Derivation of the Gauss Law of Magnetism, The Faraday Law of Induction, and O(3) Electrodynamics from The Evans Field Theory

Size: px
Start display at page:

Download "Derivation of the Gauss Law of Magnetism, The Faraday Law of Induction, and O(3) Electrodynamics from The Evans Field Theory"

Transcription

1 27 Derivtion of the Guss Lw of Mgnetism, The Frdy Lw of Induction, nd O(3) Electrodynmics from The Evns Field Theory Summry. The Guss Lws of mgnetism nd the Frdy lw of induction re derived from the Evns unified field theory. The geometricl constrints imposed on the generl field theory y these well known lws led self consistently to O(3) electrodynmics. Key words: Evns field theory, Guss lw pplied to mgnetism; Frdy lw of induction; O(3) electrodynmics Introduction In this pper the Guss lw pplied to mgnetism [1] nd the Frdy Lw of induction [1, 2] re derived from the Evns field theory [3] [33] y the imposition of well defined constrints in differentil geometry. Therefore the origin of these well known lws is trced to differentil geometry nd the properties of the generl four dimensionl mnifold known s Evns spcetime. Such inferences re not possile in the Mxwell-Heviside (MH) theory of the stndrd model [1, 2] ecuse MH is not n ojective theory of physics, rther it is theory of specil reltivity covrint only under the Lorentz trnsformtion. An ojective theory of physics must e covrint under ny coordinte trnsformtion[1] nd this is fundmentl philosophicl requirement for ll physics, s first relized y Einstein. This fundmentl requirement is known s generl reltivity nd the generl coordinte trnsformtion leds to generl covrince in contrst to the Lorentz covrince of specil reltivity. The fundmentl lck of ojectivity in the Lorentz covrint MH theory mens tht it is not le to descrie the importnt mutul effects of grvittion nd electromgnetism. In contrst the Evns unified field theory is generlly covrint nd is direct logicl consequence of Einstein s generl reltivity, which is essentilly the geometriztion of physics. The unified field theory is le y definition to nlyze the effects of grvittion on electromgnetism nd vice-vers.

2 Guss Lw, Frdy Lw, nd O(3) Electrodynmics In Section 2 fundmentl geometricl constrint on the generl field theory is derived from considertion of the first Binchi identity of differentil geometry. It is then shown tht this constrint leds to O(3) electrodynmics [3] [33] directly from the Binchi identity. These inferences trce the origin of the Guss lw pplied to mgnetism nd the Frdy lw of induction to differentil geometry nd generl reltivity, s required y Einsteinin nturl philosophy. Section 3 is discussion of the numericl methods needed to solve the generl nd restricted Evns field equtions Geometricl Condition Needed for the Guss Lw of Mgnetism nd the Frdy Lw of Induction nd Derivtion of O(3) Electrodynmics The geometricl origin of these lws in the Evns field theory is the first Binchi identity of differentil geometry [1]: which cn e rewritten s: D T = R q (27.1) d T = R q ω T. (27.2) Here T is the vector vlued torsion two-form, R is the tensor vlued curvture or Riemnn two-form; q is the vector vlued tetrd one-form;ω is the spin connection, which cn e regrded s one-form [1]. The symol D denotes the covrint exterior derivtive nd d denotes the ordinry exterior derivtive. The Binchi identity ecomes the homogeneous Evns field eqution (HE) using: A = A (0) q, (27.3) F = A (0) T. (27.4) Here A (0) is sclr vlued electromgnetic potentil mgnitude (whose S.I. unit is volt s / m). Thus A is the vector vlued electromgnetic potentil one-form nd F is the vector vlued electromgnetic field two-form. The HE is therefore: d F = R A ω F (27.5) = µ 0 j where: j = 1 µ 0 ( R A ω F ) (27.6) is the homogeneous current, vector vlued three-form. Here µ 0 is the S. I. vcuum permeility.

3 27.2 Geometricl Condition 447 The homogeneous current is theoreticlly non-zero. known experimentlly to gret precision tht: However it is d F 0. (27.7) Eqn. (27.7) encpsultes the two lws which re to e derived here from Evns field theory. These re usully written in vector nottion s follows. The Guss lw pplied to mgnetism is: B 0, (27.8) where B is mgnetic flux density. The Frdy lw of induction is: E + B t 0 (27.9) where E is electric field strength. The index ppering in Eqns. (27.8) nd (27.9) comes from eqution (27.5), i.e. from generl reltivity s required y Einstein. The physicl mening of is tht it indictes sis set of the tngent undle spcetime, Minkowski or flt spcetime. Any sis elements (e.g. unit vectors or Puli mtrices) cn e used [1]in the tngent spcetime of differentil geometry, nd the sis elements cn e used to descrie sttes of polriztion [3] [33], for exmple circulr polriztion first discovered experimentlly y Argo in Argo ws the first to oserve wht is now known s the two trnsverse sttes of circulr polriztion. It is convenient [3] [33] to descrie these sttes of circulr polriztion y the well known [34] complex circulr sis: = (1), (2) nd (3) (27.10) whose unit vectors re: e (1) = 1 2 (i ij) = e (2), (27.11) e (3) = k (27.12) where * denotes complex conjugtion. Ech stte of circulr polriztion cn e descried y two complex conjugtes. One sense of circulrly polrized rdition is descried y the complex conjugtes: A (1) 1 = A(0) 2 (i ij) e iφ, (27.13) A (2) 1 = A(0) 2 (i + ij) e iφ. (27.14) The other sense of circulrly polrized rdition is descried y the complex conjugtes:

4 Guss Lw, Frdy Lw, nd O(3) Electrodynmics A (1) 2 = A(0) 2 (i + ij) e iφ, (27.15) A (2) 2 = A(0) 2 (i ij) e iφ. (27.16) Here φ is the electromgnetic phse nd Eqns. (27.13) nd (27.16) re solutions of Eq. (27.7). The experimentlly oservle Evns spin field B (3) [3] [33] is defined y the vector cross product of one conjugte with the other. In non-liner optics [3] [33] this is known s the conjugte product, nd is oserved experimentlly in the inverse Frdy effect, (IFE), the mgnetiztion of ny mteril mtter y circulrly polrized electromgnetic rdition. In the sense of circulr polriztion defined y Eqns. (27.13) nd (27.14): B (3) 1 = iga (1) 1 A (2) 1 = B (0) k (27.17) where g = κ (27.18) A (0) nd where κ is the wvenumer. In the sense of circulr polriztion defined y Eqns. (27.15) nd (27.16) B (3) reverses sign: B (3) 2 = iga (1) 2 A (2) 2 = B (0) k (27.19) nd this is oserved experimentlly [3] [33] ecuse the oservle mgnetiztion chnges sign when the hndedness or sense of circulr polriztion is reversed. Liner polriztion is the sum of 50% left nd 50% right circulr polriztion nd in this stte the IFE is oserved to dispper. Thus B (3) in linerly polrized em vnishes ecuse hlf the em hs positive B (3) nd the other hlf negtive B (3). The B (3) field ws first inferred y Evns in 1992 [34] nd it ws recognized for the first time tht the phse free mgnetiztion of the IFE is due to third (spin) stte of polriztion now recognized s = (3) in the unified field theory. The Guss lw nd the Frdy lw of induction hold for = (3), ut it is oserved experimentlly tht A (3) = 0 [3] [33]. Therefore: B (3) 0 (27.20) B (3) t 0. (27.21) The fundmentl reson for this is tht the spin of the electromgnetic field produces n ngulr momentum which is oserved experimentlly in the Beth effect [3] [33]. The electromgnetic field is negtive under chrge conjugtion symmetry (C), so the Beth ngulr momentum produces B (3) directly, ngulr momentum nd mgnetic field eing oth xil vectors. The

