The Equivalence of Mass and Energy: Blackbody Radiation in Uniform Translational Motion
|
|
- Milo Norris
- 6 years ago
- Views:
Transcription
1 The Africn Review of Physics (2015) 10: The Equivlence of Mss nd Energy: Blckbody Rdition in Uniform Trnsltionl Motion Rndy Wyne * Lbortory of Nturl Philosophy, Section of Plnt Biology, School of Integrtivee Plnt Science, Cornell University, Ithc, New York 1485, USA Uniform trnsltionl motion cusess hollow cylinder filled with blckbody rdition to gin n pprent inertil mss. Bsed on n electrodynmic nlysis, Hsenöhrl determined tht the reltionship between the velocity-dependent pprent inertil mss () nd the energy () of rdition ws given by. The reltionship between mss nd energy derived dynmiclly by Hsenöhrl differs from derived kinemticlly by Einstein. Here I use the reltionship between the energy nd liner momentum ( ) of photon ( ) nd the dynmic effects produced in Eucliden spce nd Newtonin time by the Doppler effect expnded to second order to show tht Einstein s eqution for the mss-energy reltion is the correct one for rdition-filled cylinder in uniform motion. The increse in liner momentum cused by the velocity-induced Doppler effect expnded to the second order results in n increse in the internl energy density of the rdition. The velocity-dependent increse in the internl energy results from both n increse in temperture nd n increse of entropy consistent with Plnck s blckbody rdition lw. The velocity-induced increse in the internl energy density is equivlent to velocity-dependent increse in the pprent inertil mss of the rdition within the cylinder. 1. Introduction As result of kinemticl nlysis, Einstein [1,2,3] derived the following eqution to describe the reltionship between the energy () nd inerti () of light: (1) By contrst, Hsenöhrl [4,5,6] took dynmic pproch to determine the reltionship between the energy nd inerti of light, by considering the work done by the nisotropic rdition pressure [7] inside uniformly trnslting cylinder (Fig. 1). Hsenöhl s eqution describing the reltionship between the energy nd inerti of blckbody rdition in uniformly moving cylinder differs from Eqn. (1) by n lgebric prefctor: The gol of this pper is to show tht Eqn. (1) is the correct eqution for describing the reltionship between the energy nd inerti of rdition for uniformly trnslting blckbody rdition-filled cylinder lthough the ssumption of reltive time used by Einstein to derive Eqn. (1) is unnecessry. * row1@cornell.edu (2) Fig.1: Hsenöhrl s gednkenexperiment. A cylinder with mtte blck nd dibtic wlls nd constnt nd invrint volume contining blckbody rdition chrcterized by bsolute temperture T moves through vcuum t bsolute zero. According to the Third Lw of Thermodynmics, bsolute zero is unttinble, so in ny rel experiment, the cylinder will hve to move through vcuum with finite temperture, which itself will result in n optomechnicl friction due to the Doppler effect expnded to the second order nd the need for dditionl pplied potentil energy to move the cylinder t given uniform velocity for given time. The orienttion of reltive to the x xis is shown, the orienttion of is perpendiculr to the x xis nd prllel to the end wlls. The length () of the cylinder is equl to twice the rdius () of n end wll so tht 2 2. With this geometry, one-hlf of the photons intercting with wll interct with n end wll. The time it tkes photon to propgte from end wll to end wll is.
2 The Africn Review of Physics (2015) 10: Results nd Discussion The derivtion I give here is bsed on the postultes of Eucliden spce, Newtonin time, nd the Doppler effect expnded to second order [8]. I ssume tht the wlls of the cylinder re dibtic, tht the volume is constnt nd invrint, tht the thermodynmic system is closed, nd tht energy nd liner momentum re conserved. I discuss sitution where the wlls re mtte blck nd re perfect bsorbers nd emitters. I consider the possibility tht the portion of the potentil energy pplied to the moving cylinder tht is not trnsformed into kinetic energy is trnsformed t the moving mtte-blck wlls into thermodynmic potentil energy such s the internl energy (). According to the work-energy theorem, the pplied potentil energy ( ) needed to move n object qusi-stticlly from stte of rest to nother stte with higher uniform velocity () for time intervl () is given by the following formul: $!"# (3) $ & Where,!"# is the verge force pplied over time intervl. If one were to move blckbody rditioncontining cylinder t constnt velocity through vcuum t bsolute zero where there is no externl mteril - nor rdition-friction, the rdition inside the cylinder would still dd velocity-dependent pprent inertil mss to the cylinder. This is becuse the rdition inside the cylinder tht strikes the bck wll would be blue-shifted while the blckbody rdition inside the cylinder tht strikes the front wll would be red-shifted (Fig. 1). The Doppler-induced frequency shift expnded to second order of ech photon tht mkes up the blckbody rdition due to reltive motion is given by the following eqution [8]: ' ( ' ) * -./01, 2 3, 4-./ (4) Where, ' ) is the frequency of the photon t the pek of Plnck s blckbody rdition curve tht describes the blckbody rdition in the cvity t rest (7 8), ' ( is the frequency of the photon t the pek of Plnck s blckbody rdition curve tht describes the blckbody rdition in the cvity when the cylinder is trveling t reltive velocity 7, nd θ is the ngle subtending the bsorbed or emitted rdition nd the velocity vector 7:. The Doppleriztion of the rdition within the cylinder will lso result in chnge in the energy of ech photon: h' ( h' ) * -./01, 2 3, 4-./ (5) When the cylinder is t rest, the energy of photon ( ) ) with pek frequency (' ) ) striking norml to either end wll is given by: ) = h' ) (6) However, when the cylinder is moving t uniform velocity over given time, the energy of photon t the pek of the blckbody rdition curve tht is propgting norml to the end wlls will decrese s result of being bsorbed nd emitted by the front end wll (θ 05 nd increse s result of being bsorbed nd emitted by the bck end wll (θ 5. As result of the second order effects, the energy increse t the bck wll will be greter thn the energy decrese t the front wll. Consequently, s result of the uniform trnsltionl movement, the energy (h' ( ) of the photons bsorbed nd emitted by both wlls will increse over time. As result of the two bsorptions nd the two emissions tht tke plce t the front nd bck wlls during, the velocitydependent energy of the photon t the pek of the blck body rdition curve is given by: 4=)>?5( 2h' ) *, - 2 2h' ) * h' ) * 2 6 h' ) * B (7) Since the photons in the blckbody rdition cn strike the end wlls t ny ngle () from 0 to ± D nd ny ngle () from 0 to ±D, the energy trnsfer depends on the cosines of the ngles of incidence nd the ngles of emission reltive to the norml: H ( 4=)>?5( IH cos J 4KLMNOP5- H IH cos (8)
