GR Calculations in Specific Bases Using Mathematica

Size: px
Start display at page:

Download "GR Calculations in Specific Bases Using Mathematica"

Transcription

1 GR Calculations in Specific Bases Using Mathematica Geoge E. Habovsky MAST Midwest Relativity Meeting, 2015 CIERA, Nowesten Univesity

2 2 GR Calculations in Specific Bases Using Mathematica.nb What I Will Cove Intoduction How to Establish a Manifold How to Establish a Coodinate Chat How to Define a Metic How to Define a Tenso Computing the Chistoffel Symbols The Riemann Tenso, The Ricci Tenso, The Ricci Scala, and The Einstein Tenso The Stess-Enegy Tenso Einstein s Field Equations

3 GR Calculations in Specific Bases Using Mathematica.nb 3 Intoduction This is the thid of an appaently endless seies of talks on how to use Mathematica in geneal elativity. Two yeas ago I talked about the built-in capabilities fo handling tensos. Last yea I talked about the xact package in geneal and how to apply it to petubative geneal elativity, deiving the scala and tenso field equations fo a gavitational petubation given a Lagangian. This yea I am talking about pefoming calculations in specific coodinate bases. Past talks can be found at the website: http : // This talk will appea thee also.

4 4 GR Calculations in Specific Bases Using Mathematica.nb Establishing You Manifold The fist thing too do is activate xact. << xact`xtenso` Package xact`xpem` vesion 1.2.2, {2014, 9, 28} CopyRight (C) , Jose M. Matin-Gacia, unde the Geneal Public License. Connecting to extenal MinGW executable... Connection established Package xact`xtenso` vesion 1.1.1, {2014, 9, 28} CopyRight (C) , Jose M. Matin-Gacia, unde the Geneal Public License These packages come with ABSOLUTELY NO WARRANTY; fo details type Disclaime[]. This is fee softwae, and you ae welcome to edistibute it unde cetain conditions. See the Geneal Public License fo details Then you define you manifold.

5 GR Calculations in Specific Bases Using Mathematica.nb 5 DefManifold[M4, 4, {α, β, γ, μ, ν, λ, σ, η}] ** DefManifold: Defining manifold M4. ** DefVBundle: Defining vbundle TangentM4.

6 6 GR Calculations in Specific Bases Using Mathematica.nb DefMetic[-1, metic[-α, -β], CD, {";", " "}, PintAs "g"] ** DefTenso: Defining symmetic metic tenso metic[- α, - β]. ** DefTenso: Defining antisymmetic tenso epsilonmetic[- α, - β, - γ, - η]. ** DefTenso: Defining tetametic Tetametic[- α, - β, - γ, - η]. ** DefTenso: Defining tetametic Tetametic [- α, - β, - γ, - η]. ** DefCovD: Defining covaiant deivative CD[- α]. ** DefTenso: Defining vanishing tosion tenso TosionCD[α, - β, - γ]. ** DefTenso: Defining symmetic Chistoffel tenso ChistoffelCD[α, - β, - γ]. ** DefTenso: Defining Riemann tenso RiemannCD[- α, - β, - γ, - η]. ** DefTenso: Defining symmetic Ricci tenso RicciCD[- α, - β]. ** DefCovD: Contactions of Riemann automatically eplaced by Ricci. ** DefTenso: Defining Ricci scala RicciScalaCD[]. ** DefCovD: Contactions of Ricci automatically eplaced by RicciScala. ** DefTenso: Defining symmetic Einstein tenso EinsteinCD[- α, - β]. ** DefTenso: Defining Weyl tenso WeylCD[-α, -β, -γ, -η]. ** DefTenso: Defining symmetic TFRicci tenso TFRicciCD[- α, - β]. ** DefTenso: Defining Ketschmann scala KetschmannCD[]. ** DefCovD: Computing RiemannToWeylRules fo dim 4 ** DefCovD: Computing RicciToTFRicci fo dim 4 ** DefCovD: Computing RicciToEinsteinRules fo dim 4 ** DefTenso: Defining weight +2 density Detmetic[]. Deteminant.

7 GR Calculations in Specific Bases Using Mathematica.nb 7 Establishing You Chat << xact`xcoba` Package xact`xcoba` vesion 0.8.2, {2014, 9, 28} CopyRight (C) , David Yllanes and Jose M. Matin-Gacia, unde the Geneal Public License These packages come with ABSOLUTELY NO WARRANTY; fo details type Disclaime[]. This is fee softwae, and you ae welcome to edistibute it unde cetain conditions. See the Geneal Public License fo details

8 8 GR Calculations in Specific Bases Using Mathematica.nb $DefInfoQ = False; $PePint = SceenDollaIndices; $CVSimplify = Simplify;

9 GR Calculations in Specific Bases Using Mathematica.nb 9 DefChat[cb, M4, {0, 1, 2, 3}, {t[], [], θ[], ϕ[]}] cb /: CIndexFom[0, cb] := "t"; cb /: CIndexFom[1, cb] := ""; cb /: CIndexFom[2, cb] := "θ"; cb /: CIndexFom[3, cb] := "ϕ"; You should then define any scala functions and constants you will need fo you metic. DefConstantSymbol[M] DefConstantSymbol[G]

10 10 GR Calculations in Specific Bases Using Mathematica.nb Two Ways to Define You Metic MatixFom met = DiagonalMatix 1-2 M [], 1-2 M M Sin[θ] M [] -1, -[] 2, 2 [] Sin[θ[]] 2

11 GR Calculations in Specific Bases Using Mathematica.nb 11 MeticInBasis[metic, - cb, met] // TableFom Added independent ule g tt 1-2 M fo tenso metic Added independent ule Added independent ule Added independent ule g t 0 fo tenso metic g tθ 0 fo tenso metic g tϕ 0 fo tenso metic Added dependent ule g t g t fo tenso metic Added independent ule g M fo tenso metic Added independent ule Added independent ule g θ 0 fo tenso metic g ϕ 0 fo tenso metic Added dependent ule Added dependent ule g θt g tθ fo tenso metic g θ g θ fo tenso metic Added independent ule g θθ - 2 fo tenso metic Added independent ule g θϕ 0 fo tenso metic Added dependent ule Added dependent ule Added dependent ule g ϕt g tϕ fo tenso metic g ϕ g ϕ fo tenso metic g ϕθ g θϕ fo tenso metic Added independent ule g ϕϕ 2 Sin[θ] 2 fo tenso metic g tt 1-2 M g t 0 g tθ 0 g tϕ 0 g t 0 g M g θ 0 g ϕ 0 g θt 0 g θ 0 g θθ - 2 g θϕ 0 g ϕt 0 g ϕ 0 g ϕθ 0 g ϕϕ 2 Sin[θ] 2