5 27.2 Geometricl Condition 449 puttive rdited E (3) would e polr vector if it existed, nd would not e produced y spin. There is however no electric nlogue of the inverse Frdy effect, circulrly polrized electromgnetic field does not produce n electric polriztion experimentlly, only mgnetiztion. Similrly, in the originl Frdy effect, sttic mgnetic field rottes the plne of linerly polrized rdition, ut sttic electric field does not. The Frdy effect nd the IFE re explined using the sme hyperpolrizility tensor in the stndrd model, nd in the Evns field theory y term in the well defined Mclurin expnsion of the spin connection in terms of the tetrd, producing the IFE mgnetiztion: M (3) = i µ 0 g A (1) A (2) (27.22) where A (1) nd A (2) re complex conjugte tetrd elements comined into vectors [3] [33]. Similrly ll non-liner opticl effects in the Evns field theory re, self consistently, properties of the Evns spcetime or generl fourdimensionl se mnifold. The unified field theory therefore llows non-liner optics to e uilt up from spcetime, s required in generl reltivity. In the MH theory the spcetime is flt nd cnnot e chnged, so non-liner optics must e descried using constitutive reltions extrneous to the originl liner theory. In the unified field theory the Evns spin field nd the conjugte product re deduced self consistently from the experimentl oservtion: Eqs.(27.23) nd (27.6) imply: j 0. (27.23) R q = ω T (27.24) to high precision.in other words the Guss lw nd Frdy lw of induction pper to e true within contemporry experimentl precision.the reson for this in generl reltivity (i.e. ojective physics) is Eq.(27.24), constrint of differentil geometry. Using the Murer-Crtn structure equtions of differentil geometry [1]: T = D q (27.25) R = D ω. (27.26) Eq.(27.24) ecomes the following experimentlly implied constrint on the generl unified field theory: ( D ω ) q = ω ( D q ). (27.27) A prticulr solution of Eq.(27.27) is: ω = κɛ cq c (27.28)

6 Guss Lw, Frdy Lw, nd O(3) Electrodynmics where ɛ c is the Levi-Civit tensor in the flt tngent undle spcetime.being flt spcetime, Ltin indices cn e rised nd lowered in contrvrint covrint nottion nd so we my rewrite Eq.(27.28) s: ω = κɛ c q c. (27.29) Eqn.(27.29) sttes tht the spin connection is n ntisymmetric tensor dul to the xil vector within sclr vlued fctor with the dimensions of inverse metres. Thus Eq.(27.29) defines the wve-numer mgnitude, κ, in the unified field theory. It follows from Eqn.(27.29) tht the covrint derivtive defining the torsion form in the first Murer-Crtn structure eqution (27.25) cn e written s: T = d q + ω q (27.30) = d q + κq q c (27.31) from which it follows,using Eqs.(27.3) nd (27.4), tht: F = d A + ga A c (27.32) In the complex circulr sis,eq.(27.32) cn e expnded s the cycliclly symmetric set of three equtions: F (1) = d A (1) iga (2) A (3) (27.33) F (2) = d A (2) iga (3) A (1) (27.34) F (3) = d A (3) iga (1) A (2) (27.35) with O(3) symmetry [3] [33]. These re the defining reltions of O(3) electrodynmics, developed y Evns from 1992 to 2003 [3] [33] It hs een shown tht O(3) electrodynmics is direct result of the unified field theory given the experimentl constrints imposed y the Guss lw nd the Frdy lw of induction. It follows tht O(3) electrodynmics utomticlly produces these lws, i.e.: d F () = 0, = 1, 2, 3 (27.36) s oserved experimentlly.the existence of the conjugte product hs een DEDUCED in Eq.(27.32) from differentil geometry,nd it follows tht the spin field nd the inverse Frdy effect hve lso een deduced from differentil geometry nd the Evns unified field theory of generl reltivity or ojective physics. This is mjor dvnce from the stndrd model nd the MH theory of specil reltivity.

7 27.3 Numericl Methods of Solutions 27.3 Numericl Methods of Solutions 451 In generl the homogeneous nd inhomogeneous Evns field equtions must e solved simultneously for given initil nd oundry conditions. In this section the two equtions re written out in tensor nottion nd susidiry informtion summrized. The homogeneous field eqution in tensor nottion is: µ F νρ + ν F ρµ + ρ F µν = R µν A ρ + R νρ A µ + R ρµ A ν ω µ F νρ ω ν F ρµ ω ρ F µν (27.37) nd this is equivlent to the reones or minimlist nottion of differentil geometry: d F = R A ω F (27.38) where ll indices hve een suppressed. For the purposes of electricl engineering Eq.(27.37) is,to n excellent pproximtion: µ F νρ + ν F ρµ + ρ F µν = 0 (27.39) Eq.(27.39) is equivlent to the Guss Lw pplied to mgnetism: nd the Frdy Lw of induction: B = 0 (27.40) B + E t = 0 (27.41) for ll polriztion sttes. The exceedingly importnt influence of grvittion on electromgnetism nd vice vers must however e computed in generl when the right hnd side of Eq.(27.37) is non-zero. This tiny ut in generl non-zero influence leds to violtion of the well known lws (27.40) nd (27.41), nd this must e serched for with high precision instrumenttion. Eq.(27.39) my e rewritten s the Hodge dul eqution: µ F µν = 0 (27.42) nd for ech index this is homogeneous Mxwell-Heviside field eqution. In generl F µν is the Hodge dul of Fµν in Evns spcetime nd j ν is the Hodge dul of the chrge-current density three-form defined y the right hnd side of Eq.(27.37), i.e.y: µ F νρ + ν F ρµ + ρ F ( µν = µ 0 j µνρ + j νρµ + j ) ρµν (27.43) where:

8 Guss Lw, Frdy Lw, nd O(3) Electrodynmics j µνρ = 1 ) (R µν µ A ρ ω µ F νρ 0 etc. (27.44) Thus: j σ = 1 6 ɛµνρ σj µνρ = 1 6 ɛνρµ σj νρµ (27.45) = 1 6 ɛρµν σj ρµν nd F µσ = 1 2 ɛνρ µσf νρ, F νσ = 1 2 ɛρµ νσf ρµ, (27.46) F ρσ = 1 2 ɛµν ρσf µν. In computing these Hodge duls the correct generl definition mps from p-form of differentil geometry to n (n-p)-form of differentil geometry in the generl n dimensionl mnifold. The generl four dimensionl mnifold is the Evns spcetime, so nmed to distinguish it from the Riemnnin spcetime used in Einstein s field theory of grvittion. The Hodge dul is in generl [1]: X µ1...µ n p = 1 p! ɛν1...νp µ 1...µ n p X ν1...ν p. (27.47) The generl Levi-Civit symol is: 1 if µ 1 µ 2...µ n is n even permuttion ɛ µ 1µ 2...µ n = 1 if µ 1 µ 2...µ n is n odd permuttion 0 otherwise (27.48) nd the Levi-Civit tensor used in Eq.(27.47) is: ɛ µ1µ 2...µ n = ( g ) 1/2 ɛ µ 1µ 2...µ n (27.49) where g is the numericl vlue (i.e. numer) of the determinnt of the metric tensor g µν. The field tensor is defined y the torsion tensor: nd the potentil is defined y the tetrd: F µν = A (0) T µν (27.50)

9 where: 27.3 Numericl Methods of Solutions 453 A µ = A (0) q µ. (27.51) The metric is fctorized into dot product of tetrds: g µν = q µq ν η (27.52) η = (27.53) is the digonl metric tensor of the tngent undle spcetime, Minkowski or flt spcetime. The gmm nd spin connections re relted y the tetrd postulte: D µ q ν = µ q ν + ω µ q ν Γ λ µν q λ = 0. (27.54) The torsion nd curvture (or Riemnn) tensors re defined y the Murer-Crtn structure reltions of differentil geometry. The torsion tensor is the covrint derivtive of the tetrd nd is: T λ µν = qλ T µν = Γ λ µν Γ λ νµ. (27.55) It therefore vnishes for the Christoffel connection of Einstein s grvittionl theory: Γ λ µν = Γ λ νµ. (27.56) The curvture tensor is the covrint derivtive of the spin connection nd is: R σ λνµ = qσ q λr νµ. (27.57) It follows tht: nd R νµ = νω µ µω ν + ω νcω c µ ω µcω c ν (27.58) R σ λνµ = νγ σ µλ µγ σ νλ + Γ σ νρ Γ ρ µλ Γ σ µρ Γ ρ νλ. (27.59) The Evns spcetime is therefore completely defined y the structure reltions. The homogeneous field eqution is the first Binchi identity of differentil geometry within the C negtive fctor A (0). The second Binchi identity leds to the Noether Theorem of Evns field theory, nd sttes tht the covrint derivtive of the curvture tensor vnishes identiclly. Note tht Eq.(27.39) is equivlent to the use of Riemnn norml coordintes nd loclly flt spcetime, ecuse it is n eqution in ordinry derivtives, not covrint derivtives. In generl, g, the modulus of the determinnt of the metric, in Eq.(27.49) is function of x µ, ut t point p in