3 The Africn Review of Physics (2015) 10: Thus the verge energy trnsfer per photon t the pek of the blckbody rdition curve t ny ngle is one-fourth of the energy trnsfer of photon t the pek of the blckbody rdition curve tht strikes the end wll perpendiculr to the surfce. Consequently, when the cylinder is in uniform motion, the verge photon with frequency t the pek of the blckbody rdition curve will hve its energy incresed in time by: ( h' ( h' ) * 2 6 (9) As result of the Doppler shift expnded to second order, fter given time intervl, the energy of the photons intercting with the mtte blck end wlls of the cylinder moving t constnt velocity will contribute to blckbody distribution of rdition chrcterized by pek with greter frequency nd thus higher temperture. The firstorder Doppler effect lone cnnot ccount for the nonliner reltionship between pplied energy nd kinetic energy becuse the first-order Doppler shifts t the end wll t the front of the cylinder nd the end wll t the bck of the cylinder cncel ech other nd the verge frequency of the photons in the cvity does not chnge [9]. However, the expnsion of the Doppler effect to second order gives the symmetry necessry to convert motion into internl energy. As result of the Doppler shift expnded to second order, s 7, the energy of the verge photon with frequency t the pek of the blckbody rdition curve pproches infinity. Since this energy increses t the expense of the conversion of the pplied potentil energy into the kinetic energy of the cylinder, the incresed energy of the rdition cn be considered to be the equivlent of velocity-dependent increse in the pprent inertil mss of the rdition. Since the pprent inertil mss of the blckbody rdition increses s result of the uniform movement of the cylinder through the vcuum, the pplied force (!"# ) needed to mintin constnt velocity () cnnot be constnt but must increse over the time intervl consistent with Eqn. (3). Thus the pprent increse in the inertil mss is mnifesttion of the fct tht the pplied potentil energy is trnsformed not only into the kinetic energy of the rdition-filled cylinder but lso into the internl energy of the blckbody rdition or photon gs itself. A complete conversion of the pplied potentil energy into the kinetic energy of the cylinder would only hppen when the inside of the cylinder is t bsolute zero nd there would not be ny photons within the cvity [10,11]. As bsolute zero is unttinble, this is limiting condition wht would not hppen in nture. The temperture (R) of the photon gs within cylinder moving t constnt velocity is relted to the pek frequency of the rdition in the cylinder t rest nd on the velocity of the cylinder. It is obtined by tking Eqn. (9) into considertion in order to crete the reltivistic version of Wien s displcement lw given below: ( h' ( h' ) * YR (10) Where, Y is Boltzmnn s constnt. I ssume tht while the pek frequency nd pek energy chnge with velocity, the spectrl distribution, which is described by Plnck s blckbody rdition lw, remins invrint. The increse in the temperture (R) of the blckbody rdition tht is relted to the increse in the energy ( ( ) of the photons t the pek of the blckbody rdition curve resulting from the Doppler shift is obtined by differentiting Wien s displcement lw: ( Y R (11) Plnck s blckbody rdition lw reltes the spectrl distribution of energy to the internl energy. The internl energy () of the blckbody rdition is relted to the temperture of the blckbody rdition by the Stefn-Boltzmnn lw: ZD[ \ ] ^_`` br (12) The increse in the internl energy of the blckbody rdition tht is due to the velocityinduced increse in the temperture of the blckbody rdition is given by differentiting Eqn. (12): Where, ZD [ \ ] ^_`` d D[ \ ] ^_`` br R (13) is the product of the Stefn- Boltzmnn (c) constnt nd one-fourth the speed of light (d e = J m -3 K -4 ). Thus prt of the pplied potentil energy used in moving the
4 The Africn Review of Physics (2015) 10: cylinder through vcuum cuses n increse in the internl energy of the blckbody rdition in the cylinder consistent with the conservtion of energy. Thus the mount of potentil energy needed to move the cylinder t given constnt velocity is greter thn the potentil energy predicted to move the cylinder if the internl energy of the rdition did not chnge with movement, nd the rdition did not cquire n pprent inertil mss. In order to formlly relte the increse in the potentil energy needed to mintin constnt velocity to the pprent inertil mss, we hve to consider the liner momentum of the photons tht mke up the blckbody rdition. The liner momentum ( ) of photon is given by [12]: J _f (14) When the cylinder is t rest, ccording to Eqn. (8), the liner momentum trnsferred by the verge photon with pek frequency (' ) ) moving in ny direction when they re bsorbed or emitted by the end wll is given by: ) = _f L (15) When the cylinder is in uniform motion, the verge photon with the pek frequency (7 ( ) trveling in ny direction tht is bsorbed nd emitted by the front end wll nd then bsorbed nd emitted by the bck end wll, will hve its liner momentum incresed by: ( 2 _f L *, _fl 2 * B _f L * 6 _fl * 6 (16) 2 2 After given durtion of time, the liner momentum of the photons trveling in ny direction in the cylinder moving t uniform velocity would increse. By definition, the liner momentum of the photon with the new pek frequency is equl to the product of its mss ( ( ) nd velocity: ( _f g * 2 6 ( 7 (17) Since the velocity of the photons in the cvity is constnt nd equl to, the totl differentil of the liner momentum is given by: ( ( (18) As result of the Doppler effect expnded to second order, the rdition produces n increse in liner momentum in given durtion of time, on the cylinder moving t constnt velocity. The increse in liner momentum results in n increse in the pprent inertil mss () of the photon with pek frequency moving t velocity c in ny direction within the cylinder ccording to the following formul: ( _ ' ) * 2 6 _ ' ) ( (19) The blckbody rdition within the cylinder in uniform trnsltionl motion provides liner momentum tht increses with velocity nd time. Consequently, the pplied force needed to mintin constnt velocity during tht durtion of time cnnot remin constnt but must lso increse to compenste for the incresed liner momentum. Interestingly, while he ws working on the quntum nture of rdition, Einstein [12,13] relized tht the momentum of rdition would exert rdition friction on moving body, but ws too engged in the Generl Theory of Reltivity to re-interpret the electrodynmics of moving bodies in terms of dynmics. The pprent increse in the inertil mss of photon is obtined by dividing ll terms in Eqn. (19) by : - _ ' ) * After substitution of ( with J - we get: J - _ ' ) * After rerrngement, we get: ( h' ) * 2 16 ( (20) ccording to [12], 2 16 ( (21) 2 16 ( (22)