12 12 GR Calculations in Specific Bases Using Mathematica.nb metic FoldedRule g t g t, g θt g tθ, g θ g θ, g ϕt g tϕ, g ϕ g ϕ, g ϕθ g θϕ, g tt 1-2 M, g t 0, g tθ 0, g tϕ 0, g M g θ 0, g ϕ 0, g θθ - 2, g θϕ 0, g ϕϕ 2 Sin[θ] 2, MeticCompute[metic, cb, "Weyl"[-1, -1, -1, -1]]

13 GR Calculations in Specific Bases Using Mathematica.nb 13 Now we can exploe the second method of defining the metic. g = CTenso[met, {-cb, -cb}]; SetCMetic[g, -cb]; Hee was can specify the g tt component, g[{0, -cb}, {0, -cb}] 1-2 M MeticCompute[g, cb, "Weyl"[-1, -1, -1, -1]];

14 14 GR Calculations in Specific Bases Using Mathematica.nb Hee we define the covaiant deivative, cd = CovDOfMetic[g] CCovD PDcb, M CTenso 0, - 2 M -, 0, 0, - M, 0, 0, 0, {0, 0, 0, 0}, {0, 0, 0, 0}, 2 2 M - 2 M (2 M - ) M, 0, 0, 0, 0,, 0, 0, 3 2 M - 2 (2 M - ) Sin[θ]2 {0, 0, -2 M +, 0}, 0, 0, 0,, {0, 0, 0, 0}, 0, 0, 1, 0, 0, 1 Sin[2 θ], 0, 0, 0, 0, 0,, {0, 0, 0, 0}, 0, 0, 0, 1 1, {0, 0, 0, Cot[θ]}, 0,, Cot[θ], 0, 2 2 {cb, -cb, -cb}, 0, CTenso 1-2 M, 0, 0, 0, 0, 1, 0, 0, 1-2 M 0, 0, - 2, 0, 0, 0, 0, 2 Sin[θ] 2, {-cb, -cb}, 0

15 GR Calculations in Specific Bases Using Mathematica.nb 15 Chistoffel Symbols in a Coodinate Basis In geneal we can wite the Chistoffel symbols Chistoffel[CD, PDcb][α, -β, -γ] Γ[, ] α βγ We can make a table of these in ou coodinate basis. Pat[TensoValues@ ChistoffelCDPDcb, 2] // TableFom Γ[, ] t tt 0 Γ[, ] t t - Γ[, ] t tθ 0 Γ[, ] t tϕ 0 Γ[, ] t 0 Γ[, ] t θ 0 Γ[, ] t ϕ 0 Γ[, ] t θθ 0 Γ[, ] t θϕ 0 Γ[, ] t ϕϕ 0 Γ[, ] tt Γ[, ] t 0 Γ[, ] tθ 0 Γ[, ] tϕ 0 Γ[, ] Γ[, ] θ 0 Γ[, ] ϕ 0 M 2 M - 2 M (2 M-) 3 M 2 M - 2 Γ[, ] θθ -2 M + Γ[, ] θϕ 0 Γ[, ] ϕϕ Γ[, ] θ tt 0 Γ[, ] θ t 0 Γ[, ] θ tθ 0 Γ[, ] θ tϕ 0 (2 M-) Sin[θ]2

16 16 GR Calculations in Specific Bases Using Mathematica.nb Γ[, ] θ 0 Γ[, ] θ θ 1 Γ[, ] θ ϕ 0 Γ[, ] θ θθ 0 Γ[, ] θ θϕ 0 Γ[, ] θ ϕϕ Γ[, ] ϕ tt 0 Γ[, ] ϕ t 0 Γ[, ] ϕ tθ 0 Γ[, ] ϕ tϕ 0 Γ[, ] ϕ 0 Γ[, ] ϕ θ 0 Sin[2 θ] Γ[, ] ϕ ϕ 1 2 Γ[, ] ϕ θθ 0 Γ[, ] ϕ θϕ Cot[θ] Γ[, ] ϕ ϕϕ 0

17 GR Calculations in Specific Bases Using Mathematica.nb 17 The Riemann Tenso iemann = Riemann[cd] CTenso {{0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}}, 2 M (-2 M + ) 2 M 0,, 0, 0,, 0, 0, 0, {0, 0, 0, 0}, {0, 0, 0, 0}, 4 (2 M - ) 2 M (2 M - ) 0, 0,, 0, {0, 0, 0, 0}, - M, 0, 0, 0, {0, 0, 0, 0}, 4 M (2 M - ) 0, 0, 0,, {0, 0, 0, 0}, {0, 0, 0, 0}, M Sin[θ]2, 0, 0, 0, M (-2 M + ) 2 M 0, -, 0, 0, -, 0, 0, 0, {0, 0, 0, 0}, {0, 0, 0, 0}, 4 (2 M - ) 2 {{0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}}, M {0, 0, 0, 0}, 0, 0, (2 M - ), 0, 0, - M, 0, 0, {0, 0, 0, 0}, 2-4 M + Cot[θ] {0, 0, 0, 0}, 0, 0, 0,, 0, 0, 0,, 4 2 (-2 M + ) 2 (4 M - ) Sin[θ]2 Cos[θ] Sin[θ] 0,,, 0, M (2 M - ) 0, 0, -, 0, {0, 0, 0, 0}, M, 0, 0, 0, {0, 0, 0, 0}, 4 M {0, 0, 0, 0}, 0, 0, - (2 M - ), 0, 0, M, 0, 0, {0, 0, 0, 0}, 2 {{0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}}, {0, 0, 0, 0}, 0, 0, 0, Cot[θ], 0, 0, 0, M, Cos[θ] (2 M - ) Sin[θ] (-2 M + 3 ) Sin[θ]2 0,,, 0, 2 M (2 M - ) 0, 0, 0, -, {0, 0, 0, 0}, {0, 0, 0, 0}, - M Sin[θ]2, 0, 0, 0, M + Cot[θ] {0, 0, 0, 0}, 0, 0, 0, -, 0, 0, 0, -, 4 2 (-2 M + ) 2 (4 M - ) Sin[θ]2 Cos[θ] Sin[θ] 0, -, -, 0, {0, 0, 0, 0}, 0, 0, 0, - Cot[θ], , 0, 0, M Cos[θ] (2 M - ) Sin[θ] (-2 M + 3 ) Sin[θ]2, 0, -, -, 0, 2 {{0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}, {0, 0, 0, 0}}, {-cb, -cb, -cb, cb}, 0 iemann[{0, -cb}, {1, -cb}, {0, -cb}, {1, cb}] 2 M (-2 M + ) 4 iemann[{3, -cb}, {2, -cb}, {3, -cb}, {2, cb}] (-2 M + 3 ) Sin[θ]2-2

18 18 GR Calculations in Specific Bases Using Mathematica.nb The Ricci Tenso and Ricci Scala Ricci[cd][-α, -β] M (-2 M+) Cot[θ] 0-8 M Cot[θ] (2 M+5 ) Sin[θ]2-2 2 αβ Ricci[cd][{0, -cb}, {0, -cb}] M (-2 M + ) 2 4 s = RicciScala[cd][[1]] - 2 M