10 Guss Lw, Frdy Lw, nd O(3) Electrodynmics the Evns spcetime or mnifold M it is lwys possile to define the Riemnn norml coordinte system so the metric is in cnonicl form, nd: µ g = 0. (27.60) This defines the loclly flt spcetime. Note crefully tht the generl homogeneous eqution (27.37) cnnot e expressed s Hodge dul eqution of type (27.39), so the pproprite eqution for numericl solution must lwys e Eq.(27.37). Eq.(27.39) is mentioned only ecuse of the trditionl method of expressing the homogeneous Mxwell-Heviside eqution of Minkowski spcetime (HME) s the Hodge dul eqution. The correct form of the HME is the following Binchi identity of Minkowski spcetime: λ F µν + µ F νλ + ν F λµ = 0 (27.61) spcetime in which the Hodge dul is definle s: F µν = 1 2 ɛµνρσ F ρσ. (27.62) It my then e proven tht Eq.(27.61) is the sme eqution s: The proof is s follows. From Eq.(27.63): nd using Eq.(27.62): µ F µν = 0. (27.63) λ F λρ + µ F µρ + ν F νρ = 0 (27.64) 1 ( ( λ ɛ λρµν ) ( F 2 µν + µ ɛ µρνλ ) ( F νλ + ν ɛ νρλµ )) F λµ = 0. (27.65) Using the Leiniz Theorem nd the constncy of ɛ µνρσ in Minkowski spcetime, Eq.(27.65) ecomes: which is upon using: ɛ λρµν λ F µν + ɛ µρνλ µ F νλ + ɛ νρλµ ν F λµ = 0. (27.66) We my dd individul indices of Eq.(27.66), to give, for exmple: ɛ 1ρ23 1 F 23 + ɛ 2ρ31 2 F 31 + ɛ 3ρ12 3 F 12 + = 0 (27.67) 1 F F F 12 + = 0 (27.68) ɛ 1023 = ɛ 2031 = ɛ 3012 = 1. (27.69) Proceeding in this wy we see tht Eq.(27.61) is the sme s Eq.(27.63).Note crefully tht this proof is not true in generl for Evns spcetime, ecuse in tht spcetime we otin results such s:

11 27.3 Numericl Methods of Solutions 455 µ F µσ = 1 ( 2 µ ɛ νρ µσf ) 1 ( νρ = ɛ νρ 2 µσ µ F νρ + ( µ ɛ νρ ) µσ) F νρ nd since depends on, one otins: (27.70) µ ɛ νρ µσ 0 (27.71) nd there is n extr term which does not pper in Eq.(27.63) of Minkowski spcetime. Only in the specil cse of Eq.(27.62) do we otin: µ ɛ νρ µσ = 0. (27.72) Therefore in generl, the homogeneous Evns eqution (27.37) must e solved simultneously with the inhomogeneous Evns eqution.the ltter is n expression for the covrint exterior derivtive of the Hodge dul of Fµν. In the minimlist or reones nottion of differentil geometry this expression is: d F = R A ω F = µ 0 J (27.73) where R denotes the Hodge dul of the curvture form. Eq.(27.73) is the ojective or generlly covrint expression in unified field theory of the inhomogeneous Mxwell-Heviside eqution (IMH) of specil reltivity: d F = µ 0 J. (27.74) It is seen y comprison of Eqs.(27.73) nd (27.74) tht in the unified field theory d hs een replced y D s required. Since oth F nd R in Eq.(27.38) re two-forms it follows y symmetry tht if one tkes the Hodge dul of F on the left hnd side, one must tke the Hodge dul of R on the right hnd side. The reson is tht the Hodge dul of ny two-form in Evns spcetime is lwys nother two-form. It is convenient to rewrite Eq.(27.73) s: D F = R A (27.75) nd in nlogy with Eq.(27.37), the tensoril expression for Eq.(27.73) is: µ F νρ + ν F ρµ + ρ F µν = R µν A ρ + R νρ A µ + R ρµ A ν ω µ F νρ ω ν F ρµ ω ρ F µν. (27.76) Therefore the generl computtionl tsk is to solve Eqs.(27.37) nd (27.76) simultneously for given initil nd oundry conditions. In the lst nlysis this is prolem in simultneous prtil differentil equtions. We my now define the inhomogeneous current ( J µνρ = 1 µ R 0 µν A ρ ω F ) µ νρ (27.77).

12 Guss Lw, Frdy Lw, nd O(3) Electrodynmics nd we my note tht J µνρ is in generl much lrger thn the homogeneous current j µνρ. Therefore J µνρ is of gret prcticl importnce for the cquisition of electric power from Evns spcetime nd for counter grvittionl technology in the erospce industry. Finlly convenient form of the inhomogeneous field eqution my e otined from the following considertions.we first construct the following Hodge dul: F µν = 1 2 ɛµνρσ F ρσ (27.78) in the MH limit: nd note tht: d F = 0 (27.79) d F = µ 0 J (27.80) ( d F ) µν 1 2 ɛµνρσ (d F ) ρσ. (27.81) In convenient shorthnd nottion this result my e written s: result which ecomes: d F 1 2 ɛ d F (27.82) d F 1 2 g 1 2 ɛ d F (27.83) in Evns spcetime. This is key result ecuse it shows tht J is not zero if j is zero or lmost zero, nd it is J tht is the importnt current term for the cquisition of electric power from Evns spcetime. For the purposes of computtion systemtic method of constructing the inhomogeneous Evns field eqution (IE) is needed, where every term needed for coding is defined precisely. In order to do this egin with the fundmentl definitions of differentil geometry, the two Murer-Crtn structure equtions: nd the two Binchi identities: T = D q (27.84) R = D ω (27.85) D T = R q (27.86) D R = 0. (27.87) In order to correctly construct the Hodge duls of T nd R ppering in the IE the determinnt of the metric must e defined correctly in ech cse

13 27.3 Numericl Methods of Solutions 457 (see Eq.(27.49)). In order to proceed consider the limit of the Evns unified field theory tht gives Einstein s field theory of grvittion uninfluenced y electromgnetism. In the Einstein limit the metric tensor is symmetric nd is defined y the inner or dot product of two tetrds: (S) gµν = q (S) µ q (S) ν η. (27.88) The differentil geometry pproprite to the Einstein theory is then: T (S) = 0 (27.89) d q (S) = ω (S) q (S), (27.90) R (S) q (S) = 0. (27.91) The determinnt of the metric is defined in this limit y: (S) g (S) = gµν (27.92) nd so the Hodge dul of the Riemnn form is defined in Einstein s theory of grvittion y: R (S) = 1 2 g (S) µν 1 2 ɛ R (S). (27.93) Consider next the limit of the Evns field theory tht gives the free electromgnetic field when there is no field mtter interction, mtter eing defined y the presence of non-zero mss. The differentil geometry tht defines this limit is: T (A) = D q (A), (27.94) R (A) g c (A) µν = q (A) nd the determinnt of the metric is: = D ω (A), (27.95) µ q (A) ν, (27.96) g (A) = g c (A) µν. (27.97) The Hodge duls of the torsion nd Riemnn forms for the free electromgnetic field re therefore: T (A) = 1 2 g(a) 1 2 ɛ T (A), (27.98) R (A) = 1 2 g(a) 1 2 ɛ R (A). (27.99) Thirdly, when, the electromgnetic field intercts with mtter, s in the IE, the pproprite differentil geometry is:

14 Guss Lw, Frdy Lw, nd O(3) Electrodynmics nd the determinnt of the metric tensor is now: T = D q, (27.100) R = D ω, (27.101) g µν = q µq ν, (27.102) g = g µν. (27.103) The metric tensor itself is the sum of symmetric nd nti-symmetric component metric tensors: q µq ν = 1 ( (q 2 µ q ) (S) ( ν + q µ q ) (A) ) ν. (27.104) The Hodge dul of the Riemnn form in the IE is therefore: R = 1 2 g 1 2 ɛ R, (27.105) ecuse in generl oth the symmetric nd ntisymmetric metrics contriute to the Riemnn tensor or Riemnn form when there is field mtter interction However, the Hodge dul of the torsion form in the IE is: T = 1 2 g(a) 1 2 ɛ T, (27.106) ecuse only the ntisymmetric metric contriutes to the torsion tensor or torsion form from Eq.(27.94). Therefore the computtionl lgorithm is fully defined, nd the computtionl tsk in generl is to solve the HE nd IE SIMULTANEOUSLY for given initil nd oundry conditions. The HE nd IE contin more informtion thn the equivlents in Mxwell-Heviside field theory, nd the engineering tsk is to CAD/CAM circuit tking electric power from Evns spcetime, defined y the generl four dimensionl mnifold in which the Riemnn nd torsion tensors re oth non-zero. In the Minkowski spcetime of Mxwell-Heviside field theory oth tensors re zero. We must use the computer to define this extr source of power nd to optimize circuits which utilize this extr source of power in prcticl devices. Acknowledgments The Ted Annis Foundtion, Crddock Inc., John B.Hrt nd other scholrs re thnked for funding this work, nd the AIAS group for mny interesting discussions.