5 The Africn Review of Physics (2015) 10: which is reminiscent of the eqution given by Einstein [1]. The increse in the pprent inertil msses of the photons ( ( ) t the pek of the spectrl distribution given by Plnck s rdition lw is relted to the totl increse in the pprent inertil mss () of the blckbody rdition in the cylinder. The time needed for the photons within the cylinder to go from n initil stte whose blckbody rdition is described by pek t one frequency to finl stte whose blckbody rdition is described by pek t higher frequency my depend on the detils of the force nd the dimensions of the cylinder. To simplify mtters, I ssume tht the durtion of time needed for the blckbody rdition to rech ech stte is constnt nd the force is not constnt. Eqn. (22) describes how chnge in the uniform velocity of rdition-filled cylinder is trnsformed into chnge in the energy nd inerti of the rdition inside the cylinder. The chnge in the energy nd inerti of rdition results from the Doppler effect expnded to second order nd the reltionship between energy nd inerti depends on the defined reltionship between the energy nd momentum of rdition ( (. Below I will use Plnck s blckbody rdition lw, lw tht I contend holds in ny inertil frme, to relte the spectrl distribution of rdition t ny velocity to the internl energy of the rdition. In cylinder contining photon gs t constnt volume, the pplied potentil energy needed to move the cylinder t constnt velocity from stte 1 to stte 2 is distributed between the increse in the kinetic energy of the cylinder itself nd the energy equivlent of the pprent inertil msses of ll the photons in the photon gs. Bsed on Eqn. (22), I consider the increse in the energy equivlent of the pprent inertil msses to be equl to the increse in the internl energy () of the photon gs: (23) Since the internl energy of photon gs is relted thermodynmiclly to both therml energy nd pressure-volume energy [14,15], we cn try to chrcterize further the increse in the energy of rdition tht occurs when closed thermodynmic system is moved t constnt velocity. In closed thermodynmic system with constnt volume moving t constnt velocity, the velocity-dependent increse in internl energy () of the photon gs cn be considered thermodynmiclly s velocity-dependent increse in therml energy (i) nd pressure-volume energy (b): i b (24) However, b vnishes since the volume is constnt by definition. The complete differentil of the therml energy (i) is given by the following eqution: i Rj jr (25) Where, R is the bsolute temperture nd j is the entropy of rdition in the cvity with constnt volume (b). Note tht the increse in therml energy in the cylinder with dibtic wlls does not result from het trnsfer from therml reservoir, s it does in trditionl thermodynmic systems [16], but from the dynmic effects of the velocityinduced Doppler effect expnded to second order. The velocity-induced Doppler effect cn result in n increse in temperture nd/or n increse of entropy. The increse in the therml energy of the photon gs tht hppens in the bsence of het flow my help in the kinemtic understnding of the contentious nd contrdictory field of reltivistic thermodynmics [17]. If the wlls of the cvity re mtte blck, consistent with Plnck s blckbody rdition lw, the photon number is not conserved nd the increse in internl energy due to the uniform trnsltionl motion for given durtion will result in n increse in the temperture (due to n increse in the frequency of the photons t the pek of the blckbody rdition curve) nd n increse in entropy (due to n increse in the number of photons). Neither of these quntities lone re considered here to be invrints. The bility of the blckbody rdition to tke up therml energy is given by the specific het cpcity t constnt volume (k l ) tht is obtined by differentiting the internl energy t constnt volume with respect to temperture: k l m n o p l D[ \ ] ^_`` VR (26) The spectrl number density (r) of photons, ech with given frequency, in the cvity t given temperture (R), is obtined by dividing the internl energy (), given by Plnck s blckbody rdition lw, by h'. Plnck s [18] blckbody rdition lw gives the spectrl energy density:
6 The Africn Review of Physics (2015) 10: s4',r5' n l 4',R5' ZDf ` _f u- vw, ' (27) The spectrl number density or the number of photons with given frequency is given by: r4',r5' x4f,o5 _f ' ZD_`f u- _``vw, ' (28) The totl number density ( y ) of photons within l the cylinder vries with the velocity of the cylinder in the sme wy tht the totl number density vries with temperture. The totl number density of photons comprising blckbody distribution of rdition chrcterized by given temperture t constnt volume is obtined by integrting Eqn. (28): y l z ZD\`o` r4',r5' { _`` ZD\`o` m u vw p u} z vw _`` { u- vw, z _`f { u- \`o`vw, ' (29) The integrl in Eqn. (29) cn be solved by letting ~ _( \o nd ~ _ \o ': y z r4',r5' l { z {, ZD\`o` z 45 _`` {, (30) Since , the totl number density of photons in cvity of temperture R is: y l 60.42m\o _ p 60.42m \ _ p R ƒ R (31) Differentiting Eqn. (31), we get the chnge in the totl number density of photons with chnge of temperture t constnt volume: l m\ _ p R R (32) The totl entropy of photons within the cylinder vries with the velocity of the cylinder in the sme wy tht the totl entropy vries with temperture. The increse of entropy of the photon gs with temperture R is obtined by dividing the internl energy differentil given in Eqn. (13) by the temperture: j n o D[ \ ] ^_`` br R (33) Since j vnishes t bsolute zero where R lso vnishes, the bsolute entropy j [19] of the photon gs t ny temperture R is obtined by integrting Eqn. (33): j D[ \ ] ^_`` VR (34) The entropy density of photons within the cylinder vries with the velocity of the cylinder in the sme wy tht the entropy density vries with temperture. The vlue of the entropy obtined from Eqn. (34) cn be used to find the entropy density of the blckbody rdition in the cylinder chrcterized by temperture R: D[ \ m \o l ^ _ p (35) By tking the rtio of Eqn. (35) nd Eqn. (31), the entropy per photon in the blckbody rdition is found to be constnt independent of velocity nd temperture, nd is given by: l D[ \ m \o y yl ^ _ p {.m vw p` D[\ ^ u2 {. 3.60Y (36) How the entropy of photon reltes to the degrees of freedom of photon is mystery. If entropy is defined by the degrees of freedom, with ech degree of freedom contributing to the entropy, then the entropy of photon is close to tht of ditomic gs molecule with trnsltionl, rottionl nd vibrtionl degrees of freedom [20]. For ditomic gs molecule, the three trnsltionl degrees of freedom contribute Y, the two rottionl degrees of freedom contribute Y nd the two vibrtionl degrees of freedom contribute Y for totl of 3.5Y. If photon were point prticle with three degrees of freedom for trnsltion nd one degree of freedom for polriztion, the entropy would be close to 2.5Y. Quntum mechniclly speking [21], entropy is relted to the number of microsttes (ˆ), which for the photon would be 36.6, since j Y lnˆ. The entropy of photon given in Eqn. (35) is more consistent with the model of n extended nd dynmic photon consisting of trnsltionl nd rottionl oscilltors [22-25], nd less consistent with the model of kinemtic photon being mthemticl point with integer spin. The verge internl energy of the photons ( ) composing the photon gs in the cylinder is relted