19 GR Calculations in Specific Bases Using Mathematica.nb 19 The Einstein Tenso Einstein[cd][-α, -β] (2 M-) (4 M+5 ) M+3 Cot[θ] 0-4 M Cot[θ] 2 M αβ Einstein[cd][{0, -cb}, {0, -cb}] (2 M - ) (4 M + 5 ) - 4 4

20 20 GR Calculations in Specific Bases Using Mathematica.nb The Stess Enegy Tenso We next need to calculate the stess-enegy tenso. we begin by defining the density field. DefTenso[ρ, M4] DefTenso[ρ, M4, GenSet[]] Hee we define the 4-velocity. U = CTenso[{1, 0, 0, 0}, {-cb}] CTenso[{1, 0, 0, 0}, {-cb}, 0]

21 GR Calculations in Specific Bases Using Mathematica.nb 21 Hee is the stess-enegy tenso fo a pessue-less dust Td[α_, β_] := ρ[] U[-α] U[-β] Td[α, β] ρ[] βα Hee we have the T tt component. Td[{0, cb}, {0, cb}] ρ[]

22 22 GR Calculations in Specific Bases Using Mathematica.nb The pessue-less dust is vey simple. A little moe complicated is the pefect fluid. This equies us to define a pessue field. DefTenso[p, M4] DefTenso[p, M4, GenSet[]] The stess-enegy tenso fo this situation is, Tf[α_, β_] := (ρ[] + p[]) U[-α] U[-β] + p[] g[-α, -β] Tf[α, β] p[]+p[] 1-2 M p[] M p[] Sin[θ] 2 αβ 0 0 -p[] 2 0 Tf[{-0, cb}, {-0, cb}] p[] + p[] 1-2 M + ρ[] Tf[{-1, cb}, {-1, cb}] p[] 1-2 M

23 GR Calculations in Specific Bases Using Mathematica.nb 23 Einstein s Field Equations We will now ty to wite Einstein s equation fo the tt components of the Einstein and stess-enegy tensos. We begin with this fomulation, R tt R g tt = 8 π G T tt

24 24 GR Calculations in Specific Bases Using Mathematica.nb tteq = Ricci[cd][{0, -cb}, {0, -cb}] - 1 s g[{0, -cb}, {0, -cb}] 2 8 π G Tf[{-0, cb}, {-0, cb}] M (-2 M + ) M (2 M + 5 ) 8 G π p[] + p[] 1-2 M ρ[] tteq // FullSimplify - (2 M - ) (4 M + 5 ) 8 G π p[] 2-2 M ρ[] We can also wite the equation, G tt = 8 π G T tt tteq2 = Einstein[cd][{0, -cb}, {0, -cb}] 8 π G Tf[{-0, cb}, {-0, cb}] // FullSimplify - (2 M - ) (4 M + 5 ) 8 G π p[] 2-2 M ρ[]

25 GR Calculations in Specific Bases Using Mathematica.nb 25 We can genalize this eineq[a_, b_] := Einstein[cd][{a, -cb}, {b, -cb}] - 8 π G Tf[{-a, cb}, {-b, cb}] // FullSimplify eineq[0, 0] - (2 M - ) (4 M + 5 ) - 8 G π p[] 2-2 M ρ[] eineq[1, 1] M G π p[] (-2 M + ) eineq[0, 1] 0

26 26 GR Calculations in Specific Bases Using Mathematica.nb Table[eineq[a, b], {a, 0, 3}, {b, 0, 3}] // TableFom (2 M-) (4 M+5 ) G π p[] 2-2 M + ρ[] M+3-16 G π p[] (-2 M+) Cot[θ] M + 8 G π p[] G π p[] Sin[θ] 2 Cot[θ] 2 0

27 Thank You! GR Calculations in Specific Bases Using Mathematica.nb 27

Homework # 3 Solution Key

Homework # 3 Solution Key PHYSICS 631: Geneal Relativity Homewok # 3 Solution Key 1. You e on you hono not to do this one by hand. I ealize you can use a compute o simply look it up. Please don t. In a flat space, the metic in

More information

Conformal transformations + Schwarzschild

Conformal transformations + Schwarzschild Intoduction to Geneal Relativity Solutions of homewok assignments 5 Confomal tansfomations + Schwazschild 1. To pove the identity, let s conside the fom of the Chistoffel symbols in tems of the metic tenso

More information

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c

d 2 x 0a d d =0. Relative to an arbitrary (accelerating frame) specified by x a = x a (x 0b ), the latter becomes: d 2 x a d 2 + a dx b dx c Chapte 6 Geneal Relativity 6.1 Towads the Einstein equations Thee ae seveal ways of motivating the Einstein equations. The most natual is pehaps though consideations involving the Equivalence Pinciple.

More information

The Precession of Mercury s Perihelion

The Precession of Mercury s Perihelion The Pecession of Mecuy s Peihelion Owen Biesel Januay 25, 2008 Contents 1 Intoduction 2 2 The Classical olution 2 3 Classical Calculation of the Peiod 4 4 The Relativistic olution 5 5 Remaks 9 1 1 Intoduction

More information

Fluid flow in curved geometries: Mathematical Modeling and Applications

Fluid flow in curved geometries: Mathematical Modeling and Applications Fluid flow in cuved geometies: Mathematical Modeling and Applications D. Muhammad Sajid Theoetical Plasma Physics Division PINSTECH, P.O. Niloe, PAEC, Islamabad Mach 01-06, 010 Islamabad, Paistan Pesentation

More information

Geometry of the homogeneous and isotropic spaces

Geometry of the homogeneous and isotropic spaces Geomety of the homogeneous and isotopic spaces H. Sonoda Septembe 2000; last evised Octobe 2009 Abstact We summaize the aspects of the geomety of the homogeneous and isotopic spaces which ae most elevant

More information

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!! Physics 161 Fall 011 Exta Cedit Investigating Black Holes - olutions The Following is Woth 50 Points!!! This exta cedit assignment will investigate vaious popeties of black holes that we didn t have time

More information

A New Approach to General Relativity

A New Approach to General Relativity Apeion, Vol. 14, No. 3, July 7 7 A New Appoach to Geneal Relativity Ali Rıza Şahin Gaziosmanpaşa, Istanbul Tukey E-mail: aizasahin@gmail.com Hee we pesent a new point of view fo geneal elativity and/o

More information

The Strain Compatibility Equations in Polar Coordinates RAWB, Last Update 27/12/07

The Strain Compatibility Equations in Polar Coordinates RAWB, Last Update 27/12/07 The Stain Compatibility Equations in Pola Coodinates RAWB Last Update 7//7 In D thee is just one compatibility equation. In D polas it is (Equ.) whee denotes the enineein shea (twice the tensoial shea)

More information

Introduction to General Relativity 2

Introduction to General Relativity 2 Intoduction to Geneal Relativity 2 Geneal Relativity Diffeential geomety Paallel tanspot How to compute metic? Deviation of geodesics Einstein equations Consequences Tests of Geneal Relativity Sola system

