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thoroughly versed in their philosophy says in his " Amphi- theatro
The theory of heat radiation
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The Translation Studies Reader.pdf
REFRACTION IN A THEORY OF LITERATURE. 19 William Frawley. 250. PROLEGOMENON TO A THEORY OF TRANSLATION. 20 Philip E.Lewis. 264. THE MEASURE OF TRANSLATION
OPTics
conditions more on evanescent waves
MATHEMATICS
"by any attempt to dissociate it from its history.". J. W. L. GLAISHMR gatfc. MACMILLAN AND CO.
time-and-free-will-bergson.pdf
of opinion is part of the whole evolution". philosophic la physique
CURSUSINGENIEURSUPELEC
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the machine to help them compute the motion of Mars and the refraction of starlight. Difference engines were never widely used; the technology was eclipsed
ASTRONOMYDEPT,
THETHEORYOFHEATRADIATION
PLANCKANDMASIUS
LiTHETHEORY
OFHEATRADIATION
BYDR.MAXPLANCK
AUTHORISEDJTRANSLATION
BYMORTONJVUSIUS,M.A.,Ph.D.(Leipzig)
WITH7ILLUSTRATIONS
PHILADELPHIA
P.BLAKISTONSSON&CO.
1012WALNUTSTREET
SEP29ASTRONOMYDEFT;
COPYRIGHT,1914,BYP.BLAKISTONSSON&Co.
THE.MAPLHPRESS-YORK-PA
TRANSLATORSPREFACE
ofreasoninginaforeignlanguage. toobriefortopresentsomedifficulties. viTRANSLATORSPREFACE scriptandthegalleyproof.MORTONMASIUS.WORCESTER,MASS.,
February,1914.
PREFACETOSECONDEDITION
vii viiiPREFACETOSECONDEDITIONPREFACETOSECONDEDITIONix
discussalldifferingopinions. quantumofactionpromisestothrowsomelight. generation.THEAUTHOR.
BERLIN,
November,1912.
PREFACETOFIRSTEDITION
asregardsspecialdetails. XITABLEOFCONTENTS
PARTIFUNDAMENTALFACTSANDDEFINITIONS
CHAPTERPAGE
I.GeneralIntroduction1
BlackRadiation22
PARTII
,I.MaxwellsRadiationPressure49II.Stefan-BoltzmannLawofRadiation59
III.WiensDisplacementLaw69
PARTIII
ENTROPYANDPROBABILITY
II.IdealMonatomicGases127
III.IdealLinearOscillators135
Equilibrium144
PARTIV
ASYSTEMOFOSCILLATORSINASTATIONARYFIELDOF
RADIATION
II.AbsorbedEnergy155
III.EmittedEnergy.StationaryState161
QuantaofMatterandofElectricity167
xiii xivTABLEOFCONTENTS PARTVIRREVERSIBLERADIATIONPROCESSES
I.FieldsofRadiationinGeneral189
II.OneOscillatorintheFieldofRadiation196
III.ASystemofOscillators200
bytheAuthor216Appendices218
Errata..225
PARTIFUNDAMENTALFACTSANDDEFINITIONS
RADIATIONOFHEAT
CHAPTERI
GENERALINTRODUCTION
conduction. 12FUNDAMENTALFACTSANDDEFINITIONS
speakofthe " giverisetoanyparticulardifficulty.GENERALINTRODUCTION3
wespeakof phenomenatobeconsidered.4FUNDAMENTALFACTSANDDEFINITIONS
randomundirectedheatmotioncannotbemade. firstthethreeprocessesjustmentioned. otherformsofenergy(heat,1chemicalorelectricenergy,etc.)
lessintenseradiations. "heat."(Tr.)GENERALINTRODUCTION5
r >v.The6FUNDAMENTALFACTSANDDEFINITIONS
the alsobefinite. prism. elementdrto dtdT-dttdv2*,.(1) conicalelementsdttis4,w,weget: CO dt-dr.SwI<,dv.t(2)GENERALINTRODUCTION7
weaker,BastrongeremitterthanA. giventhecommonname "phenomenaofluminescence."We shalldealwithpure pletelydeterminedbythetemperature. nonof " chemically. p.155,1904.8FUNDAMENTALFACTSANDDEFINITIONS
erlyregardedasopticallyhomogeneous,1providedonlythatthe
turbidbythepresenceofmolecules. phereasbytheairmoleculesthemselves. tionisproportionaltos,say fts(3) radiationandiscalledthe appliedtoanymaterialsubstance.GENERALINTRODUCTION9
forraysofshorterwavelength;1hencethebluecolorofdiffuse
skylight. anyfurtherdiscussionofthesequestions. andrefractionmaybe " regular,"therebeingasinglereflected medium. iLordRayleigh,Phil.Mag.,47,p.379,1899.10FUNDAMENTALFACTSANDDEFINITIONS
called "black."Inadditionto
used.AccordingtoG.Kirchhoff1itdenotesabodywhichhas
thesurface.2 definition. body.GENERALINTRODUCTION11
12.Absorption.Heatraysaredestroyedby
" absorption." isused. andmaybewritten a,s(4)Hereavisknownasthe
peratureT,andthenatureofthemedium. small,containsmanywavelengths(Sec.2).12FUNDAMENTALFACTSANDDEFINITIONS
ray,butonadefinitepositioninspace. when >=!GENERALINTRODUCTION13
surface. andbyanazimuth coneis d!2=sin0-d6-d<i>.(5) do-inthedirectionoftheconedttis: dtdo-cosddttK=Ksin6cosdd d<t>do-dt.(6) stitutingTTforandTT+ <for precedingone. integratingwithrespectto (/>fromto2irandwithrespectto7Tfromto-
27T2I <*0f t/ot/o ddKsincos8do-dt.