7 The Africn Review of Physics (2015) 10: to the velocity of the cylinder in the sme wy tht the verge internl energy of the photons is relted to the temperture. The verge internl energy of the photons in the blckbody rdition is given by the rtio of the internl energy density given in Eqn. (12) nd the totl number of photons per unit volume given in Eqn. (31): nl ZD[ yl ^ {. YR 2.70 YR (37) Consistent with the shpe of the curve tht describes blckbody rdition, the vlue for the verge internl energy of the photon is slightly lower thn the vlue of the internl energy of the photon t the pek of the blckbody rdition curve given by the Wien displcement lw: 4\ YR (38) When the wlls of the cvity re mtte blck, both the energy of the photon t the pek of the curve tht chrcterizes the blckbody rdition nd the number of photons t the pek of the curve increses s result of the velocity-induced Doppler effect (Fig. 2). This is best chrcterized by the velocity-dependent temperture of the photon gs inside the cylinder. The velocityinduced temperture increse hs greter effect on photon number thn on the energy of the photon t the pek of the blckbody rdition curve since the energy of the photon t the pek of the blckbody rdition curve is directly proportionl to temperture while the number of photons in the blckbody rdition is proportionl to the third power of temperture. The velocity-induced Doppler effect expnded to the second order results in n increse in the internl energy density, the temperture, the entropy density, nd the pprent inertil mss (Tble 1). When the wlls of the cvity re not blck, but re perfectly speculr reflecting, uniform trnsltionl motion will cuse n increse in the energy of the photon t the pek of the curve tht chrcterizes the rdition but there will be neither chnge in photon number ( 0) nor entropy (j 0). Consequently, the rdition in the cvity will no longer be distributed ccording to Plnck s blckbody rdition lw nd the nlysis given here will not hold. Nevertheless, whether the wlls of the cvity re mtte blck or perfectly speculr reflecting, the velocity-induced chnge in the pek of rdition would be irreversible nd the potentil energy irretrievble becuse moving the blckbody rdition-filled cylinder t uniform velocity in the opposite direction would not cuse decrese in internl energy but further increse. Indeed I hve shown tht the interction of Doppler-shifted photons with moving bodies is the fundmentl nd inevitble cuse of irreversibility [10]. Spectrl Energy Density, J m -3 3E E-18 2E E-18 1E-18 5E E00 Frequency, s E14 Fig.2: The velocity-induced chnge in the distribution of blckbody rdition in cylinder with mtte blck nd dibtic wlls nd constnt nd invrint volume trnslting uniformly t vrious speeds (0, 0.5c, nd 0.9c). Note tht the spectrl energy density (in J/m 3 ) t given velocity multiplied by the squre of the speed of light gives the spectrl mss density (in kg/m 3 ) t given velocity. Likewise the integrl of the spectrl energy density (in J/m 3 ) t given velocity multiplied by the squre of the speed of light gives the totl mss density (in kg/m 3 ) of the enclosed rdition t given velocity. As result of the increse in the internl energy () of the photon gs in the moving cylinder described nd explined by the velocity-induced Doppler effect expnded to second order, the blckbody rdition within the cvity cn be considered to hve velocity-dependent pprent inertil mss () tht provides resistnce to movement t constnt velocity (Tble 1). For the cylinder to move t constnt velocity, n dditionl mount of potentil energy must be pplied to the moving cylinder in order to compenste for the pprent inertil mss of the blckbody rdition within. In light of wht we hve deduced bout the velocity-induced increse in internl energy tht will tke plce s result of the Doppler effect expnded to second order, we cn write the reltionship between the pplied potentil energy nd the chnge in kinetic energy of the rdition filled cylinder like so: 7 (39) Where, is the differentil in the internl energy density tht results from the differentil velocity 0.5c.9c
8 The Africn Review of Physics (2015) 10: chnge 7. Given tht Eqn. (23) sttes tht, 7 (40) Tble 1: The velocity-induced increse in the frequency ('), energy (h') nd momentum ( _f ) of photon t the pek of the curve chrcterizing blckbody rdition; the velocity-induced increse in the temperture (R), internl energy density ( n ), photon number density l (y) nd entropy density l ( ) of the blckbody rdition; nd l the velocity-induced increse in the pprent mss ( n ) of blckbody rdition initilly t rest t 300 K for cylinder with mtte blck nd dibtic wlls nd with constnt nd invrint volume. The vlues re given for n initil stte of zero velocity nd finl stte with constnt velocity of 0.9c. 7 ' s -1 h' J h' kg m s -1 R K b J m -3 b m -3 j b J K -1 m -3 kg c This mens tht the verge force clculted from the work-energy theorem given in Eqn. (3) to be sufficient to ccelerte the cvity with constnt mss t rest to given velocity will ctully be n underestimte of the required force. The dditionl force necessry is result of the velocity-dependent increse in pprent inerti () of the photon gs within the cylinder tht must lso be considered when clculting the reltionship between the verge pplied force (!"# ) nd ccelertion ():!"# 4 5 (41) The optomechnicl counterforce ( Ž " ) resulting from the Doppler effect expnded to second order ws lredy found to describe nd explin the nonliner reltionship between pplied force nd the ccelertion of prticles with chrge nd/or mgnetic moment [11,26]:!"# Ž " (42) nd here I hve shown tht the Doppler effect cn describe nd explin the nonliner reltionship between pplied potentil energy nd constnt velocity for n extended object: $ $ Ž "!"# $ & $ & (43) The discrepncy between Hsenöhrl s nd Einstein s equtions for the reltionship between the energy nd inerti of rdition hs been difficult to reconcile [27-35]. Here I hve obtined Einstein s reltionship for the energy equivlent of mss bsed on Hsenöhrl s gednkenexperiment by tking into considertion the reltionship between the energy nd liner momentum of photon nd the dynmic processes tht result from the Doppler effect expnded to the second order in Eucliden spce nd Newtonin time. References [1] A. Einstein, Does the inerti of body depend upon its energy content? In: The Collected Ppers of Albert Einstein. Volume 2. Doc. 24. Trnslted by Ann Beck. Princeton University Press, Princeton, NJ pp (1905). [2] A. Einstein, On the inerti of energy required by the reltivity principle. In: The Collected Ppers of Albert Einstein. Volume 2. Doc. 45. Trnslted by Ann Beck. Princeton University Press, Princeton, NJ pp (1907). [3] A. Einstein, On the reltivity principle nd the conclusions drwn from it. In: The Collected Ppers of Albert Einstein. Volume 2. Doc. 47. Trnslted by Ann Beck. Princeton University Press, Princeton, NJ pp (1907).