More information

3.3.1 Expanded forms of the Continuity Equation. θ (ρv θ)+ z (ρv z)=0. θ (ρv θ sin θ)+ 1

3.3.1 Expanded forms of the Continuity Equation. θ (ρv θ)+ z (ρv z)=0. θ (ρv θ sin θ)+ 1 Ke Equations 58 3.3 Ke Equations 3.3.1 Epanded foms of the Continuit Equation Rectangula coodinates: t (v (v z (v z0 Clindical coodinates: t 1 Spheical coodinates: (v 1 t 1 2 (2 v 1 θ (v θ z (v z0 θ (v

More information

arxiv:gr-qc/ v1 29 Jan 1998

arxiv:gr-qc/ v1 29 Jan 1998 Gavitational Analog of the Electomagnetic Poynting Vecto L.M. de Menezes 1 axiv:g-qc/9801095v1 29 Jan 1998 Dept. of Physics and Astonomy, Univesity of Victoia, Victoia, B.C. Canada V8W 3P6 Abstact The

More information

COORDINATE TRANSFORMATIONS - THE JACOBIAN DETERMINANT

COORDINATE TRANSFORMATIONS - THE JACOBIAN DETERMINANT COORDINATE TRANSFORMATIONS - THE JACOBIAN DETERMINANT Link to: phsicspages home page. To leave a comment o epot an eo, please use the auilia blog. Refeence: d Inveno, Ra, Intoducing Einstein s Relativit

More information

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3. Appendix A Vecto Algeba As is natual, ou Aeospace Stuctues will be descibed in a Euclidean thee-dimensional space R 3. A.1 Vectos A vecto is used to epesent quantities that have both magnitude and diection.

More information

Tolman-Oppenheimer-Volkoff equations

Tolman-Oppenheimer-Volkoff equations Tolman-Oppenheime-Volkoff equations This Jupyte/SageMath woksheet is elative to the lectues Geneal elativity computations with SageManifolds given at the NewCompSta School 216 (Coimba, Potugal). These

More information

Stress, Cauchy s equation and the Navier-Stokes equations

Stress, Cauchy s equation and the Navier-Stokes equations Chapte 3 Stess, Cauchy s equation and the Navie-Stokes equations 3. The concept of taction/stess Conside the volume of fluid shown in the left half of Fig. 3.. The volume of fluid is subjected to distibuted

More information

General Relativity Homework 5

General Relativity Homework 5 Geneal Relativity Homewok 5. In the pesence of a cosmological constant, Einstein s Equation is (a) Calculate the gavitational potential point souce with = M 3 (). R µ Rg µ + g µ =GT µ. in the Newtonian

More information

Vector d is a linear vector function of vector d when the following relationships hold:

Vector d is a linear vector function of vector d when the following relationships hold: Appendix 4 Dyadic Analysis DEFINITION ecto d is a linea vecto function of vecto d when the following elationships hold: d x = a xxd x + a xy d y + a xz d z d y = a yxd x + a yy d y + a yz d z d z = a zxd

More information

The Schwarzschild Solution

The Schwarzschild Solution The Schwazschild Solution Johannes Schmude 1 Depatment of Physics Swansea Univesity, Swansea, SA2 8PP, United Kingdom Decembe 6, 2007 1 pyjs@swansea.ac.uk Intoduction We use the following conventions:

More information

Do not turn over until you are told to do so by the Invigilator.

Do not turn over until you are told to do so by the Invigilator. UNIVERSITY OF EAST ANGLIA School of Mathematics Main Seies UG Examination 2015 16 FLUID DYNAMICS WITH ADVANCED TOPICS MTH-MD59 Time allowed: 3 Hous Attempt QUESTIONS 1 and 2, and THREE othe questions.

More information

8 Separation of Variables in Other Coordinate Systems

8 Separation of Variables in Other Coordinate Systems 8 Sepaation of Vaiables in Othe Coodinate Systems Fo the method of sepaation of vaiables to succeed you need to be able to expess the poblem at hand in a coodinate system in which the physical boundaies

More information

Perturbation theory and stability analysis for string-corrected black holes in arbitrary dimensions

Perturbation theory and stability analysis for string-corrected black holes in arbitrary dimensions CPHT-RR-046-0805 SPHT-T05/50 axiv:hep-th/0608009 v Aug 006 Petubation theoy and stability analysis fo sting-coected black holes in abitay dimensions Filipe Moua Cente de Physique Théoique, École Polytéchnique

More information

This gives rise to the separable equation dr/r = 2 cot θ dθ which may be integrated to yield r(θ) = R sin 2 θ (3)

This gives rise to the separable equation dr/r = 2 cot θ dθ which may be integrated to yield r(θ) = R sin 2 θ (3) Physics 506 Winte 2008 Homewok Assignment #10 Solutions Textbook poblems: Ch. 12: 12.10, 12.13, 12.16, 12.19 12.10 A chaged paticle finds itself instantaneously in the equatoial plane of the eath s magnetic

More information

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr.

PROBLEM SET #1 SOLUTIONS by Robert A. DiStasio Jr. POBLM S # SOLUIONS by obet A. DiStasio J. Q. he Bon-Oppenheime appoximation is the standad way of appoximating the gound state of a molecula system. Wite down the conditions that detemine the tonic and

More information

Solution of a Spherically Symmetric Static Problem of General Relativity for an Elastic Solid Sphere

Solution of a Spherically Symmetric Static Problem of General Relativity for an Elastic Solid Sphere Applied Physics eseach; Vol. 9, No. 6; 7 ISSN 96-969 E-ISSN 96-9647 Published by Canadian Cente of Science and Education Solution of a Spheically Symmetic Static Poblem of Geneal elativity fo an Elastic

More information

KEPLER S LAWS OF PLANETARY MOTION

KEPLER S LAWS OF PLANETARY MOTION EPER S AWS OF PANETARY MOTION 1. Intoduction We ae now in a position to apply what we have leaned about the coss poduct and vecto valued functions to deive eple s aws of planetay motion. These laws wee

More information

Figure 1. We will begin by deriving a very general expression before returning to Equations 1 and 2 to determine the specifics.

Figure 1. We will begin by deriving a very general expression before returning to Equations 1 and 2 to determine the specifics. Deivation of the Laplacian in Spheical Coodinates fom Fist Pinciples. Fist, let me state that the inspiation to do this came fom David Giffiths Intodction to Electodynamics textbook Chapte 1, Section 4.

