmetry Spherical symmetry Cylindrical symmetry Plane symmetry Superposition of symmetric geometries Motion of point charges

More information

第 1 頁, 共 8 頁 Chap32&Chap33 1. Test Bank, Question 2 Gauss' law for magnetism tells us: the net charge in any given volume that the line integral of a magnetic around any closed loop must vanish the magnetic

More information

Physics 351, Spring 2017, Homework #4. Due at start of class, Friday, February 10, 2017

Physics 351, Spring 2017, Homework #4. Due at start of class, Friday, February 10, 2017 Physics 351, Spring 2017, Homework #4. Due at start of class, Friday, February 10, 2017 Course info is at positron.hep.upenn.edu/p351 When you finish this homework, remember to visit the feedback page

More information

Math 3c Solutions: Exam 1 Fall Graph by eliiminating the parameter; be sure to write the equation you get when you eliminate the parameter.

Math 3c Solutions: Exam 1 Fall Graph by eliiminating the parameter; be sure to write the equation you get when you eliminate the parameter. Math c Solutions: Exam 1 Fall 16 1. Graph by eliiminating the parameter; be sure to write the equation you get when you eliminate the parameter. x tan t x tan t y sec t y sec t t π 4 To eliminate the parameter,

More information

Phys 4322 Final Exam - Solution May 12, 2015

Phys 4322 Final Exam - Solution May 12, 2015 Phys 4322 Final Exam - Solution May 12, 2015 You may NOT use any book or notes other than that supplied with this test. You will have 3 hours to finish. DO YOUR OWN WORK. Express your answers clearly and

More information

(You may need to make a sin / cos-type trigonometric substitution.) Solution.

(You may need to make a sin / cos-type trigonometric substitution.) Solution. MTHE 7 Problem Set Solutions. As a reminder, a torus with radii a and b is the surface of revolution of the circle (x b) + z = a in the xz-plane about the z-axis (a and b are positive real numbers, with

More information

Compton Storage Rings

Compton Storage Rings Compton Polarimetry @ Storage Rings Wolfgang Hillert ELectron Stretcher Accelerator Physics Institute of Bonn University Møller-Polarimeter Compton-Polarimeter Mott-Polarimeter Compton Scattering Differential

More information

PHY492: Nuclear & Particle Physics. Lecture 3 Homework 1 Nuclear Phenomenology

PHY492: Nuclear & Particle Physics. Lecture 3 Homework 1 Nuclear Phenomenology PHY49: Nuclear & Particle Physics Lecture 3 Homework 1 Nuclear Phenomenology Measuring cross sections in thin targets beam particles/s n beam m T = ρts mass of target n moles = m T A n nuclei = n moles

More information

X. Assembling the Pieces

X. Assembling the Pieces X. Assembling the Pieces 179 Introduction Our goal all along has been to gain an understanding of nuclear reactors. As we ve noted many times, this requires knowledge of how neutrons are produced and lost.

More information

θ N e θ 0 θ 0 = λ A 0 (θ,φ) 2 sinθdθdφ = 1 (3) A i(θ,φ)a j (θ,φ)sinθdθdφ (4)

θ N e θ 0 θ 0 = λ A 0 (θ,φ) 2 sinθdθdφ = 1 (3) A i(θ,φ)a j (θ,φ)sinθdθdφ (4) 1 Introduction 1.1 Angular Spectrum of Plane Waves A Gaussian beam with a beam waist of w 0 has a corresponding angular representation A 0 (θ,φ) = 1 ( ) 2 θ N e θ 0 (1) where and the normalization N is

More information

e x3 dx dy. 0 y x 2, 0 x 1.

e x3 dx dy. 0 y x 2, 0 x 1. Problem 1. Evaluate by changing the order of integration y e x3 dx dy. Solution:We change the order of integration over the region y x 1. We find and x e x3 dy dx = y x, x 1. x e x3 dx = 1 x=1 3 ex3 x=

More information

10. Scattering from Central Force Potential

10. Scattering from Central Force Potential University of Rhode Island DigitalCommons@URI Classical Dynamics Physics Course Materials 215 1. Scattering from Central Force Potential Gerhard Müller University of Rhode Island, gmuller@uri.edu Creative