9 The Africn Review of Physics (2015) 10: [4] F. Hsenöhrl, F. Sitzungsberichte der mthemtisch-nturwissenschftliche Klsse der kiserlichen Akdemie der Wissenschften, Wien 113 II, 1039 (1904). [5] F. Hsenöhrl, Annlen der Physik 320, 344 (1904). [6] F. Hsenöhrl, Annlen der Physik 321, 589 (1905). [7] J. H. Poynting, Philosophicl Trnsctions of the Royl Society of London A 202, 525 (1904). [8] R. Wyne, The Africn Physicl Review 4, 43 (2010); v/rticle/view/369/175 [9] L. Pge, Proceedings of the Ntionl Acdemy of Science USA 4, 47 (1918). [10] R. Wyne, The Africn Review of Physics 7, 115 (2012); v/rticle/view/539/233 [11] R. Wyne, Act Physic Polonic B. 41, 2297 (2010). [12] A. Einstein, On the quntum theory of rdition. In: The Collected Ppers of Albert Einstein. Volume 6. Doc. 38. Trnslted by Alfred Engel. Princeton University Press, Princeton, NJ pp (1916). [13] A. Einstein, On the development of our views concerning the nture nd constitution of rdition. In: The Collected Ppers of Albert Einstein. Volume 2. Doc. 60. Trnslted by Ann Beck. Princeton University Press, Princeton, NJ pp (1909). [14] H. S. Leff, Americn Journl of Physics 70, 792 (2002). [15] R. E. Kelly, Americn Journl of Physics 49, 714 (1981). [16] B.-Z. Ginzburg nd R. Wyne, Turkish Journl of Physics 36, 155 (2012). [17] H. Cllen nd G. Horwitz, Americn Journl of Physics 39, 938 (1971). [18] M. Plnck, The Theory of Het Rdition (Blkiston s Son & Co., Phildelphi, 1914). [19] D. V. Schroeder, An Introduction to Therml Physics (Addison Wesley Longmn, Sn Frncisco, 2000). [20] R. Clusius, Philosophicl Mgzine 4 th Series 14, 108 (1857). [21] H. A. Bent, The Second Lw. An Introduction to Clssicl nd Sttisticl Thermodynmics, second edition (Oxford University Press, New York. 1965). [22] R. Wyne, Light nd Video Microscopy (Elsevier/Acdemic Press, Amsterdm, 2009). [23] R. Wyne, Turkish Journl of Physics 36, 165 (2012). [24] R. Wyne, The Africn Review of Physics 9, 183 (2012). [25] R. Wyne, Nture of Light from the Perspective of Biologist: Wht is Photon? In: Hndbook of Photosynthesis, Third Edition, M. Pessrkli, ed. CRC Press, Tylor nd Frncis Group, London. [26] R. Wyne, The Africn Review of Physics 8, 283 (2013); v/rticle/view/761/320 [27] P. Lenrd, Gret Men of Science. A History of Scientific Progress (G. Bell nd Sons, London, 1933) p.371. [28] M. von Lue, Inerti nd Energy. In: Albert Einstein: Philosopher-Scientist. P. A. Schilpp, ed. Tudor Publishing Co., New York. pp (1949). [29] E. Whittker, A History of the Theories of Aether nd Electricity. Volume 2. The Modern Theories. Thoms Nelson nd Sons, London. pp (1953). [30] W. Puli, Theory of Reltivity, Dover, New York. pp (1981). [31] M. Jmmer, Concepts of Mss in Contemporry Physics nd Philosophy (Princeton University Press, Princeton, NJ, 2000) p.72. [32] A. Einstein, The principle of conservtion of motion of the center of grvity nd the inerti of energy. In: The Collected Ppers of Albert Einstein. Volume 2. Doc. 35. Trnslted by Ann Beck. Princeton University Press, Princeton, NJ pp (1906). [33] S. Boughn. nd T. Rothmn, Hsenöhrl nd the equivlence of mss nd energy (2011); [34] S. Boughn, Europen Physicl Journl H. 38, 261 (2013); rt253a fepjh252fe pdf?uth66= _ fdc b eee9&ext=.pdf [35] A. Einstein, Reltivity. The Specil nd the Generl Theory (Bonnz Books, New York, 1961) p.44. Received: 16 September, 2014 Accepted: 4 Mrch, 2015
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 informationKINEMATICS OF RIGID BODIES
KINEMTICS OF RIGID ODIES Introduction In rigid body kinemtics, e use the reltionships governing the displcement, velocity nd ccelertion, but must lso ccount for the rottionl motion of the body. Description
More information4 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 informationA5682: 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 information13.4 Work done by Constant Forces
13.4 Work done by Constnt Forces We will begin our discussion of the concept of work by nlyzing the motion of n object in one dimension cted on by constnt forces. Let s consider the following exmple: push
More informationThe heat budget of the atmosphere and the greenhouse effect
The het budget of the tmosphere nd the greenhouse effect 1. Solr rdition 1.1 Solr constnt The rdition coming from the sun is clled solr rdition (shortwve rdition). Most of the solr rdition is visible light
More informationMath 8 Winter 2015 Applications of Integration
Mth 8 Winter 205 Applictions of Integrtion Here re few importnt pplictions of integrtion. The pplictions you my see on n exm in this course include only the Net Chnge Theorem (which is relly just the Fundmentl
More information2.57/2.570 Midterm Exam No. 1 March 31, :00 am -12:30 pm
2.57/2.570 Midterm Exm No. 1 Mrch 31, 2010 11:00 m -12:30 pm Instructions: (1) 2.57 students: try ll problems (2) 2.570 students: Problem 1 plus one of two long problems. You cn lso do both long problems,
More informationConsequently, 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 informationName Solutions to Test 3 November 8, 2017
Nme Solutions to Test 3 November 8, 07 This test consists of three prts. Plese note tht in prts II nd III, you cn skip one question of those offered. Some possibly useful formuls cn be found below. Brrier
More informationEnergy creation in a moving solenoid? Abstract
Energy cretion in moving solenoid? Nelson R. F. Brg nd Rnieri V. Nery Instituto de Físic, Universidde Federl do Rio de Jneiro, Cix Postl 68528, RJ 21941-972 Brzil Abstrct The electromgnetic energy U em
More informationConducting 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 informationSummary 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 informationStudy Guide Final Exam. Part A: Kinetic Theory, First Law of Thermodynamics, Heat Engines
Msschusetts Institute of Technology Deprtment of Physics 8.0T Fll 004 Study Guide Finl Exm The finl exm will consist of two sections. Section : multiple choice concept questions. There my be few concept
More information(See Notes on Spontaneous Emission)
ECE 240 for Cvity from ECE 240 (See Notes on ) Quntum Rdition in ECE 240 Lsers - Fll 2017 Lecture 11 1 Free Spce ECE 240 for Cvity from Quntum Rdition in The electromgnetic mode density in free spce is
More informationWeek 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 informationDIRECT CURRENT CIRCUITS
DRECT CURRENT CUTS ELECTRC POWER Consider the circuit shown in the Figure where bttery is connected to resistor R. A positive chrge dq will gin potentil energy s it moves from point to point b through
More informationImproper 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 informationState 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- 5 - TEST 2. This test is on the final sections of this session's syllabus and. should be attempted by all students.