More information

Conditions for the naked singularity formation in generalized Vaidya spacetime

Conditions for the naked singularity formation in generalized Vaidya spacetime Jounal of Physics: Confeence Seies PAPER OPEN ACCESS Conditions fo the naked singulaity fomation in genealized Vaidya spacetime To cite this aticle: V D Vetogadov 2016 J. Phys.: Conf. Se. 769 012013 View

More information

3D-Central Force Problems I

3D-Central Force Problems I 5.73 Lectue #1 1-1 Roadmap 1. define adial momentum 3D-Cental Foce Poblems I Read: C-TDL, pages 643-660 fo next lectue. All -Body, 3-D poblems can be educed to * a -D angula pat that is exactly and univesally

More information

Problems with Mannheim s conformal gravity program

Problems with Mannheim s conformal gravity program Poblems with Mannheim s confomal gavity pogam Abstact We show that Mannheim s confomal gavity pogam, whose potential has a tem popotional to 1/ and anothe tem popotional to, does not educe to Newtonian

More information

Continuum mechanics II. Kinematics in curvilinear coordinates. 1. Strain in cartesian coordinates (recapitulation)

Continuum mechanics II. Kinematics in curvilinear coordinates. 1. Strain in cartesian coordinates (recapitulation) Continuum mechanics office Math.7 ales.janka@unif.ch http://peso.unif.ch/ales.janka/mechanics Decembe 22, 2, Univesité de Fiboug. Stain in catesian coodinates (ecapitulation) Geen stain tenso: Lagange

More information

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk

Appendix A. Appendices. A.1 ɛ ijk and cross products. Vector Operations: δ ij and ɛ ijk Appendix A Appendices A1 ɛ and coss poducts A11 Vecto Opeations: δ ij and ɛ These ae some notes on the use of the antisymmetic symbol ɛ fo expessing coss poducts This is an extemely poweful tool fo manipulating

More information

Is there a magnification paradox in gravitational lensing?

Is there a magnification paradox in gravitational lensing? Is thee a magnification paadox in gavitational ing? Olaf Wucknitz wucknitz@asto.uni-bonn.de Astophysics semina/colloquium, Potsdam, 6 Novembe 7 Is thee a magnification paadox in gavitational ing? gavitational

More information

arxiv: v2 [gr-qc] 18 Aug 2014

arxiv: v2 [gr-qc] 18 Aug 2014 Self-Consistent, Self-Coupled Scala Gavity J. Fanklin Depatment of Physics, Reed College, Potland, Oegon 970, USA Abstact A scala theoy of gavity extending Newtonian gavity to include field enegy as its

More information

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925)

2 Lecture 2: The Bohr atom (1913) and the Schrödinger equation (1925) 1 Lectue 1: The beginnings of quantum physics 1. The Sten-Gelach expeiment. Atomic clocks 3. Planck 1900, blackbody adiation, and E ω 4. Photoelectic effect 5. Electon diffaction though cystals, de Boglie

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 151 Lectue 5 Cental Foce Poblem (Chapte 3) What We Did Last Time Intoduced Hamilton s Pinciple Action integal is stationay fo the actual path Deived Lagange s Equations Used calculus

More information

-Δ u = λ u. u(x,y) = u 1. (x) u 2. (y) u(r,θ) = R(r) Θ(θ) Δu = 2 u + 2 u. r = x 2 + y 2. tan(θ) = y/x. r cos(θ) = cos(θ) r.

-Δ u = λ u. u(x,y) = u 1. (x) u 2. (y) u(r,θ) = R(r) Θ(θ) Δu = 2 u + 2 u. r = x 2 + y 2. tan(θ) = y/x. r cos(θ) = cos(θ) r. The Laplace opeato in pola coodinates We now conside the Laplace opeato with Diichlet bounday conditions on a cicula egion Ω {(x,y) x + y A }. Ou goal is to compute eigenvalues and eigenfunctions of the

More information

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx.

( ) [ ] [ ] [ ] δf φ = F φ+δφ F. xdx. 9. LAGRANGIAN OF THE ELECTROMAGNETIC FIELD In the pevious section the Lagangian and Hamiltonian of an ensemble of point paticles was developed. This appoach is based on a qt. This discete fomulation can

More information

Now we just need to shuffle indices around a bit. The second term is already of the form

Now we just need to shuffle indices around a bit. The second term is already of the form Depatment of Physics, UCSD Physics 5B, Geneal Relativity Winte 05 Homewok, solutions. (a) Fom the Killing equation, ρ K σ ` σ K ρ 0 taking one deivative, µ ρ K σ ` µ σ K ρ 0 σ µ K ρ σ ρ K µ 0 ρ µ K σ `

More information

Supplementary material for the paper Platonic Scattering Cancellation for Bending Waves on a Thin Plate. Abstract

Supplementary material for the paper Platonic Scattering Cancellation for Bending Waves on a Thin Plate. Abstract Supplementay mateial fo the pape Platonic Scatteing Cancellation fo Bending Waves on a Thin Plate M. Fahat, 1 P.-Y. Chen, 2 H. Bağcı, 1 S. Enoch, 3 S. Guenneau, 3 and A. Alù 2 1 Division of Compute, Electical,

More information

The Concept of the Effective Mass Tensor in GR. Clocks and Rods

The Concept of the Effective Mass Tensor in GR. Clocks and Rods The Concept of the Effective Mass Tenso in GR Clocks and Rods Miosław J. Kubiak Zespół Szkół Technicznych, Gudziądz, Poland Abstact: In the pape [] we pesented the concept of the effective ass tenso (EMT)

More information

1 Spherical multipole moments

1 Spherical multipole moments Jackson notes 9 Spheical multipole moments Suppose we have a chage distibution ρ (x) wheeallofthechageiscontained within a spheical egion of adius R, as shown in the diagam. Then thee is no chage in the

More information

Topic 7: Electrodynamics of spinning particles Revised Draft

Topic 7: Electrodynamics of spinning particles Revised Draft Lectue Seies: The Spin of the Matte, Physics 4250, Fall 2010 1 Topic 7: Electodynamics of spinning paticles Revised Daft D. Bill Pezzaglia CSUEB Physics Updated Nov 28, 2010 Index: Rough Daft 2 A. Classical

More information

The Schwartzchild Geometry

The Schwartzchild Geometry UNIVERSITY OF ROCHESTER The Schwatzchild Geomety Byon Osteweil Decembe 21, 2018 1 INTRODUCTION In ou study of geneal elativity, we ae inteested in the geomety of cuved spacetime in cetain special cases

More information

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e.,

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e., Stella elaxation Time [Chandasekha 1960, Pinciples of Stella Dynamics, Chap II] [Ostike & Davidson 1968, Ap.J., 151, 679] Do stas eve collide? Ae inteactions between stas (as opposed to the geneal system

More information

Geodesic motion in Kerr spacetime

Geodesic motion in Kerr spacetime Chapte 20 Geodesic motion in Ke spacetime Let us conside a geodesic with affine paamete λ and tangent vecto u µ = dxµ dλ ẋµ. (20.1) In this section we shall use Boye-Lindquist s coodinates, and the dot

More information

Vectors, Vector Calculus, and Coordinate Systems

Vectors, Vector Calculus, and Coordinate Systems Apil 5, 997 A Quick Intoduction to Vectos, Vecto Calculus, and Coodinate Systems David A. Randall Depatment of Atmospheic Science Coloado State Univesity Fot Collins, Coloado 80523. Scalas and vectos Any