More information

Solutions to Sample Questions for Final Exam

Solutions to Sample Questions for Final Exam olutions to ample Questions for Final Exam Find the points on the surface xy z 3 that are closest to the origin. We use the method of Lagrange Multipliers, with f(x, y, z) x + y + z for the square of the

More information

Multiple Integrals and Vector Calculus (Oxford Physics) Synopsis and Problem Sets; Hilary 2015

Multiple Integrals and Vector Calculus (Oxford Physics) Synopsis and Problem Sets; Hilary 2015 Multiple Integrals and Vector Calculus (Oxford Physics) Ramin Golestanian Synopsis and Problem Sets; Hilary 215 The outline of the material, which will be covered in 14 lectures, is as follows: 1. Introduction

More information

MATH 241 Practice Second Midterm Exam - Fall 2012

MATH 241 Practice Second Midterm Exam - Fall 2012 MATH 41 Practice Second Midterm Exam - Fall 1 1. Let f(x = { 1 x for x 1 for 1 x (a Compute the Fourier sine series of f(x. The Fourier sine series is b n sin where b n = f(x sin dx = 1 = (1 x cos = 4

More information

f(p i )Area(T i ) F ( r(u, w) ) (r u r w ) da

f(p i )Area(T i ) F ( r(u, w) ) (r u r w ) da MAH 55 Flux integrals Fall 16 1. Review 1.1. Surface integrals. Let be a surface in R. Let f : R be a function defined on. efine f ds = f(p i Area( i lim mesh(p as a limit of Riemann sums over sampled-partitions.

More information

Physics 221. Exam III Spring f S While the cylinder is rolling up, the frictional force is and the cylinder is rotating

Physics 221. Exam III Spring f S While the cylinder is rolling up, the frictional force is and the cylinder is rotating Physics 1. Exam III Spring 003 The situation below refers to the next three questions: A solid cylinder of radius R and mass M with initial velocity v 0 rolls without slipping up the inclined plane. N

More information

MCRT: L4 A Monte Carlo Scattering Code

MCRT: L4 A Monte Carlo Scattering Code MCRT: L4 A Monte Carlo Scattering Code Plane parallel scattering slab Optical depths & physical distances Emergent flux & intensity Internal intensity moments Constant density slab, vertical optical depth

More information

Problem Set #4: 4.1,4.7,4.9 (Due Monday, March 25th)

Problem Set #4: 4.1,4.7,4.9 (Due Monday, March 25th) Chapter 4 Multipoles, Dielectrics Problem Set #4: 4.,4.7,4.9 (Due Monday, March 5th 4. Multipole expansion Consider a localized distribution of charges described by ρ(x contained entirely in a sphere of

More information

Lecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2

Lecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 Lecture 6 Scattering theory Partial Wave Analysis SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 The Born approximation for the differential cross section is valid if the interaction

More information

Problem Set 5 Math 213, Fall 2016

Problem Set 5 Math 213, Fall 2016 Problem Set 5 Math 213, Fall 216 Directions: Name: Show all your work. You are welcome and encouraged to use Mathematica, or similar software, to check your answers and aid in your understanding of the

More information

Moments of Inertia (7 pages; 23/3/18)

Moments of Inertia (7 pages; 23/3/18) Moments of Inertia (7 pages; 3/3/8) () Suppose that an object rotates about a fixed axis AB with angular velocity θ. Considering the object to be made up of particles, suppose that particle i (with mass

More information

Heriot-Watt University

Heriot-Watt University Heriot-Watt University Distinctly Global www.hw.ac.uk Thermodynamics By Peter Cumber Prerequisites Interest in thermodynamics Some ability in calculus (multiple integrals) Good understanding of conduction

More information

Practice Final Solutions

Practice Final Solutions Practice Final Solutions Math 1, Fall 17 Problem 1. Find a parameterization for the given curve, including bounds on the parameter t. Part a) The ellipse in R whose major axis has endpoints, ) and 6, )

More information

SAMPLING SPECIAL DISTRIBUTIONS

SAMPLING SPECIAL DISTRIBUTIONS SAMPLING SPECIAL DISTRIBUTIONS M. Ragheb 4/9/4 INTRODUCTION Monte Carlo simulations require the sampling of various distributions at different steps in the simulation process. There exist a multitude of