- 5 - TEST 2 This test is on the finl sections of this session's syllbus nd should be ttempted by ll students. Anything written here will not be mrked. - 6 - QUESTION 1 [Mrks 22] A thin non-conducting
More informationMeasuring Electron Work Function in Metal
n experiment of the Electron topic Mesuring Electron Work Function in Metl Instructor: 梁生 Office: 7-318 Emil: shling@bjtu.edu.cn Purposes 1. To understnd the concept of electron work function in metl nd
More informationMAC-solutions of the nonexistent solutions of mathematical physics
Proceedings of the 4th WSEAS Interntionl Conference on Finite Differences - Finite Elements - Finite Volumes - Boundry Elements MAC-solutions of the nonexistent solutions of mthemticl physics IGO NEYGEBAUE
More informationPhysics 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 informationPractive Derivations for MT 1 GSI: Goni Halevi SOLUTIONS
Prctive Derivtions for MT GSI: Goni Hlevi SOLUTIONS Note: These solutions re perhps excessively detiled, but I wnted to ddress nd explin every step nd every pproximtion in cse you forgot where some of
More informationForces from Strings Under Tension A string under tension medites force: the mgnitude of the force from section of string is the tension T nd the direc
Physics 170 Summry of Results from Lecture Kinemticl Vribles The position vector ~r(t) cn be resolved into its Crtesin components: ~r(t) =x(t)^i + y(t)^j + z(t)^k. Rtes of Chnge Velocity ~v(t) = d~r(t)=
More informationJackson 2.26 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell
Jckson 2.26 Homework Problem Solution Dr. Christopher S. Bird University of Msschusetts Lowell PROBLEM: The two-dimensionl region, ρ, φ β, is bounded by conducting surfces t φ =, ρ =, nd φ = β held t zero
More informationChapter 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 informationPHYS Summer Professor Caillault Homework Solutions. Chapter 2
PHYS 1111 - Summer 2007 - Professor Cillult Homework Solutions Chpter 2 5. Picture the Problem: The runner moves long the ovl trck. Strtegy: The distnce is the totl length of trvel, nd the displcement
More informationPhysics 712 Electricity and Magnetism Solutions to Final Exam, Spring 2016
Physics 7 Electricity nd Mgnetism Solutions to Finl Em, Spring 6 Plese note tht some possibly helpful formuls pper on the second pge The number of points on ech problem nd prt is mrked in squre brckets
More informationSet up Invariable Axiom of Force Equilibrium and Solve Problems about Transformation of Force and Gravitational Mass
Applied Physics Reserch; Vol. 5, No. 1; 013 ISSN 1916-9639 E-ISSN 1916-9647 Published by Cndin Center of Science nd Eduction Set up Invrible Axiom of orce Equilibrium nd Solve Problems bout Trnsformtion
More informationHeat flux and total heat
Het flux nd totl het John McCun Mrch 14, 2017 1 Introduction Yesterdy (if I remember correctly) Ms. Prsd sked me question bout the condition of insulted boundry for the 1D het eqution, nd (bsed on glnce
More informationCHM 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 informationReview 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 informationProblems 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 informationCHAPTER 20: Second Law of Thermodynamics
CHAER 0: Second Lw of hermodynmics Responses to Questions 3. kg of liquid iron will hve greter entropy, since it is less ordered thn solid iron nd its molecules hve more therml motion. In ddition, het
More informationThe Wave Equation I. MA 436 Kurt Bryan
1 Introduction The Wve Eqution I MA 436 Kurt Bryn Consider string stretching long the x xis, of indeterminte (or even infinite!) length. We wnt to derive n eqution which models the motion of the string
More informationPart I: Basic Concepts of Thermodynamics
Prt I: Bsic Concepts o Thermodynmics Lecture 4: Kinetic Theory o Gses Kinetic Theory or rel gses 4-1 Kinetic Theory or rel gses Recll tht or rel gses: (i The volume occupied by the molecules under ordinry
More informationPDE Notes. Paul Carnig. January ODE s vs PDE s 1
PDE Notes Pul Crnig Jnury 2014 Contents 1 ODE s vs PDE s 1 2 Section 1.2 Het diffusion Eqution 1 2.1 Fourier s w of Het Conduction............................. 2 2.2 Energy Conservtion.....................................
More informationPressure Wave Analysis of a Cylindrical Drum
Pressure Wve Anlysis of Cylindricl Drum Chris Clrk, Brin Anderson, Brin Thoms, nd Josh Symonds Deprtment of Mthemtics The University of Rochester, Rochester, NY 4627 (Dted: December, 24 In this pper, hypotheticl
More informationExam 1 Solutions (1) C, D, A, B (2) C, A, D, B (3) C, B, D, A (4) A, C, D, B (5) D, C, A, B
PHY 249, Fll 216 Exm 1 Solutions nswer 1 is correct for ll problems. 1. Two uniformly chrged spheres, nd B, re plced t lrge distnce from ech other, with their centers on the x xis. The chrge on sphere
More informationMaterial Space Motion Time Phenomenon of Kinetic Energy and Inertia of Material Bodies
AASCIT Journl of Physics 15; 1(4): 9-96 Published online July, 15 (http://wwwscitorg/journl/physics) Mteril Spce Motion Time Phenomenon of Kinetic Energy nd Inerti of Mteril Bodies F F Mende B Verkin Institute
More informationSimulation of Eclipsing Binary Star Systems. Abstract
Simultion of Eclipsing Binry Str Systems Boris Yim 1, Kenny Chn 1, Rphel Hui 1 Wh Yn College Kowloon Diocesn Boys School Abstrct This report briefly introduces the informtion on eclipsing binry str systems.
More informationThis 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 informationJURONG JUNIOR COLLEGE
JURONG JUNIOR COLLEGE 2010 JC1 H1 8866 hysics utoril : Dynmics Lerning Outcomes Sub-topic utoril Questions Newton's lws of motion 1 1 st Lw, b, e f 2 nd Lw, including drwing FBDs nd solving problems by
More informationMethod 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 informationPHYSICS 211 MIDTERM I 21 April 2004
PHYSICS MIDERM I April 004 Exm is closed book, closed notes. Use only your formul sheet. Write ll work nd nswers in exm booklets. he bcks of pges will not be grded unless you so request on the front of
More informationKINEMATICS OF RIGID BODIES
KINEMTICS OF RIGI OIES Introduction In rigid body kinemtics, e use the reltionships governing the displcement, velocity nd ccelertion, but must lso ccount for the rottionl motion of the body. escription
More informationHigher Checklist (Unit 3) Higher Checklist (Unit 3) Vectors
Vectors Skill Achieved? Know tht sclr is quntity tht hs only size (no direction) Identify rel-life exmples of sclrs such s, temperture, mss, distnce, time, speed, energy nd electric chrge Know tht vector
More informationMath 124A October 04, 2011
Mth 4A October 04, 0 Viktor Grigoryn 4 Vibrtions nd het flow In this lecture we will derive the wve nd het equtions from physicl principles. These re second order constnt coefficient liner PEs, which model
More informationPhysics 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 informationINTRODUCTION. The three general approaches to the solution of kinetics problems are:
INTRODUCTION According to Newton s lw, prticle will ccelerte when it is subjected to unblnced forces. Kinetics is the study of the reltions between unblnced forces nd the resulting chnges in motion. The
More informationSOLUTIONS FOR ADMISSIONS TEST IN MATHEMATICS, COMPUTER SCIENCE AND JOINT SCHOOLS WEDNESDAY 5 NOVEMBER 2014
SOLUTIONS FOR ADMISSIONS TEST IN MATHEMATICS, COMPUTER SCIENCE AND JOINT SCHOOLS WEDNESDAY 5 NOVEMBER 014 Mrk Scheme: Ech prt of Question 1 is worth four mrks which re wrded solely for the correct nswer.