15 References 1. S.P.Crroll., Lecture Notes in Generl Reltivity ( grdute course t Hrvrd, UC Snt Brr nd U.Chicgo, pulic domin rxic:gr-gq v1 Dec 1997, pulic domin). 2. L.H.Ryder, Quntum Field Theory, (Cmridge Univ Press,1996,2nd ed.). 3. M.W.Evns, A Unified Field Theory for Grvittion nd Electromgnetism, Found.Phys.Lett., 16, 367 (2003). 4. M.W.Evns, A Generlly Covrint Wve Eqution for Grnd Unified Field Theory, Found.Phys.Lett., 16, 507 (2003). 5. M.W.Evns, The Equtions of Grnd Unified Field Theory in Terms of the Murer-Crtn Structure reltions of Differentil Geometry, Found.Phys.Lett.,17,25 (2004). 6. M.W.Evns, Derivtion of Dirc s Eqution from the Evns Wve Eqution, Found.Phys.Lett.,17,149 (2004). 7. M.W.Evns, Unifiction of the Grvittionl nd Strong Nucler Fields, Found.Phys.Lett., 17,267 (2004). 8. M.W.Evns, The Evns Lemm of Differentil Geometry, Found.Phys.Lett., 17,433 (2004). 9. M.W.Evns, Derivtion of the Evns Wve Eqution form the Lgrngin nd Action,Origin of the Plnck Constnt in Generl Reltivity, Found.Phys.Lett.,17,535 (2004). 10. M.W.Evns et. l. (AIAS Author Group), Development of the Evns Wve Eqution in the Wek Field Limit: the Electrogrvitic Eqution, Found.Phys.Lett., 17,497 (2004). 11. M.W.Evns, Physicl Optics, the Sgnc Effect nd the Ahronov Bohm Effect in the Evns Unified Field Theory, Found.Phys.Lett., 17, 301 (2004). 12. M.W.Evns, Derivtion of the Geometricl Phse from the Evns Phse Lw of Generlly Covrint Unified Field Theory, Found.Phys.Lett.,17,393 (2004). 13. M.W.Evns, Derivtion of the Lorentz Boost from the Evns Wve Eqution, Found.Phys.Lett.,17,663 (2004). 14. M.W.Evns,The Electromgnetic Sector of the Evns Field Theory, Found.Phys.Lett., in press (2005),preprint on M.W.Evns, New Concepts from the Evns Field Theory,Prt One:The Evolution of Curvture, Oscilltory Universe without Singulrity nd generl Force nd Field Equtions, Found.Phys.Lett., in press (2005),preprint on

16 460 References 16. M.W.Evns, New Concepts from the Evns Field Theory,Prt Two: Derivtion of the Heisenerg Eqution nd Reinterprettion of the Heisenerg Uncertinty Principle, Found.Phys.Lett., in press (2005), preprint on M.W.Evns, The Spinning nd Curving of Spcetime, the Electromgnetic nd Grvittionl Fields in the Evns Unified Field Theory, Found.Phys.Lett., in press,(2005), preprint on M.W.Evns, Derivtion of O(3) Electrodynmics from Generlly Covrint Unified Field Theory, Found.Phys.Lett., in press, preprint on M.W.Evns, Derivtion of O(3) Electrodynmics form the Evns Unified Field Theory, Found.Phys.Lett., in press, preprint on M.W.Evns, Clcultion of the Anomlous Mgnetic Moment of the Electron, Found.Phys.Lett., in press, preprint on M.W.Evns, Generlly Covrint Electro-wek Theory, Found.Phys.Lett., in press, preprint on M.W.Evns, Evns Field Theory of Neutrino Oscilltions, Found.Phys.Lett., in press, preprint on M.W.Evns, The Interction of Grvittion nd Electromgnetism, Found.Phys.Lett., preprint on M.W.Evns, Electromgnetic Energy from Grvittion, Found.Phys.Lett., in press, preprint on M.W.Evns, The Fundmentl Invrints of the Evns Field Theory, Found.Phys.Lett., in press, preprint on M.W.Evns, The Homogeneous nd Inhomogeneous Evns Field Equtions, Found.Phys.Lett., in press, preprint on M.W.Evns, Generlly Covrint Unified Field Theory: the Geometriztion of Physics, (in press, 2005), preprint on L.Felker, The Evns Equtions, (freshmn text in prep.). 29. M.Anderson, Artspeed Wesite for the Collected Works of Myron Evns, M.W.Evns nd L.B.Crowell, Clssicl nd Quntum Electrodynmics nd the B (3) Field (World Scientific,Singpore,2001). 31. M.W.Evns (ed.), Modern Nonliner Optics, specil topicl issue in three prts of I.Prigogine nd S.A.Rice (series eds.), Advnces in Chemicl Physics, (Wile Interscience, New York, 2001, 2nd ed., nd 1992,1993,1997,1st ed.), vols 119 nd M.W.Evns, J.-P.Vigier et l, The Enigmtic Photon, (Kluwer,Dordrecht,1994 to 2002,hrdck nd softck), in five volumes. 33. M.W.Evns nd A.A.Hsnein, The Photomgneton in Quntum Field Theory (World Scientific,Singpore,1994) 34. M.W.Evns, Physic B, 182,227,237 (1992).

Some basic concepts of fluid dynamics derived from ECE theory

Some basic concepts of fluid dynamics derived from ECE theory Some sic concepts of fluid dynmics 363 Journl of Foundtions of Physics nd Chemistry, 2, vol. (4) 363 374 Some sic concepts of fluid dynmics derived from ECE theory M.W. Evns Alph Institute for Advnced

More information

Simplified proofs of the Cartan structure equations

Simplified proofs of the Cartan structure equations 382 M.W. Ens Journl of Foundtions of Physics nd Chemistry, 2011, ol. 1 (4) 382 390 Simplified proofs of the Crtn structure eutions M.W. Ens 1 Alph Institute for Adnced Studies (www.is.us) The two Crtn

More information

GAUGE THEORY ON A SPACE-TIME WITH TORSION

GAUGE THEORY ON A SPACE-TIME WITH TORSION GAUGE THEORY ON A SPACE-TIME WITH TORSION C. D. OPRISAN, G. ZET Fculty of Physics, Al. I. Cuz University, Isi, Romni Deprtment of Physics, Gh. Aschi Technicl University, Isi 700050, Romni Received September

More information

7.6 The Riemann curvature tensor

7.6 The Riemann curvature tensor 7.6. The Riemnn curvture tensor 53 7.6 The Riemnn curvture tensor Before we egin with the derivtion of the Riemnn curvture tensor, rief discussion of the concept of curvture ppers pproprite. Mthemticins

More information

Chapter 4 Contravariance, Covariance, and Spacetime Diagrams

Chapter 4 Contravariance, Covariance, and Spacetime Diagrams Chpter 4 Contrvrince, Covrince, nd Spcetime Digrms 4. The Components of Vector in Skewed Coordintes We hve seen in Chpter 3; figure 3.9, tht in order to show inertil motion tht is consistent with the Lorentz

More information

d 2 Area i K i0 ν 0 (S.2) d 3 x t 0ν

d 2 Area i K i0 ν 0 (S.2) d 3 x t 0ν PHY 396 K. Solutions for prolem set #. Prolem 1: Let T µν = λ K λµ ν. Regrdless of the specific form of the K λµ ν φ, φ tensor, its ntisymmetry with respect to its first two indices K λµ ν K µλ ν implies

More information

4 The dynamical FRW universe

4 The dynamical FRW universe 4 The dynmicl FRW universe 4.1 The Einstein equtions Einstein s equtions G µν = T µν (7) relte the expnsion rte (t) to energy distribution in the universe. On the left hnd side is the Einstein tensor which

More information

Lecture Solution of a System of Linear Equation

Lecture Solution of a System of Linear Equation ChE Lecture Notes, Dept. of Chemicl Engineering, Univ. of TN, Knoville - D. Keffer, 5/9/98 (updted /) Lecture 8- - Solution of System of Liner Eqution 8. Why is it importnt to e le to solve system of liner

More information

Things to Memorize: A Partial List. January 27, 2017

Things to Memorize: A Partial List. January 27, 2017 Things to Memorize: A Prtil List Jnury 27, 2017 Chpter 2 Vectors - Bsic Fcts A vector hs mgnitude (lso clled size/length/norm) nd direction. It does not hve fixed position, so the sme vector cn e moved