More information

Transformation of the Navier-Stokes Equations in Curvilinear Coordinate Systems with Maple

Transformation of the Navier-Stokes Equations in Curvilinear Coordinate Systems with Maple Global Jounal of Pue and Applied Mathematics. ISSN 0973-1768 Volume 12, Numbe 4 2016, pp. 3315 3325 Reseach India Publications http://www.ipublication.com/gjpam.htm Tansfomation of the Navie-Stokes Equations

More information

Spherical Solutions due to the Exterior Geometry of a Charged Weyl Black Hole

Spherical Solutions due to the Exterior Geometry of a Charged Weyl Black Hole Spheical Solutions due to the Exteio Geomety of a Chaged Weyl Black Hole Fain Payandeh 1, Mohsen Fathi Novembe 7, 018 axiv:10.415v [g-qc] 10 Oct 01 1 Depatment of Physics, Payame Noo Univesity, PO BOX

More information

From Here to Eternity and Back: Are Traversable Wormholes Possible?

From Here to Eternity and Back: Are Traversable Wormholes Possible? Fom Hee to Etenity and Back: Ae Tavesable Womholes Possible? May Magaet McEachen with advising fom D. Russell L. Heman Phys. 495 Sping 009 Apil 4, 009 Dedicated in Memoy of My Dea Fiend and UNCW Alumnus

More information

Mean Curvature and Shape Operator of Slant Immersions in a Sasakian Space Form

Mean Curvature and Shape Operator of Slant Immersions in a Sasakian Space Form Mean Cuvatue and Shape Opeato of Slant Immesions in a Sasakian Space Fom Muck Main Tipathi, Jean-Sic Kim and Son-Be Kim Abstact Fo submanifolds, in a Sasakian space fom, which ae tangential to the stuctue

More information

PHYS 705: Classical Mechanics. Small Oscillations

PHYS 705: Classical Mechanics. Small Oscillations PHYS 705: Classical Mechanics Small Oscillations Fomulation of the Poblem Assumptions: V q - A consevative system with depending on position only - The tansfomation equation defining does not dep on time

More information

Pressure Calculation of a Constant Density Star in the Dynamic Theory of Gravity

Pressure Calculation of a Constant Density Star in the Dynamic Theory of Gravity Pessue Calculation of a Constant Density Sta in the Dynamic Theoy of Gavity Ioannis Iaklis Haanas Depatment of Physics and Astonomy Yok Univesity A Petie Science Building Yok Univesity Toonto Ontaio CANADA

More information

MMAT5520. Lau Chi Hin The Chinese University of Hong Kong

MMAT5520. Lau Chi Hin The Chinese University of Hong Kong MMAT550 Lau Chi Hin The Chinese Univesit of Hong Kong Isaac Newton (1643-177) Keple s Laws of planeta motion 1. The obit is an ellipse with the sun at one of the foci.. A line joining a planet and the

More information

Classical Mechanics Homework set 7, due Nov 8th: Solutions

Classical Mechanics Homework set 7, due Nov 8th: Solutions Classical Mechanics Homewok set 7, due Nov 8th: Solutions 1. Do deivation 8.. It has been asked what effect does a total deivative as a function of q i, t have on the Hamiltonian. Thus, lets us begin with

More information

Problem Set 10 Solutions

Problem Set 10 Solutions Chemisty 6 D. Jean M. Standad Poblem Set 0 Solutions. Give the explicit fom of the Hamiltonian opeato (in atomic units) fo the lithium atom. You expession should not include any summations (expand them

More information

On the integration of the equations of hydrodynamics

On the integration of the equations of hydrodynamics Uebe die Integation de hydodynamischen Gleichungen J f eine u angew Math 56 (859) -0 On the integation of the equations of hydodynamics (By A Clebsch at Calsuhe) Tanslated by D H Delphenich In a pevious

More information

Physics 235 Chapter 5. Chapter 5 Gravitation

Physics 235 Chapter 5. Chapter 5 Gravitation Chapte 5 Gavitation In this Chapte we will eview the popeties of the gavitational foce. The gavitational foce has been discussed in geat detail in you intoductoy physics couses, and we will pimaily focus

More information

Problems with Mannheim s conformal gravity program

Problems with Mannheim s conformal gravity program Poblems with Mannheim s confomal gavity pogam June 4, 18 Youngsub Yoon axiv:135.163v6 [g-qc] 7 Jul 13 Depatment of Physics and Astonomy Seoul National Univesity, Seoul 151-747, Koea Abstact We show that

More information

AP-C WEP. h. Students should be able to recognize and solve problems that call for application both of conservation of energy and Newton s Laws.

AP-C WEP. h. Students should be able to recognize and solve problems that call for application both of conservation of energy and Newton s Laws. AP-C WEP 1. Wok a. Calculate the wok done by a specified constant foce on an object that undegoes a specified displacement. b. Relate the wok done by a foce to the aea unde a gaph of foce as a function

More information

B da = 0. Q E da = ε. E da = E dv

B da = 0. Q E da = ε. E da = E dv lectomagnetic Theo Pof Ruiz, UNC Asheville, doctophs on YouTube Chapte Notes The Maxwell quations in Diffeential Fom 1 The Maxwell quations in Diffeential Fom We will now tansfom the integal fom of the

More information

DonnishJournals

DonnishJournals DonnishJounals 041-1189 Donnish Jounal of Educational Reseach and Reviews. Vol 1(1) pp. 01-017 Novembe, 014. http:///dje Copyight 014 Donnish Jounals Oiginal Reseach Pape Vecto Analysis Using MAXIMA Savaş

More information

Lau Chi Hin The Chinese University of Hong Kong

Lau Chi Hin The Chinese University of Hong Kong Lau Chi Hin The Chinese Univesit of Hong Kong Can Antson each the othe end? 1cms 1 Can I each the othe end? Rubbe band 1m 1ms 1 Can Antson each the othe end? Gottfied Wilhelm Leibniz (1646-1716) Isaac

More information

Dilatonic black holes in heterotic string theory: perturbations and stability

Dilatonic black holes in heterotic string theory: perturbations and stability Dilatonic black holesin heteotic sting theoy:petubations and stability p. 1/2 Dilatonic black holes in heteotic sting theoy: petubations and stability Filipe Moua Cento de Matemática, Univesidade do Minho,

More information

Adiabatic evolution of the constants of motion in resonance (I)

Adiabatic evolution of the constants of motion in resonance (I) Adiabatic evolution of the constants of motion in esonance (I) BH Gavitational 重 力力波 waves Takahio Tanaka (YITP, Kyoto univesity) R. Fujita, S. Isoyama, H. Nakano, N. Sago PTEP 013 (013) 6, 063E01 e-pint:

More information

MATH 220: SECOND ORDER CONSTANT COEFFICIENT PDE. We consider second order constant coefficient scalar linear PDEs on R n. These have the form

MATH 220: SECOND ORDER CONSTANT COEFFICIENT PDE. We consider second order constant coefficient scalar linear PDEs on R n. These have the form MATH 220: SECOND ORDER CONSTANT COEFFICIENT PDE ANDRAS VASY We conside second ode constant coefficient scala linea PDEs on R n. These have the fom Lu = f L = a ij xi xj + b i xi + c i whee a ij b i and

More information

15 Solving the Laplace equation by Fourier method

15 Solving the Laplace equation by Fourier method 5 Solving the Laplace equation by Fouie method I aleady intoduced two o thee dimensional heat equation, when I deived it, ecall that it taes the fom u t = α 2 u + F, (5.) whee u: [0, ) D R, D R is the

More information

Gravitational Memory?