More informationVibrational Relaxation of HF (v=3) + CO
Journl of the Koren Chemicl Society 26, Vol. 6, No. 6 Printed in the Republic of Kore http://dx.doi.org/.52/jkcs.26.6.6.462 Notes Vibrtionl Relxtion of HF (v3) + CO Chng Soon Lee Deprtment of Chemistry,
More informationTheoretische Physik 2: Elektrodynamik (Prof. A.-S. Smith) Home assignment 4
WiSe 1 8.1.1 Prof. Dr. A.-S. Smith Dipl.-Phys. Ellen Fischermeier Dipl.-Phys. Mtthis Sb m Lehrstuhl für Theoretische Physik I Deprtment für Physik Friedrich-Alexnder-Universität Erlngen-Nürnberg Theoretische
More information+ x 2 dω 2 = c 2 dt 2 +a(t) [ 2 dr 2 + S 1 κx 2 /R0
Notes for Cosmology course, fll 2005 Cosmic Dynmics Prelude [ ds 2 = c 2 dt 2 +(t) 2 dx 2 ] + x 2 dω 2 = c 2 dt 2 +(t) [ 2 dr 2 + S 1 κx 2 /R0 2 κ (r) 2 dω 2] nd x = S κ (r) = r, R 0 sin(r/r 0 ), R 0 sinh(r/r
More informationData Provided: A formula sheet and table of physical constants are attached to this paper.
PHY51A Dt Provided: A formul sheet nd tble of physicl constnts re ttched to this pper. DEPARTMENT OF PHYSICS AND ASTRONOMY Spring Semester (015-016) From Thermodynmics to Atomic nd Nucler Physics Pper
More informationPhysics 1402: Lecture 7 Today s Agenda
1 Physics 1402: Lecture 7 Tody s gend nnouncements: Lectures posted on: www.phys.uconn.edu/~rcote/ HW ssignments, solutions etc. Homework #2: On Msterphysics tody: due Fridy Go to msteringphysics.com Ls:
More informationPh2b Quiz - 1. Instructions
Ph2b Winter 217-18 Quiz - 1 Due Dte: Mondy, Jn 29, 218 t 4pm Ph2b Quiz - 1 Instructions 1. Your solutions re due by Mondy, Jnury 29th, 218 t 4pm in the quiz box outside 21 E. Bridge. 2. Lte quizzes will
More informationCMDA 4604: Intermediate Topics in Mathematical Modeling Lecture 19: Interpolation and Quadrature
CMDA 4604: Intermedite Topics in Mthemticl Modeling Lecture 19: Interpoltion nd Qudrture In this lecture we mke brief diversion into the res of interpoltion nd qudrture. Given function f C[, b], we sy
More informationConservation 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 informationA 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 informationCandidates must show on each answer book the type of calculator used.
UNIVERSITY OF EAST ANGLIA School of Mthemtics My/June UG Exmintion 2007 2008 ELECTRICITY AND MAGNETISM Time llowed: 3 hours Attempt FIVE questions. Cndidtes must show on ech nswer book the type of clcultor
More informationMATH 144: Business Calculus Final Review
MATH 144: Business Clculus Finl Review 1 Skills 1. Clculte severl limits. 2. Find verticl nd horizontl symptotes for given rtionl function. 3. Clculte derivtive by definition. 4. Clculte severl derivtives
More information1 Which of the following summarises the change in wave characteristics on going from infra-red to ultraviolet in the electromagnetic spectrum?
Which of the following summrises the chnge in wve chrcteristics on going from infr-red to ultrviolet in the electromgnetic spectrum? frequency speed (in vcuum) decreses decreses decreses remins constnt
More informationPhysics 116C Solution of inhomogeneous ordinary differential equations using Green s functions
Physics 6C Solution of inhomogeneous ordinry differentil equtions using Green s functions Peter Young November 5, 29 Homogeneous Equtions We hve studied, especilly in long HW problem, second order liner
More informationCAPACITORS AND DIELECTRICS
Importnt Definitions nd Units Cpcitnce: CAPACITORS AND DIELECTRICS The property of system of electricl conductors nd insultors which enbles it to store electric chrge when potentil difference exists between
More informationMain topics for the Second Midterm
Min topics for the Second Midterm The Midterm will cover Sections 5.4-5.9, Sections 6.1-6.3, nd Sections 7.1-7.7 (essentilly ll of the mteril covered in clss from the First Midterm). Be sure to know the
More informationSpecial 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 informationProblem Set 3 Solutions
Chemistry 36 Dr Jen M Stndrd Problem Set 3 Solutions 1 Verify for the prticle in one-dimensionl box by explicit integrtion tht the wvefunction ψ ( x) π x is normlized To verify tht ψ ( x) is normlized,
More informationPhysics 9 Fall 2011 Homework 2 - Solutions Friday September 2, 2011
Physics 9 Fll 0 Homework - s Fridy September, 0 Mke sure your nme is on your homework, nd plese box your finl nswer. Becuse we will be giving prtil credit, be sure to ttempt ll the problems, even if you
More informationSection 4: Integration ECO4112F 2011
Reding: Ching Chpter Section : Integrtion ECOF Note: These notes do not fully cover the mteril in Ching, ut re ment to supplement your reding in Ching. Thus fr the optimistion you hve covered hs een sttic
More informationJackson 2.7 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell
Jckson.7 Homework Problem Solution Dr. Christopher S. Bird University of Msschusetts Lowell PROBLEM: Consider potentil problem in the hlf-spce defined by, with Dirichlet boundry conditions on the plne
More informationMATH , Calculus 2, Fall 2018
MATH 36-2, 36-3 Clculus 2, Fll 28 The FUNdmentl Theorem of Clculus Sections 5.4 nd 5.5 This worksheet focuses on the most importnt theorem in clculus. In fct, the Fundmentl Theorem of Clculus (FTC is rgubly
More informationwest (mrw3223) HW 24 lyle (16001) 1
west (mrw3223) HW 24 lyle (16001) 1 This print-out should hve 30 questions. Multiple-choice questions my continue on the next column or pge find ll choices before nswering. Reding ssignment: Hecht, sections
More informationIntroduction to Astrophysics
PHY472 Dt Provided: Formul sheet nd physicl constnts Dt Provided: A formul sheet nd tble of physicl constnts is ttched to this pper. DEPARTMENT OF PHYSICS & Autumn Semester 2009-2010 ASTRONOMY DEPARTMENT
More information200 points 5 Problems on 4 Pages and 20 Multiple Choice/Short Answer Questions on 5 pages 1 hour, 48 minutes
PHYSICS 132 Smple Finl 200 points 5 Problems on 4 Pges nd 20 Multiple Choice/Short Answer Questions on 5 pges 1 hour, 48 minutes Student Nme: Recittion Instructor (circle one): nme1 nme2 nme3 nme4 Write