More information

A response to the papers by Hehl and Hehl and Obukhov

A response to the papers by Hehl and Hehl and Obukhov Response to the Ppers y Hehl nd Hehl nd Oukhov 573 Journl of Foundtions of Physics nd Chemistry, 011, vol. 1 (5) 573 616 A response to the ppers y Hehl nd Hehl nd Oukhov M.W. Evns 1 *Alph Institute for

More information

2. VECTORS AND MATRICES IN 3 DIMENSIONS

2. VECTORS AND MATRICES IN 3 DIMENSIONS 2 VECTORS AND MATRICES IN 3 DIMENSIONS 21 Extending the Theory of 2-dimensionl Vectors x A point in 3-dimensionl spce cn e represented y column vector of the form y z z-xis y-xis z x y x-xis Most of the

More information

A Vectors and Tensors in General Relativity

A Vectors and Tensors in General Relativity 1 A Vectors nd Tensors in Generl Reltivity A.1 Vectors, tensors, nd the volume element The metric of spcetime cn lwys be written s ds 2 = g µν dx µ dx ν µ=0 ν=0 g µν dx µ dx ν. (1) We introduce Einstein

More information

Analytically, vectors will be represented by lowercase bold-face Latin letters, e.g. a, r, q.

Analytically, vectors will be represented by lowercase bold-face Latin letters, e.g. a, r, q. 1.1 Vector Alger 1.1.1 Sclrs A physicl quntity which is completely descried y single rel numer is clled sclr. Physiclly, it is something which hs mgnitude, nd is completely descried y this mgnitude. Exmples

More information

Review of Gaussian Quadrature method

Review of Gaussian Quadrature method Review of Gussin Qudrture method Nsser M. Asi Spring 006 compiled on Sundy Decemer 1, 017 t 09:1 PM 1 The prolem To find numericl vlue for the integrl of rel vlued function of rel vrile over specific rnge

More information

dx dt dy = G(t, x, y), dt where the functions are defined on I Ω, and are locally Lipschitz w.r.t. variable (x, y) Ω.

dx dt dy = G(t, x, y), dt where the functions are defined on I Ω, and are locally Lipschitz w.r.t. variable (x, y) Ω. Chpter 8 Stility theory We discuss properties of solutions of first order two dimensionl system, nd stility theory for specil clss of liner systems. We denote the independent vrile y t in plce of x, nd

More information

Matrix Algebra. Matrix Addition, Scalar Multiplication and Transposition. Linear Algebra I 24

Matrix Algebra. Matrix Addition, Scalar Multiplication and Transposition. Linear Algebra I 24 Mtrix lger Mtrix ddition, Sclr Multipliction nd rnsposition Mtrix lger Section.. Mtrix ddition, Sclr Multipliction nd rnsposition rectngulr rry of numers is clled mtrix ( the plurl is mtrices ) nd the

More information

Vector potential quantization and the photon wave-particle representation

Vector potential quantization and the photon wave-particle representation Vector potentil quntiztion nd the photon wve-prticle representtion Constntin Meis, Pierre-Richrd Dhoo To cite this version: Constntin Meis, Pierre-Richrd Dhoo. Vector potentil quntiztion nd the photon

More information

221B Lecture Notes WKB Method

221B Lecture Notes WKB Method Clssicl Limit B Lecture Notes WKB Method Hmilton Jcobi Eqution We strt from the Schrödinger eqution for single prticle in potentil i h t ψ x, t = [ ] h m + V x ψ x, t. We cn rewrite this eqution by using

More information

PHYS 4390: GENERAL RELATIVITY LECTURE 6: TENSOR CALCULUS

PHYS 4390: GENERAL RELATIVITY LECTURE 6: TENSOR CALCULUS PHYS 4390: GENERAL RELATIVITY LECTURE 6: TENSOR CALCULUS To strt on tensor clculus, we need to define differentition on mnifold.a good question to sk is if the prtil derivtive of tensor tensor on mnifold?

More information

Classical Mechanics. From Molecular to Con/nuum Physics I WS 11/12 Emiliano Ippoli/ October, 2011

Classical Mechanics. From Molecular to Con/nuum Physics I WS 11/12 Emiliano Ippoli/ October, 2011 Clssicl Mechnics From Moleculr to Con/nuum Physics I WS 11/12 Emilino Ippoli/ October, 2011 Wednesdy, October 12, 2011 Review Mthemtics... Physics Bsic thermodynmics Temperture, idel gs, kinetic gs theory,

More information

Math 520 Final Exam Topic Outline Sections 1 3 (Xiao/Dumas/Liaw) Spring 2008

Math 520 Final Exam Topic Outline Sections 1 3 (Xiao/Dumas/Liaw) Spring 2008 Mth 520 Finl Exm Topic Outline Sections 1 3 (Xio/Dums/Liw) Spring 2008 The finl exm will be held on Tuesdy, My 13, 2-5pm in 117 McMilln Wht will be covered The finl exm will cover the mteril from ll of

More information

Physics Graduate Prelim exam

Physics Graduate Prelim exam Physics Grdute Prelim exm Fll 2008 Instructions: This exm hs 3 sections: Mechnics, EM nd Quntum. There re 3 problems in ech section You re required to solve 2 from ech section. Show ll work. This exm is

More information

Physics 201 Lab 3: Measurement of Earth s local gravitational field I Data Acquisition and Preliminary Analysis Dr. Timothy C. Black Summer I, 2018

Physics 201 Lab 3: Measurement of Earth s local gravitational field I Data Acquisition and Preliminary Analysis Dr. Timothy C. Black Summer I, 2018 Physics 201 Lb 3: Mesurement of Erth s locl grvittionl field I Dt Acquisition nd Preliminry Anlysis Dr. Timothy C. Blck Summer I, 2018 Theoreticl Discussion Grvity is one of the four known fundmentl forces.

More information

New Expansion and Infinite Series

New Expansion and Infinite Series Interntionl Mthemticl Forum, Vol. 9, 204, no. 22, 06-073 HIKARI Ltd, www.m-hikri.com http://dx.doi.org/0.2988/imf.204.4502 New Expnsion nd Infinite Series Diyun Zhng College of Computer Nnjing University

More information

How do we solve these things, especially when they get complicated? How do we know when a system has a solution, and when is it unique?

How do we solve these things, especially when they get complicated? How do we know when a system has a solution, and when is it unique? XII. LINEAR ALGEBRA: SOLVING SYSTEMS OF EQUATIONS Tody we re going to tlk out solving systems of liner equtions. These re prolems tht give couple of equtions with couple of unknowns, like: 6= x + x 7=

More information

Jim Lambers MAT 169 Fall Semester Lecture 4 Notes

Jim Lambers MAT 169 Fall Semester Lecture 4 Notes Jim Lmbers MAT 169 Fll Semester 2009-10 Lecture 4 Notes These notes correspond to Section 8.2 in the text. Series Wht is Series? An infinte series, usully referred to simply s series, is n sum of ll of

More information

CHAPTER 1 PROGRAM OF MATRICES

CHAPTER 1 PROGRAM OF MATRICES CHPTER PROGRM OF MTRICES -- INTRODUCTION definition of engineering is the science y which the properties of mtter nd sources of energy in nture re mde useful to mn. Thus n engineer will hve to study the

More information

Physics 202, Lecture 14

Physics 202, Lecture 14 Physics 202, Lecture 14 Tody s Topics Sources of the Mgnetic Field (Ch. 28) Biot-Svrt Lw Ampere s Lw Mgnetism in Mtter Mxwell s Equtions Homework #7: due Tues 3/11 t 11 PM (4th problem optionl) Mgnetic

More information

This final is a three hour open book, open notes exam. Do all four problems.