Gravitational Memory? Gavitational Memoy? a Petubative Appoach T. Haada 1, Depatment of Physics, Waseda Univesity, Shinjuku, Tokyo 169-8555, Japan B.J. Ca 2,andC.A.Goyme 3 Astonomy Unit, Queen May and Westfield College, Univesity

More information

arxiv: v5 [gr-qc] 12 Feb 2018

arxiv: v5 [gr-qc] 12 Feb 2018 The global monopole spacetime and its topological chage Hongwei Tan, Jinbo Yang,, Jingyi Zhang, and Tangmei He Cente fo Astophysics, Guangzhou Univesity, Guangzhou 50006 co-fist autho axiv:705.0087v5 [g-qc]

More information

Section 8.2 Polar Coordinates

Section 8.2 Polar Coordinates Section 8. Pola Coodinates 467 Section 8. Pola Coodinates The coodinate system we ae most familia with is called the Catesian coodinate system, a ectangula plane divided into fou quadants by the hoizontal

More information

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1 Please ead this fist... AST S: The oigin and evolution of the Univese Intoduction to Mathematical Handout This is an unusually long hand-out and one which uses in places mathematics that you may not be

More information

Notation. 1 Vectors. 2 Spherical Coordinates The Problem

Notation. 1 Vectors. 2 Spherical Coordinates The Problem Notation 1 Vectos As aleady noted, we neve wite vectos as pais o tiples of numbes; this notation is eseved fo coodinates, a quite diffeent concept. The symbols we use fo vectos have aows on them (to match

More information

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum 2. Electostatics D. Rakhesh Singh Kshetimayum 1 2.1 Intoduction In this chapte, we will study how to find the electostatic fields fo vaious cases? fo symmetic known chage distibution fo un-symmetic known

More information

Physics 505 Homework No. 9 Solutions S9-1

Physics 505 Homework No. 9 Solutions S9-1 Physics 505 Homewok No 9 s S9-1 1 As pomised, hee is the tick fo summing the matix elements fo the Stak effect fo the gound state of the hydogen atom Recall, we need to calculate the coection to the gound

More information

On Pseudo-Union Curves in a Hypersurface of a Weyl Space

On Pseudo-Union Curves in a Hypersurface of a Weyl Space Intenational Mathematical Foum, Vol., 07, no. 6, 78-793 HIKARI Ltd, www.m-hikai.com https://doi.og/0.988/imf.07.7760 On Pseudo-Union Cues in a Hypesuface of a Weyl Space Nil Kofoğlu Beykent Uniesity Faculty

More information

TRAVERSABLE SCHWARZSCHILD WORMHOLE SOLUTION

TRAVERSABLE SCHWARZSCHILD WORMHOLE SOLUTION JURNAL FIZIK MALAYSIA Volume 34, numbe 3 3 TRAVERSABLE SCHWARZSCHILD WORMHOLE SOLUTION Nu Izzati Ishak and Wan Ahmad Tajuddin Bin Wan Abdullah Theoetical Physics Laboatoy Depatment of Physics, Faculty

More information

J. N. R E DDY ENERGY PRINCIPLES AND VARIATIONAL METHODS APPLIED MECHANICS

J. N. R E DDY ENERGY PRINCIPLES AND VARIATIONAL METHODS APPLIED MECHANICS J. N. E DDY ENEGY PINCIPLES AND VAIATIONAL METHODS IN APPLIED MECHANICS T H I D E DI T IO N JN eddy - 1 MEEN 618: ENEGY AND VAIATIONAL METHODS A EVIEW OF VECTOS AND TENSOS ead: Chapte 2 CONTENTS Physical

More information

ON RICCI TYPE IDENTITIES IN MANIFOLDS WITH NON-SYMMETRIC AFFINE CONNECTION. Svetislav M. Minčić

ON RICCI TYPE IDENTITIES IN MANIFOLDS WITH NON-SYMMETRIC AFFINE CONNECTION. Svetislav M. Minčić PUBLICATIONS DE L INSTITUT MATHÉMATIQUE Nouvelle séie, tome 9 (08) (0), 0 7 DOI: 0.98/PIM080M ON RICCI TPE IDENTITIES IN MANIFOLDS WITH NON-SMMETRIC AFFINE CONNECTION Svetislav M. Minčić Abstact. In [8],

More information

Lecture 1a: Satellite Orbits

Lecture 1a: Satellite Orbits Lectue 1a: Satellite Obits Outline 1. Newton s Laws of Motion 2. Newton s Law of Univesal Gavitation 3. Calculating satellite obital paametes (assuming cicula motion) Scala & Vectos Scala: a physical quantity

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 9

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 9 MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Depatment Physics 8.033 Novembe 17, 2006 Poblem Set 9 Due: Decembe 8, at 4:00PM. Please deposit the poblem set in the appopiate 8.033 bin, labeled with name

More information

THE LAPLACE EQUATION. The Laplace (or potential) equation is the equation. u = 0. = 2 x 2. x y 2 in R 2

THE LAPLACE EQUATION. The Laplace (or potential) equation is the equation. u = 0. = 2 x 2. x y 2 in R 2 THE LAPLACE EQUATION The Laplace (o potential) equation is the equation whee is the Laplace opeato = 2 x 2 u = 0. in R = 2 x 2 + 2 y 2 in R 2 = 2 x 2 + 2 y 2 + 2 z 2 in R 3 The solutions u of the Laplace

More information

Hawking radiation from Kerr Newman Kasuya black hole via quantum anomalies

Hawking radiation from Kerr Newman Kasuya black hole via quantum anomalies Vol 17 No 6, June 008 c 008 Chin. Phys. Soc. 1674-1056/008/1706/31-05 Chinese Physics B and IOP Publishing Ltd Hawking adiation fom Ke Newman Kasuya black hole via quantum anomalies He Tang-Mei a, Fan

More information

MATH 417 Homework 3 Instructor: D. Cabrera Due June 30. sin θ v x = v r cos θ v θ r. (b) Then use the Cauchy-Riemann equations in polar coordinates

MATH 417 Homework 3 Instructor: D. Cabrera Due June 30. sin θ v x = v r cos θ v θ r. (b) Then use the Cauchy-Riemann equations in polar coordinates MATH 417 Homewok 3 Instucto: D. Cabea Due June 30 1. Let a function f(z) = u + iv be diffeentiable at z 0. (a) Use the Chain Rule and the fomulas x = cosθ and y = to show that u x = u cosθ u θ, v x = v

More information

An Electrical Spinning Particle in Einstein s Unified Field Theory

An Electrical Spinning Particle in Einstein s Unified Field Theory An Electical Spinnin Paticle in Einstein s Unified Field Theoy S.N. Pandey, B.K. Sinha, Ra Kuma.. Depatment of Mathematics, M.N.N.I.T, Allahabad (U.P.) India.. Depatment of Mathematics, U.N.S.I.E.T, V.B.S.P.U.