More information5.7 Improper Integrals
458 pplictions of definite integrls 5.7 Improper Integrls In Section 5.4, we computed the work required to lift pylod of mss m from the surfce of moon of mss nd rdius R to height H bove the surfce of the
More informationME 141. Lecture 10: Kinetics of particles: Newton s 2 nd Law
ME 141 Engineering Mechnics Lecture 10: Kinetics of prticles: Newton s nd Lw Ahmd Shhedi Shkil Lecturer, Dept. of Mechnicl Engg, BUET E-mil: sshkil@me.buet.c.bd, shkil6791@gmil.com Website: techer.buet.c.bd/sshkil
More informationLecture 13 - Linking E, ϕ, and ρ
Lecture 13 - Linking E, ϕ, nd ρ A Puzzle... Inner-Surfce Chrge Density A positive point chrge q is locted off-center inside neutrl conducting sphericl shell. We know from Guss s lw tht the totl chrge on
More informationPhysicsAndMathsTutor.com
1. A uniform circulr disc hs mss m, centre O nd rdius. It is free to rotte bout fixed smooth horizontl xis L which lies in the sme plne s the disc nd which is tngentil to the disc t the point A. The disc
More informationPhysics 319 Classical Mechanics. G. A. Krafft Old Dominion University Jefferson Lab Lecture 2
Physics 319 Clssicl Mechnics G. A. Krfft Old Dominion University Jefferson Lb Lecture Undergrdute Clssicl Mechnics Spring 017 Sclr Vector or Dot Product Tkes two vectors s inputs nd yields number (sclr)
More informationTHE INTERVAL LATTICE BOLTZMANN METHOD FOR TRANSIENT HEAT TRANSFER IN A SILICON THIN FILM
ROMAI J., v.9, no.2(2013), 173 179 THE INTERVAL LATTICE BOLTZMANN METHOD FOR TRANSIENT HEAT TRANSFER IN A SILICON THIN FILM Alicj Piseck-Belkhyt, Ann Korczk Institute of Computtionl Mechnics nd Engineering,
More informationProf. Anchordoqui. Problems set # 4 Physics 169 March 3, 2015
Prof. Anchordoui Problems set # 4 Physics 169 Mrch 3, 15 1. (i) Eight eul chrges re locted t corners of cube of side s, s shown in Fig. 1. Find electric potentil t one corner, tking zero potentil to be
More informationIntro to Nuclear and Particle Physics (5110)
Intro to Nucler nd Prticle Physics (5110) Feb, 009 The Nucler Mss Spectrum The Liquid Drop Model //009 1 E(MeV) n n(n-1)/ E/[ n(n-1)/] (MeV/pir) 1 C 16 O 0 Ne 4 Mg 7.7 14.44 19.17 8.48 4 5 6 6 10 15.4.41
More informationPhysics 2135 Exam 1 February 14, 2017
Exm Totl / 200 Physics 215 Exm 1 Ferury 14, 2017 Printed Nme: Rec. Sec. Letter: Five multiple choice questions, 8 points ech. Choose the est or most nerly correct nswer. 1. Two chrges 1 nd 2 re seprted
More informationNew 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 informationFig. 1. Open-Loop and Closed-Loop Systems with Plant Variations
ME 3600 Control ystems Chrcteristics of Open-Loop nd Closed-Loop ystems Importnt Control ystem Chrcteristics o ensitivity of system response to prmetric vritions cn be reduced o rnsient nd stedy-stte responses
More informationPhysics 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 informationBernoulli 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 informationThe final exam will take place on Friday May 11th from 8am 11am in Evans room 60.
Mth 104: finl informtion The finl exm will tke plce on Fridy My 11th from 8m 11m in Evns room 60. The exm will cover ll prts of the course with equl weighting. It will cover Chpters 1 5, 7 15, 17 21, 23
More informationLight and Optics Propagation of light Electromagnetic waves (light) in vacuum and matter Reflection and refraction of light Huygens principle
Light nd Optics Propgtion of light Electromgnetic wves (light) in vcuum nd mtter Reflection nd refrction of light Huygens principle Polristion of light Geometric optics Plne nd curved mirrors Thin lenses
More informationFirst Law of Thermodynamics. Control Mass (Closed System) Conservation of Mass. Conservation of Energy
First w of hermodynmics Reding Problems 3-3-7 3-0, 3-5, 3-05 5-5- 5-8, 5-5, 5-9, 5-37, 5-0, 5-, 5-63, 5-7, 5-8, 5-09 6-6-5 6-, 6-5, 6-60, 6-80, 6-9, 6-, 6-68, 6-73 Control Mss (Closed System) In this section
More informationProperties of Integrals, Indefinite Integrals. Goals: Definition of the Definite Integral Integral Calculations using Antiderivatives
Block #6: Properties of Integrls, Indefinite Integrls Gols: Definition of the Definite Integrl Integrl Clcultions using Antiderivtives Properties of Integrls The Indefinite Integrl 1 Riemnn Sums - 1 Riemnn
More informationThe Atwood Machine OBJECTIVE INTRODUCTION APPARATUS THEORY
The Atwood Mchine OBJECTIVE To derive the ening of Newton's second lw of otion s it pplies to the Atwood chine. To explin how ss iblnce cn led to the ccelertion of the syste. To deterine the ccelertion
More informationpivot F 2 F 3 F 1 AP Physics 1 Practice Exam #3 (2/11/16)
AP Physics 1 Prctice Exm #3 (/11/16) Directions: Ech questions or incomplete sttements below is followed by four suggested nswers or completions. Select one tht is best in ech cse nd n enter pproprite
More informationA formula sheet and table of physical constants is attached to this paper. Linear graph paper is available.
DEPARTMENT OF PHYSICS AND ASTRONOMY Dt Provided: A formul sheet nd tble of physicl constnts is ttched to this pper. Liner grph pper is vilble. Spring Semester 2015-2016 PHYSICS 1 HOUR Answer questions
More informationPlates on elastic foundation
Pltes on elstic foundtion Circulr elstic plte, xil-symmetric lod, Winkler soil (fter Timoshenko & Woinowsky-Krieger (1959) - Chpter 8) Prepred by Enzo Mrtinelli Drft version ( April 016) Introduction Winkler
More informationQuantum 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 informationTerminal Velocity and Raindrop Growth
Terminl Velocity nd Rindrop Growth Terminl velocity for rindrop represents blnce in which weight mss times grvity is equl to drg force. F 3 π3 ρ L g in which is drop rdius, g is grvittionl ccelertion,
More informationCHEM-UA 652: Thermodynamics and Kinetics
CHEM-UA 65: Thermodynmics nd Kinetics Notes for Lecture I. WHAT IS PHYSICAL CHEMISTRY? Physicl chemistry is truly interdisciplinry brnch of chemistry tht exists t the boundry between chemistry nd physics.
More information