This final is a three hour open book, open notes exam. Do all four problems. Physics 55 Fll 27 Finl Exm Solutions This finl is three hour open book, open notes exm. Do ll four problems. [25 pts] 1. A point electric dipole with dipole moment p is locted in vcuum pointing wy from

More information

September 13 Homework Solutions

September 13 Homework Solutions College of Engineering nd Computer Science Mechnicl Engineering Deprtment Mechnicl Engineering 5A Seminr in Engineering Anlysis Fll Ticket: 5966 Instructor: Lrry Cretto Septemer Homework Solutions. Are

More information

Quadratic Forms. Quadratic Forms

Quadratic Forms. Quadratic Forms Qudrtic Forms Recll the Simon & Blume excerpt from n erlier lecture which sid tht the min tsk of clculus is to pproximte nonliner functions with liner functions. It s ctully more ccurte to sy tht we pproximte

More information

1B40 Practical Skills

1B40 Practical Skills B40 Prcticl Skills Comining uncertinties from severl quntities error propgtion We usully encounter situtions where the result of n experiment is given in terms of two (or more) quntities. We then need

More information

Bases for Vector Spaces

Bases for Vector Spaces Bses for Vector Spces 2-26-25 A set is independent if, roughly speking, there is no redundncy in the set: You cn t uild ny vector in the set s liner comintion of the others A set spns if you cn uild everything

More information

p-adic Egyptian Fractions

p-adic Egyptian Fractions p-adic Egyptin Frctions Contents 1 Introduction 1 2 Trditionl Egyptin Frctions nd Greedy Algorithm 2 3 Set-up 3 4 p-greedy Algorithm 5 5 p-egyptin Trditionl 10 6 Conclusion 1 Introduction An Egyptin frction

More information

ODE: Existence and Uniqueness of a Solution

ODE: Existence and Uniqueness of a Solution Mth 22 Fll 213 Jerry Kzdn ODE: Existence nd Uniqueness of Solution The Fundmentl Theorem of Clculus tells us how to solve the ordinry differentil eqution (ODE) du = f(t) dt with initil condition u() =

More information

A REVIEW OF CALCULUS CONCEPTS FOR JDEP 384H. Thomas Shores Department of Mathematics University of Nebraska Spring 2007

A REVIEW OF CALCULUS CONCEPTS FOR JDEP 384H. Thomas Shores Department of Mathematics University of Nebraska Spring 2007 A REVIEW OF CALCULUS CONCEPTS FOR JDEP 384H Thoms Shores Deprtment of Mthemtics University of Nebrsk Spring 2007 Contents Rtes of Chnge nd Derivtives 1 Dierentils 4 Are nd Integrls 5 Multivrite Clculus

More information

Best Approximation in the 2-norm

Best Approximation in the 2-norm Jim Lmbers MAT 77 Fll Semester 1-11 Lecture 1 Notes These notes correspond to Sections 9. nd 9.3 in the text. Best Approximtion in the -norm Suppose tht we wish to obtin function f n (x) tht is liner combintion

More information

Sufficient condition on noise correlations for scalable quantum computing

Sufficient condition on noise correlations for scalable quantum computing Sufficient condition on noise correltions for sclble quntum computing John Presill, 2 Februry 202 Is quntum computing sclble? The ccurcy threshold theorem for quntum computtion estblishes tht sclbility

More information

I1 = I2 I1 = I2 + I3 I1 + I2 = I3 + I4 I 3

I1 = I2 I1 = I2 + I3 I1 + I2 = I3 + I4 I 3 2 The Prllel Circuit Electric Circuits: Figure 2- elow show ttery nd multiple resistors rrnged in prllel. Ech resistor receives portion of the current from the ttery sed on its resistnce. The split is

More information

Bypassing no-go theorems for consistent interactions in gauge theories

Bypassing no-go theorems for consistent interactions in gauge theories Bypssing no-go theorems for consistent interctions in guge theories Simon Lykhovich Tomsk Stte University Suzdl, 4 June 2014 The tlk is bsed on the rticles D.S. Kprulin, S.L.Lykhovich nd A.A.Shrpov, Consistent

More information

Parse trees, ambiguity, and Chomsky normal form

Parse trees, ambiguity, and Chomsky normal form Prse trees, miguity, nd Chomsky norml form In this lecture we will discuss few importnt notions connected with contextfree grmmrs, including prse trees, miguity, nd specil form for context-free grmmrs

More information

How do we solve these things, especially when they get complicated? How do we know when a system has a solution, and when is it unique?

How do we solve these things, especially when they get complicated? How do we know when a system has a solution, and when is it unique? XII. LINEAR ALGEBRA: SOLVING SYSTEMS OF EQUATIONS Tody we re going to tlk bout solving systems of liner equtions. These re problems tht give couple of equtions with couple of unknowns, like: 6 2 3 7 4

More information

Review of Calculus, cont d

Review of Calculus, cont d Jim Lmbers MAT 460 Fll Semester 2009-10 Lecture 3 Notes These notes correspond to Section 1.1 in the text. Review of Clculus, cont d Riemnn Sums nd the Definite Integrl There re mny cses in which some

More information

Coalgebra, Lecture 15: Equations for Deterministic Automata

Coalgebra, Lecture 15: Equations for Deterministic Automata Colger, Lecture 15: Equtions for Deterministic Automt Julin Slmnc (nd Jurrin Rot) Decemer 19, 2016 In this lecture, we will study the concept of equtions for deterministic utomt. The notes re self contined

More information

221A Lecture Notes WKB Method

221A Lecture Notes WKB Method A Lecture Notes WKB Method Hmilton Jcobi Eqution We strt from the Schrödinger eqution for single prticle in potentil i h t ψ x, t = [ ] h m + V x ψ x, t. We cn rewrite this eqution by using ψ x, t = e

More information

Note 16. Stokes theorem Differential Geometry, 2005

Note 16. Stokes theorem Differential Geometry, 2005 Note 16. Stokes theorem ifferentil Geometry, 2005 Stokes theorem is the centrl result in the theory of integrtion on mnifolds. It gives the reltion between exterior differentition (see Note 14) nd integrtion

More information

Lecture Outline. Dispersion Relation Electromagnetic Wave Polarization 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3c

Lecture Outline. Dispersion Relation Electromagnetic Wave Polarization 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3c Course Instructor Dr. Rymond C. Rumpf Office: A 337 Phone: (915) 747 6958 E Mil: rcrumpf@utep.edu EE 4347 Applied Electromgnetics Topic 3c Wve Dispersion & Polriztion Wve Dispersion These notes & Polriztion

More information

LECTURE 1. Introduction. 1. Rough Classiæcation of Partial Diæerential Equations

LECTURE 1. Introduction. 1. Rough Classiæcation of Partial Diæerential Equations LECTURE 1 Introduction 1. Rough Clssiction of Prtil Dierentil Equtions A prtil dierentil eqution is eqution relting function of n vribles x 1 ;::: ;x n, its prtil derivtives, nd the coordintes x =èx 1

More information

Special Relativity solved examples using an Electrical Analog Circuit

Special Relativity solved examples using an Electrical Analog Circuit 1-1-15 Specil Reltivity solved exmples using n Electricl Anlog Circuit Mourici Shchter mourici@gmil.com mourici@wll.co.il ISRAE, HOON 54-54855 Introduction In this pper, I develop simple nlog electricl

More information

Quantum Mechanics Qualifying Exam - August 2016 Notes and Instructions

Quantum Mechanics Qualifying Exam - August 2016 Notes and Instructions Quntum Mechnics Qulifying Exm - August 016 Notes nd Instructions There re 6 problems. Attempt them ll s prtil credit will be given. Write on only one side of the pper for your solutions. Write your lis

More information

Fierz transformations

Fierz transformations Fierz trnsformtions Fierz identities re often useful in quntum field theory clcultions. They re connected to reordering of field opertors in contct four-prticle interction. The bsic tsk is: given four

More information

9.4. The Vector Product. Introduction. Prerequisites. Learning Outcomes

9.4. The Vector Product. Introduction. Prerequisites. Learning Outcomes The Vector Product 9.4 Introduction In this section we descrie how to find the vector product of two vectors. Like the sclr product its definition my seem strnge when first met ut the definition is chosen

More information

Week 10: Line Integrals

Week 10: Line Integrals Week 10: Line Integrls Introduction In this finl week we return to prmetrised curves nd consider integrtion long such curves. We lredy sw this in Week 2 when we integrted long curve to find its length.