More information

Topic 7. Electric flux Gauss s Law Divergence of E Application of Gauss Law Curl of E

Topic 7. Electric flux Gauss s Law Divergence of E Application of Gauss Law Curl of E Topic 7 Electric flux Gauss s Law Divergence of E Application of Gauss Law Curl of E urface enclosing an electric dipole. urface enclosing charges 2q and q. Electric flux Flux density : The number of field

More information

Elastic Scattering. R = m 1r 1 + m 2 r 2 m 1 + m 2. is the center of mass which is known to move with a constant velocity (see previous lectures):

Elastic Scattering. R = m 1r 1 + m 2 r 2 m 1 + m 2. is the center of mass which is known to move with a constant velocity (see previous lectures): Elastic Scattering In this section we will consider a problem of scattering of two particles obeying Newtonian mechanics. The problem of scattering can be viewed as a truncated version of dynamic problem

More information

Notes 19 Gradient and Laplacian

Notes 19 Gradient and Laplacian ECE 3318 Applied Electricity and Magnetism Spring 218 Prof. David R. Jackson Dept. of ECE Notes 19 Gradient and Laplacian 1 Gradient Φ ( x, y, z) =scalar function Φ Φ Φ grad Φ xˆ + yˆ + zˆ x y z We can

More information

Calculus III 2004 Summer Practice Final 8/3/2004

Calculus III 2004 Summer Practice Final 8/3/2004 .. Calculus III 4 ummer Practice Final 8/3/4. Compute the following limits if they exist: (a) lim (x,y) (,) e xy x+. cos x (b) lim x. (x,y) (,) x 4 +y 4 (a) ince lim (x,y) (,) exy and lim x + 6 in a (x,y)

More information

Created by T. Madas SURFACE INTEGRALS. Created by T. Madas

Created by T. Madas SURFACE INTEGRALS. Created by T. Madas SURFACE INTEGRALS Question 1 Find the area of the plane with equation x + 3y + 6z = 60, 0 x 4, 0 y 6. 8 Question A surface has Cartesian equation y z x + + = 1. 4 5 Determine the area of the surface which

More information

Applications of Gauss Law

Applications of Gauss Law Applications of Gauss Law The Gauss Law of electrostatics relates the net electric field flux through a complete surface S of some volume V to the net electric charge inside that volume, Φ E [S] def =

More information

1. (30 points) In the x-y plane, find and classify all local maxima, local minima, and saddle points of the function. f(x, y) = 3y 2 2y 3 3x 2 + 6xy.

1. (30 points) In the x-y plane, find and classify all local maxima, local minima, and saddle points of the function. f(x, y) = 3y 2 2y 3 3x 2 + 6xy. APPM 35 FINAL EXAM FALL 13 INSTUTIONS: Electronic devices, books, and crib sheets are not permitted. Write your name and your instructor s name on the front of your bluebook. Work all problems. Show your

More information

Volume in n Dimensions

Volume in n Dimensions Volume in n Dimensions MA 305 Kurt Bryan Introduction You ve seen that if we have two vectors v and w in two dimensions then the area spanned by these vectors can be computed as v w = v 1 w 2 v 2 w 1 (where

More information

Chapter 5 Trigonometric Functions of Angles

Chapter 5 Trigonometric Functions of Angles Chapter 5 Trigonometric Functions of Angles Section 3 Points on Circles Using Sine and Cosine Signs Signs I Signs (+, +) I Signs II (+, +) I Signs II (, +) (+, +) I Signs II (, +) (+, +) I III Signs II

More information

1. (3) Write Gauss Law in differential form. Explain the physical meaning.

1. (3) Write Gauss Law in differential form. Explain the physical meaning. Electrodynamics I Midterm Exam - Part A - Closed Book KSU 204/0/23 Name Instructions: Use SI units. Where appropriate, define all variables or symbols you use, in words. Try to tell about the physics involved,

More information

1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER

1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 5.1 Introduction As radiation struggles to make its way upwards through a stellar atmosphere, it may be weakened by absorption

More information

Week 7: Integration: Special Coordinates

Week 7: Integration: Special Coordinates Week 7: Integration: Special Coordinates Introduction Many problems naturally involve symmetry. One should exploit it where possible and this often means using coordinate systems other than Cartesian coordinates.

More information