More information

Chapter 2: Basic Physics and Math Supplements

Chapter 2: Basic Physics and Math Supplements Chapte 2: Basic Physics and Math Supplements Decembe 1, 215 1 Supplement 2.1: Centipetal Acceleation This supplement expands on a topic addessed on page 19 of the textbook. Ou task hee is to calculate

More information

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j.

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j. 7. We denote the two foces F A + F B = ma,sof B = ma F A. (a) In unit vecto notation F A = ( 20.0 N)ˆ i and Theefoe, Phys 201A Homewok 6 Solutions F A and F B. Accoding to Newton s second law, a = [ (

More information

Galilean Transformation vs E&M y. Historical Perspective. Chapter 2 Lecture 2 PHYS Special Relativity. Sep. 1, y K K O.

Galilean Transformation vs E&M y. Historical Perspective. Chapter 2 Lecture 2 PHYS Special Relativity. Sep. 1, y K K O. PHYS-2402 Chapte 2 Lectue 2 Special Relativity 1. Basic Ideas Sep. 1, 2016 Galilean Tansfomation vs E&M y K O z z y K In 1873, Maxwell fomulated Equations of Electomagnetism. v Maxwell s equations descibe

More information

arxiv:gr-qc/ v2 8 Jun 2006

arxiv:gr-qc/ v2 8 Jun 2006 On Quantization of the Electical Chage Mass Dmitiy M Palatnik 1 6400 N Sheidan Rd 2605, Chicago, IL 60626 axiv:g-qc/060502v2 8 Jun 2006 Abstact Suggested a non-linea, non-gauge invaiant model of Maxwell

More information

VECTOR MECHANICS FOR ENGINEERS: STATICS

VECTOR MECHANICS FOR ENGINEERS: STATICS 4 Equilibium CHAPTER VECTOR MECHANICS FOR ENGINEERS: STATICS Fedinand P. Bee E. Russell Johnston, J. of Rigid Bodies Lectue Notes: J. Walt Ole Texas Tech Univesity Contents Intoduction Fee-Body Diagam

More information

Chapter 6 Differential Analysis of Fluid Flow

Chapter 6 Differential Analysis of Fluid Flow 1 Chapte 6 Diffeential Analysis of Fluid Flow Inviscid flow: Eule s equations of otion Flow fields in which the sheaing stesses ae zeo ae said to be inviscid, nonviscous, o fictionless. fo fluids in which

More information

Nonradial linear oscillations of shells in general relativity

Nonradial linear oscillations of shells in general relativity Nonadial linea oscillations of shells in geneal elativity Bend G. Schmidt* Max-Planck-Institut fü Gavitationsphysik, Albet-Einstein-Institut, Schlaatzweg 1, 14473 Potsdam, Gemany Received 30 July 1998;

More information

Cosmology & White Holes

Cosmology & White Holes Semina 1 Mach 013, Vitoia,, Bazil Cosmology & White Holes V. N. Lukash co: E. V. Mikheeva,, V. N. Stokov Asto Space Cente of Lebedev Physics Institute LMS, Phys. Uspechi (#,8) 01; LS, IJMPA 013 Extapolating

More information

Green s Identities and Green s Functions

Green s Identities and Green s Functions LECTURE 7 Geen s Identities and Geen s Functions Let us ecall The ivegence Theoem in n-dimensions Theoem 7 Let F : R n R n be a vecto field ove R n that is of class C on some closed, connected, simply

More information

The R-W Metric Has No Constant Curvature When Scalar Factor R(t) Changes with Time

The R-W Metric Has No Constant Curvature When Scalar Factor R(t) Changes with Time Intenational Jounal of Astonomy and Astophysics,,, 77-8 doi:.436/ijaa..43 Published Online Decembe (http://www.scip.og/jounal/ijaa) The -W Metic Has No Constant Cuvatue When Scala Facto (t) Changes with

More information

Review: Electrostatics and Magnetostatics

Review: Electrostatics and Magnetostatics Review: Electostatics and Magnetostatics In the static egime, electomagnetic quantities do not vay as a function of time. We have two main cases: ELECTROSTATICS The electic chages do not change postion

More information

Earth and Moon orbital anomalies

Earth and Moon orbital anomalies Eath and Moon obital anomalies Si non è veo, è ben tovato Ll. Bel axiv:1402.0788v2 [g-qc] 18 Feb 2014 Febuay 19, 2014 Abstact A time-dependent gavitational constant o mass would coectly descibe the suspected

More information

GROWTH ESTIMATES THROUGH SCALING FOR QUASILINEAR PARTIAL DIFFERENTIAL EQUATIONS

GROWTH ESTIMATES THROUGH SCALING FOR QUASILINEAR PARTIAL DIFFERENTIAL EQUATIONS Annales Academiæ Scientiaum Fennicæ Mathematica Volumen 32, 2007, 595 599 GROWTH ESTIMATES THROUGH SCALING FOR QUASILINEAR PARTIAL DIFFERENTIAL EQUATIONS Teo Kilpeläinen, Henik Shahgholian and Xiao Zhong

More information

MODULE 5a and 5b (Stewart, Sections 12.2, 12.3) INTRO: In MATH 1114 vectors were written either as rows (a1, a2,..., an) or as columns a 1 a. ...

MODULE 5a and 5b (Stewart, Sections 12.2, 12.3) INTRO: In MATH 1114 vectors were written either as rows (a1, a2,..., an) or as columns a 1 a. ... MODULE 5a and 5b (Stewat, Sections 2.2, 2.3) INTRO: In MATH 4 vectos wee witten eithe as ows (a, a2,..., an) o as columns a a 2... a n and the set of all such vectos of fixed length n was called the vecto

More information

Nuclear models: Shell model

Nuclear models: Shell model Lectue 3 Nuclea models: Shell model WS0/3: Intoduction to Nuclea and Paticle Physics,, Pat I Nuclea models Nuclea models Models with stong inteaction between the nucleons Liquid dop model α-paticle model

More information

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased PHYS 0B - HW #7 Sping 2004, Solutions by David Pace Any efeenced euations ae fom Giffiths Poblem statements ae paaphased. Poblem 0.3 fom Giffiths A point chage,, moves in a loop of adius a. At time t 0

More information