More information

1.9 C 2 inner variations

1.9 C 2 inner variations 46 CHAPTER 1. INDIRECT METHODS 1.9 C 2 inner vritions So fr, we hve restricted ttention to liner vritions. These re vritions of the form vx; ǫ = ux + ǫφx where φ is in some liner perturbtion clss P, for

More information

MAS 4156 Lecture Notes Differential Forms

MAS 4156 Lecture Notes Differential Forms MAS 4156 Lecture Notes Differentil Forms Definitions Differentil forms re objects tht re defined on mnifolds. For this clss, the only mnifold we will put forms on is R 3. The full definition is: Definition:

More information

Conducting Ellipsoid and Circular Disk

Conducting Ellipsoid and Circular Disk 1 Problem Conducting Ellipsoid nd Circulr Disk Kirk T. McDonld Joseph Henry Lbortories, Princeton University, Princeton, NJ 08544 (September 1, 00) Show tht the surfce chrge density σ on conducting ellipsoid,

More information

63. Representation of functions as power series Consider a power series. ( 1) n x 2n for all 1 < x < 1

63. Representation of functions as power series Consider a power series. ( 1) n x 2n for all 1 < x < 1 3 9. SEQUENCES AND SERIES 63. Representtion of functions s power series Consider power series x 2 + x 4 x 6 + x 8 + = ( ) n x 2n It is geometric series with q = x 2 nd therefore it converges for ll q =

More information

A5682: Introduction to Cosmology Course Notes. 4. Cosmic Dynamics: The Friedmann Equation. = GM s

A5682: Introduction to Cosmology Course Notes. 4. Cosmic Dynamics: The Friedmann Equation. = GM s 4. Cosmic Dynmics: The Friedmnn Eqution Reding: Chpter 4 Newtonin Derivtion of the Friedmnn Eqution Consider n isolted sphere of rdius R s nd mss M s, in uniform, isotropic expnsion (Hubble flow). The

More information

Summary of equations chapters 7. To make current flow you have to push on the charges. For most materials:

Summary of equations chapters 7. To make current flow you have to push on the charges. For most materials: Summry of equtions chpters 7. To mke current flow you hve to push on the chrges. For most mterils: J E E [] The resistivity is prmeter tht vries more thn 4 orders of mgnitude between silver (.6E-8 Ohm.m)

More information

DEFINITION The inner product of two functions f 1 and f 2 on an interval [a, b] is the number. ( f 1, f 2 ) b DEFINITION 11.1.

DEFINITION The inner product of two functions f 1 and f 2 on an interval [a, b] is the number. ( f 1, f 2 ) b DEFINITION 11.1. 398 CHAPTER 11 ORTHOGONAL FUNCTIONS AND FOURIER SERIES 11.1 ORTHOGONAL FUNCTIONS REVIEW MATERIAL The notions of generlized vectors nd vector spces cn e found in ny liner lger text. INTRODUCTION The concepts

More information

arxiv:gr-qc/ v1 14 Mar 2000

arxiv:gr-qc/ v1 14 Mar 2000 The binry blck-hole dynmics t the third post-newtonin order in the orbitl motion Piotr Jrnowski Institute of Theoreticl Physics, University of Bi lystok, Lipow 1, 15-2 Bi lystok, Polnd Gerhrd Schäfer Theoretisch-Physiklisches

More information

Chapter 4: Techniques of Circuit Analysis. Chapter 4: Techniques of Circuit Analysis

Chapter 4: Techniques of Circuit Analysis. Chapter 4: Techniques of Circuit Analysis Chpter 4: Techniques of Circuit Anlysis Terminology Node-Voltge Method Introduction Dependent Sources Specil Cses Mesh-Current Method Introduction Dependent Sources Specil Cses Comprison of Methods Source

More information

ECON 331 Lecture Notes: Ch 4 and Ch 5

ECON 331 Lecture Notes: Ch 4 and Ch 5 Mtrix Algebr ECON 33 Lecture Notes: Ch 4 nd Ch 5. Gives us shorthnd wy of writing lrge system of equtions.. Allows us to test for the existnce of solutions to simultneous systems. 3. Allows us to solve

More information

Polynomials and Division Theory

Polynomials and Division Theory Higher Checklist (Unit ) Higher Checklist (Unit ) Polynomils nd Division Theory Skill Achieved? Know tht polynomil (expression) is of the form: n x + n x n + n x n + + n x + x + 0 where the i R re the

More information

Physics 3323, Fall 2016 Problem Set 7 due Oct 14, 2016

Physics 3323, Fall 2016 Problem Set 7 due Oct 14, 2016 Physics 333, Fll 16 Problem Set 7 due Oct 14, 16 Reding: Griffiths 4.1 through 4.4.1 1. Electric dipole An electric dipole with p = p ẑ is locted t the origin nd is sitting in n otherwise uniform electric

More information

Review of basic calculus

Review of basic calculus Review of bsic clculus This brief review reclls some of the most importnt concepts, definitions, nd theorems from bsic clculus. It is not intended to tech bsic clculus from scrtch. If ny of the items below

More information

Math 1B, lecture 4: Error bounds for numerical methods

Math 1B, lecture 4: Error bounds for numerical methods Mth B, lecture 4: Error bounds for numericl methods Nthn Pflueger 4 September 0 Introduction The five numericl methods descried in the previous lecture ll operte by the sme principle: they pproximte the

More information

Bernoulli Numbers Jeff Morton

Bernoulli Numbers Jeff Morton Bernoulli Numbers Jeff Morton. We re interested in the opertor e t k d k t k, which is to sy k tk. Applying this to some function f E to get e t f d k k tk d k f f + d k k tk dk f, we note tht since f

More information

Lecture 4 Notes, Electromagnetic Theory I Dr. Christopher S. Baird University of Massachusetts Lowell

Lecture 4 Notes, Electromagnetic Theory I Dr. Christopher S. Baird University of Massachusetts Lowell Lecture 4 Notes, Electromgnetic Theory I Dr. Christopher S. Bird University of Msschusetts Lowell 1. Orthogonl Functions nd Expnsions - In the intervl (, ) of the vrile x, set of rel or complex functions

More information

HW3, Math 307. CSUF. Spring 2007.

HW3, Math 307. CSUF. Spring 2007. HW, Mth 7. CSUF. Spring 7. Nsser M. Abbsi Spring 7 Compiled on November 5, 8 t 8:8m public Contents Section.6, problem Section.6, problem Section.6, problem 5 Section.6, problem 7 6 5 Section.6, problem

More information

The Dirichlet Problem in a Two Dimensional Rectangle. Section 13.5

The Dirichlet Problem in a Two Dimensional Rectangle. Section 13.5 The Dirichlet Prolem in Two Dimensionl Rectngle Section 13.5 1 Dirichlet Prolem in Rectngle In these notes we will pply the method of seprtion of vriles to otin solutions to elliptic prolems in rectngle

More information

Module 6: LINEAR TRANSFORMATIONS

Module 6: LINEAR TRANSFORMATIONS Module 6: LINEAR TRANSFORMATIONS. Trnsformtions nd mtrices Trnsformtions re generliztions of functions. A vector x in some set S n is mpped into m nother vector y T( x). A trnsformtion is liner if, for

More information

Chapter 6 Techniques of Integration

Chapter 6 Techniques of Integration MA Techniques of Integrtion Asst.Prof.Dr.Suprnee Liswdi Chpter 6 Techniques of Integrtion Recll: Some importnt integrls tht we hve lernt so fr. Tle of Integrls n+ n d = + C n + e d = e + C ( n ) d = ln

More information

u( t) + K 2 ( ) = 1 t > 0 Analyzing Damped Oscillations Problem (Meador, example 2-18, pp 44-48): Determine the equation of the following graph.

u( t) + K 2 ( ) = 1 t > 0 Analyzing Damped Oscillations Problem (Meador, example 2-18, pp 44-48): Determine the equation of the following graph. nlyzing Dmped Oscilltions Prolem (Medor, exmple 2-18, pp 44-48): Determine the eqution of the following grph. The eqution is ssumed to e of the following form f ( t) = K 1 u( t) + K 2 e!"t sin (#t + $

More information

Chapter 9 Many Electron Atoms

Chapter 9 Many Electron Atoms Chem 356: Introductory Quntum Mechnics Chpter 9 Mny Electron Atoms... 11 MnyElectron Atoms... 11 A: HrtreeFock: Minimize the Energy of Single Slter Determinnt.... 16 HrtreeFock Itertion Scheme... 17 Chpter

More information

SUMMER KNOWHOW STUDY AND LEARNING CENTRE

SUMMER KNOWHOW STUDY AND LEARNING CENTRE SUMMER KNOWHOW STUDY AND LEARNING CENTRE Indices & Logrithms 2 Contents Indices.2 Frctionl Indices.4 Logrithms 6 Exponentil equtions. Simplifying Surds 13 Opertions on Surds..16 Scientific Nottion..18

More information

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1 MATH34032: Green s Functions, Integrl Equtions nd the Clculus of Vritions 1 Section 1 Function spces nd opertors Here we gives some brief detils nd definitions, prticulrly relting to opertors. For further

More information

Improper Integrals, and Differential Equations

Improper Integrals, and Differential Equations Improper Integrls, nd Differentil Equtions October 22, 204 5.3 Improper Integrls Previously, we discussed how integrls correspond to res. More specificlly, we sid tht for function f(x), the region creted

More information

Method of Localisation and Controlled Ejection of Swarms of Likely Charged Particles

Method of Localisation and Controlled Ejection of Swarms of Likely Charged Particles Method of Loclistion nd Controlled Ejection of Swrms of Likely Chrged Prticles I. N. Tukev July 3, 17 Astrct This work considers Coulom forces cting on chrged point prticle locted etween the two coxil,

More information

State space systems analysis (continued) Stability. A. Definitions A system is said to be Asymptotically Stable (AS) when it satisfies

State space systems analysis (continued) Stability. A. Definitions A system is said to be Asymptotically Stable (AS) when it satisfies Stte spce systems nlysis (continued) Stbility A. Definitions A system is sid to be Asymptoticlly Stble (AS) when it stisfies ut () = 0, t > 0 lim xt () 0. t A system is AS if nd only if the impulse response

More information

Lecture 3. In this lecture, we will discuss algorithms for solving systems of linear equations.