14FUNDAMENTALFACTSANDDEFINITIONS
TTKd<jdt.(7)
Fromapencilofrayscalled
"parallel "afiniteamountofenergyof narrowcone. homogeneousormonochromatic. intensitymaybewrittenintheformK.cosV+K/sinV
andK.sinV+K/cosV(8)GENERALINTRODUCTION15
the v.Hencewecallthesevaluesthe
"principalvaluesoftheintensi maywritegenerally I (9) CO dtdo-cos6dQIdv(K.+K/)(10)I K,:ForunpolarizedraysK,=K/,andhence
ooK=2CdvK,,(12)=2CdvK
2dtdo-cos$dtiK,dv=2dtdo-sin6cosdd
d<j>K,dv.(13) foundfrom(7)and(12);itis27rdadt1Kvdv.(14)I
16FUNDAMENTALFACTSANDDEFINITIONS
Thiswillbefurtherdiscussedlateron.
from v=\(15)A qdXdv--* isobtained.Hencewegetbysubstitution:E,=.(16)
GENERALINTRODUCTION17
lineardimensionsoftheelementsdaandda fbutstillsosmall manousmedia. angleis dacos(/,r)^-I"
where/denotesthenormalofda fandtheangle(v 1 ,r)istobe ofthevertexoftheconeonda. radiationrequiredisfoundtobe:ArArcos(r,r)-cos(/,r)K----at.(17)
energywillbe,accordingtoequation(11), dadacos(v,r)cos(i>,r)K,,dv--dt.(18)r2
ifwechoosedalargecomparedwithda.18FUNDAMENTALFACTSANDDEFINITIONS
"focalplanes"ofthepencil. thatcasethe "cross-section "ofthewholepencilatadefiniteGENERALINTRODUCTION19
liesataninfinitedistance. ofradiusr,rbeinglargecompared withthelineardimensionsofvbut stillsosmallthatnoappreciable absorptionorscatteringoftheradia tiontakesplaceinthedistancer (Fig.1).Everyraywhichreaches vmustthencomefromsomepoint onthesurfaceofthesphere.If, then,weatfirstconsideronlyallthe raysthatcomefromthepointsofan morethanonce.20FUNDAMENTALFACTSANDDEFINITIONS
sis: certainelementofa hencetheenergyis: -f-f rdaJ~K=-S2-Kda.(19)
fromdaandentervwehaveKda_Kdo-
r2qr2q -ofa thesphere,wegetforthewholeenergy: -IKdQ. dividingbyv.Itis =-KdQ. lj (20)GENERALINTRODUCTION21
onintegrationweget: trumweget: (22) -(K.+K/)dfi,(23)u,=Ii ij directions: STTK, u,=-(24)CHAPTERII
inentropyispossible. significance. (Sec.52). 22RADIATIONATTHERMODYNAMICEQUILIBRIUM23
scattering. theelementofarea.24FUNDAMENTALFACTSANDDEFINITIONS
volume-elementv. CO dtVS-JTIdvV-STTI Jo chemicalnatureofthemedium. intensity(energyradiatedperunittime) da-~ 2-K spectrumseparately: 2daHencetheintensityofamonochromaticrayis:
2da*K,dv.
r2 thetimedtis,accordingto(4), dta,,s2da9K,dv. r2RADIATIONATTHERMODYNAMICEQUILIBRIUM25
Cda= Jr*= 00 f,K, Jo dtvSirIavK,dv.(25) Jo oo =IOLK,,dv.f*,^=r JotJo frequencytherelation: e,=a,K,,or(26)K,=(27)av
tionofthemediumforthisfrequency.26FUNDAMENTALFACTSANDDEFINITIONS
whateverofthatcolor. raysofthefrequencyv.RADIATIONATTHERMODYNAMICEQUILIBRIUM27
finitecoefficientofabsorption. similarto(25),namely, CO ftK,dv.(28) sionby-r-.Thisgives 00 fJo K,dv, dtvdSlhK,,dv.(29)28FUNDAMENTALFACTSANDDEFINITIONS
otherrays. ousisotropicmediumwhichisinthermodynamic thiscasedt=l,6=0,by dadfiK,dv. .(30) mediumwereperfectlydiathermanous.RADIATIONATTHERMODYNAMICEQUILIBRIUM29
byputting do- dt=l,dr=drr2dtt,dtt=-^TO andomittingthenumericalfactor2.WethusgetE=drdttdae,dv.(31)
distances=drwehave or, dr and,byintegration, whichreachesisfoundtobeE=Ee-(a
"+^ro=drdfido-c,*-**+**dv.(32) 00 d!2dadve,fdre-(a >+ft >)r=dttda^dv.(33)f 130FUNDAMENTALFACTSANDDEFINITIONS
fromwithout.TheradiationE fthuscollectedbythevolume- elementatrisfound,byputtingin(29), dt=1,v=drdQ,r do- tobeE=drdQdaftK,dv.
rwefind:E+E=drdttdo-(e,+ftK,)dv.
Thepartofthisreachingis,similarto(32):
drdtida(e,+ftK.)dve~ ro(a-"W theenergyultimatelyreachingdo- dtidafe+ftK,)d asmaybeseenbycomparisonwith(26).RADIATIONATTHERMODYNAMICEQUILIBRIUM31
32FUNDAMENTALFACTSANDDEFINITIONS
ever.RADIATIONATTHERMODYNAMICEQUILIBRIUM33
mediumandfallingontheboundingsurface.BoundingSurface
FIG.3.
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