Lecture 3. In this lecture, we will discuss algorithms for solving systems of linear equations. Lecture 3 3 Solving liner equtions In this lecture we will discuss lgorithms for solving systems of liner equtions Multiplictive identity Let us restrict ourselves to considering squre mtrices since one

More information

Linear Systems with Constant Coefficients

Linear Systems with Constant Coefficients Liner Systems with Constnt Coefficients 4-3-05 Here is system of n differentil equtions in n unknowns: x x + + n x n, x x + + n x n, x n n x + + nn x n This is constnt coefficient liner homogeneous system

More information

Problems for HW X. C. Gwinn. November 30, 2009

Problems for HW X. C. Gwinn. November 30, 2009 Problems for HW X C. Gwinn November 30, 2009 These problems will not be grded. 1 HWX Problem 1 Suppose thn n object is composed of liner dielectric mteril, with constnt reltive permittivity ɛ r. The object

More information

13: Diffusion in 2 Energy Groups

13: Diffusion in 2 Energy Groups 3: Diffusion in Energy Groups B. Rouben McMster University Course EP 4D3/6D3 Nucler Rector Anlysis (Rector Physics) 5 Sept.-Dec. 5 September Contents We study the diffusion eqution in two energy groups

More information

Resistive Network Analysis

Resistive Network Analysis C H A P T E R 3 Resistive Network Anlysis his chpter will illustrte the fundmentl techniques for the nlysis of resistive circuits. The methods introduced re sed on the circuit lws presented in Chpter 2:

More information

2.4 Linear Inequalities and Interval Notation

2.4 Linear Inequalities and Interval Notation .4 Liner Inequlities nd Intervl Nottion We wnt to solve equtions tht hve n inequlity symol insted of n equl sign. There re four inequlity symols tht we will look t: Less thn , Less thn or

More information

Consequently, the temperature must be the same at each point in the cross section at x. Let:

Consequently, the temperature must be the same at each point in the cross section at x. Let: HW 2 Comments: L1-3. Derive the het eqution for n inhomogeneous rod where the therml coefficients used in the derivtion of the het eqution for homogeneous rod now become functions of position x in the

More information

Metric Compatibility Condition And Tetrad Postulate

Metric Compatibility Condition And Tetrad Postulate Chapter 8 Metric Compatibility Condition And Tetrad Postulate by Myron W. Evans, Alpha Foundation s Institutute for Advance Study (AIAS). (emyrone@oal.com, www.aias.us, www.atomicprecision.com) Abstract

More information

( dg. ) 2 dt. + dt. dt j + dh. + dt. r(t) dt. Comparing this equation with the one listed above for the length of see that

( dg. ) 2 dt. + dt. dt j + dh. + dt. r(t) dt. Comparing this equation with the one listed above for the length of see that Arc Length of Curves in Three Dimensionl Spce If the vector function r(t) f(t) i + g(t) j + h(t) k trces out the curve C s t vries, we cn mesure distnces long C using formul nerly identicl to one tht we

More information

Conservation Law. Chapter Goal. 5.2 Theory

Conservation Law. Chapter Goal. 5.2 Theory Chpter 5 Conservtion Lw 5.1 Gol Our long term gol is to understnd how mny mthemticl models re derived. We study how certin quntity chnges with time in given region (sptil domin). We first derive the very

More information

CHM Physical Chemistry I Chapter 1 - Supplementary Material

CHM Physical Chemistry I Chapter 1 - Supplementary Material CHM 3410 - Physicl Chemistry I Chpter 1 - Supplementry Mteril For review of some bsic concepts in mth, see Atkins "Mthemticl Bckground 1 (pp 59-6), nd "Mthemticl Bckground " (pp 109-111). 1. Derivtion

More information

Today in Physics 122: work, energy and potential in electrostatics

Today in Physics 122: work, energy and potential in electrostatics Tody in Physics 1: work, energy nd potentil in electrosttics Leftovers Perfect conductors Fields from chrges distriuted on perfect conductors Guss s lw for grvity Work nd energy Electrosttic potentil energy,

More information

A matrix is a set of numbers or symbols arranged in a square or rectangular array of m rows and n columns as

A matrix is a set of numbers or symbols arranged in a square or rectangular array of m rows and n columns as RMI University ENDIX MRIX GEBR INRDUCIN Mtrix lgebr is powerful mthemticl tool, which is extremely useful in modern computtionl techniques pplicble to sptil informtion science. It is neither new nor difficult,

More information

Designing finite automata II

Designing finite automata II Designing finite utomt II Prolem: Design DFA A such tht L(A) consists of ll strings of nd which re of length 3n, for n = 0, 1, 2, (1) Determine wht to rememer out the input string Assign stte to ech of

More information

MA Handout 2: Notation and Background Concepts from Analysis

MA Handout 2: Notation and Background Concepts from Analysis MA350059 Hndout 2: Nottion nd Bckground Concepts from Anlysis This hndout summrises some nottion we will use nd lso gives recp of some concepts from other units (MA20023: PDEs nd CM, MA20218: Anlysis 2A,

More information

The Algebra (al-jabr) of Matrices

The Algebra (al-jabr) of Matrices Section : Mtri lgebr nd Clculus Wshkewicz College of Engineering he lgebr (l-jbr) of Mtrices lgebr s brnch of mthemtics is much broder thn elementry lgebr ll of us studied in our high school dys. In sense

More information

MA123, Chapter 10: Formulas for integrals: integrals, antiderivatives, and the Fundamental Theorem of Calculus (pp.

MA123, Chapter 10: Formulas for integrals: integrals, antiderivatives, and the Fundamental Theorem of Calculus (pp. MA123, Chpter 1: Formuls for integrls: integrls, ntiderivtives, nd the Fundmentl Theorem of Clculus (pp. 27-233, Gootmn) Chpter Gols: Assignments: Understnd the sttement of the Fundmentl Theorem of Clculus.

More information

308K. 1 Section 3.2. Zelaya Eufemia. 1. Example 1: Multiplication of Matrices: X Y Z R S R S X Y Z. By associativity we have to choices:

308K. 1 Section 3.2. Zelaya Eufemia. 1. Example 1: Multiplication of Matrices: X Y Z R S R S X Y Z. By associativity we have to choices: 8K Zely Eufemi Section 2 Exmple : Multipliction of Mtrices: X Y Z T c e d f 2 R S X Y Z 2 c e d f 2 R S 2 By ssocitivity we hve to choices: OR: X Y Z R S cr ds er fs X cy ez X dy fz 2 R S 2 Suggestion

More information

Chapter 5. , r = r 1 r 2 (1) µ = m 1 m 2. r, r 2 = R µ m 2. R(m 1 + m 2 ) + m 2 r = r 1. m 2. r = r 1. R + µ m 1

Chapter 5. , r = r 1 r 2 (1) µ = m 1 m 2. r, r 2 = R µ m 2. R(m 1 + m 2 ) + m 2 r = r 1. m 2. r = r 1. R + µ m 1 Tor Kjellsson Stockholm University Chpter 5 5. Strting with the following informtion: R = m r + m r m + m, r = r r we wnt to derive: µ = m m m + m r = R + µ m r, r = R µ m r 3 = µ m R + r, = µ m R r. 4

More information

NUMERICAL INTEGRATION. The inverse process to differentiation in calculus is integration. Mathematically, integration is represented by.

NUMERICAL INTEGRATION. The inverse process to differentiation in calculus is integration. Mathematically, integration is represented by. NUMERICAL INTEGRATION 1 Introduction The inverse process to differentition in clculus is integrtion. Mthemticlly, integrtion is represented by f(x) dx which stnds for the integrl of the function f(x) with

More information