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This is the Past Exam of Physics which includes Kepler Third Law, Total Lunar Eclipses, Ecliptic, Types of Electromagnetic Radiation, Astronomical Telescopes, Constellations of Zodiac, Twin Paradox, Fundamental Forces etc. Key important points are: Mean Free Path, Kinetic Temperature, Steady State, Thermal Conductivity, Constant Pressure, Change in Entropy of Gas, Optical Spectrum, Refractve Index, State of Polarisation
Typology: Exams
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(Semester l: AY2009-10, 28November2009)
TimeAllowed:2Hours
(8)printedpages withFIVE(5)shortquestions in
Part
'l
andTHREE(3)longquestionsinPart2.
questions.
questions are tobewrittenintheanswerbooklet
provided.
5, Thisisa CLOSEDBOOKexamination. Calculatorsareallowed.
A list ofphysicalconstantsandformulaeisgivenonpages 2 and3,
Thermal
physics andkinetictheory:
(i) Kinetic mean free path is
given by
4
I = --: - , where
nvis thenumber density
J Z x. n , ' d 2
andd isthemolecular diameter.
(ii) Maxwell-Boltzmanndistributionin3D:
/ l 3 l 2 r a
(a)Root-mean-squarespeed:
y-^ = ^ltrt' .
V m
(v).Oneform of adiabat:p .Vv = Constanf .
(vi)Stefan-Boltzmann equation: P,"a
= 6. A.e .Ta
(vii)Planck radiationequation:
2 n. h. c 2
f o a l r , ) = m
(. r' k , ' T
(viii)Wiendisplacement law:
" 2.898x10-3m
.K
lu
peak
=
(ix) Convectionequation: Pror,
= h. A. LT.
(x)Conductionequation:
Pcond
= -k A +
L
(xi)Linear thermalexpansion: AL= cr.L.LT.
(b)Averagespeed:
v,,
(c)Most-probable speed: ,," =
^l2krT '
l l m
(iii) ldealgasequation:p .V = n .R.T .
(iv) VanderWaalsequation:
^ ^ 2
( p +
o ' l '
). ( v- n. b )
= n ' R. T.
" v z
Thermodynamics:
(i)First lawof thermodynamics:LU
= qin
expansionworkdonebythegas: W,,,
=
[p
.dV.
(ii)Carnotheat-engine efficiency e. =1-L.
" T ,
Geometricoptics:
(i)p and
q are objectandimage distancesmeasured
respectivelyon oppositesidesof thelensor of the
refracting surface:
(a) Object-imagerelation(thin
t
' . R ,
R r )
(b)Refracting-surfaceequation:
bns):
1*
1
=
1
,
p q t
f r t
,
D z
_ f l 2 - D t
p q R
(iii)Enhopy
dS
=
dg',n
.
T
(iv)EnthalpyH= E+ PV.
(v)HelmholtzfreeenergyF = E- IS.
(vi)Gibbs freeenergyG
= H- IS,
(ii) Gullstrand equation:
(a)Effectivepower:
P = P, +
p,
(b)Fronfvertexrefractingpower:
P. -P. +
P
. t. ,
n
p r. d
n
(c)Back-vertex refractingpower:
P. - P *
q
. o. ,
n
q. d
n
' - n
SkBT
nn
PC1142Physicsll
Part1 Answer allFIVE
questions. Allquestionscarry 8 markseach.
centimetre.Thesehavea root-mean-squareSpeedof 1400 m s-1.
[Nofe:
H hasan
atomicweightof1,
g mol-t anda diameterof1.0A.l
(i) Compute themeanfree
path oftheseHatoms,
(ii) Compute theirkinetictemperature.
andhavinga uniformtemperatureI', surroundedbya thermally-insulating solid shell
of
thicknessd withthermalconductivityk,asshownbelow.Heat isproducedinternallyinthe
coreata rateof P. Derive anexpressionforthevalueof I, atsteady state,intermsofP,
k,16,d,andothernecessaryconstants.
vacuum
1,0kgof helium
gasis heatedatconstant
pressure
from 300 K to600K. Computethe
changeinentropy ofthe
gas.[Nofe: Hehasanatomicweightof4.0g moFt,]
theopticalimageof theground fromanaeroplane flying10kmaboveground. Canthis
cameraresolvea carontheground, if thelens systemis freefrom aberrations,basedon
Rayleigh'scriteria?
[Nofe:
The opticalspectrumspans 450-650nm.]
components of a polarisedbeam.One suchwave
plate ismade ofbirefringent crystalline
quartz withanordinary refractiveindex(no) of 1.5426andanextraordinary refractive index
(ne) of 1.5517at a wavelength of632.8nm,and orientedasshown below.Thefast axis
hastheindex no,whiletheslow axishasindexnr, The thicknessof theplateis 1.00g
mm.
A linearlypolarised beamof 632.8-nm lightis incident normallywiththe plane of
polarisation
at anangle0 measured clockwisefromthefastaxis.Compute thephase shift
between lhecomponent
polarised parallel tothefastaxis andthat
polarised parallel tothe
slowaxis,andgive thestateofpolarisation after
passing thiswaveplate.
for imagingapplications.An achromat(general structureshown below)consistsof a
positivelow-index crown
Elass
lenselementwithradii of curvature h ?ndh, andcentre
thickness fcr,ceffiertodto a negativehigh-indexflintglass lenselementwithradil of
curvature h and
rl, ?fldcentre thicknessfcz.Theselens elementsarechosen so asto
cancel chromaticabenationat the red (630-nmwavelength) and blue(450nm)
wavelengths.Onesuchachromat hasa diameterof 6.35mmandis constructedwithrr
8.609mm,rz=-5,134mm,ta = 2.7mm, andtcz
0] mm. lt hasaneffective focallength
of 12.7mmat 589-nmwavelength.Therefractive indexforthecrownglass usedis
1,52andforflint
glass is 1.66at thiswavelength. BFL
= back
focallength, FFL
= front
focallength.
(i) Compute thevalueofrr inthethin-lens
paraxial ray approximation.
[8marks]
(ii) Compute thelateralmagnificationoftheimage ofanobjectlocated12, minfront
ofthelens,
(iii) Brieflyexplainthemeaningof
"chromatic
aberration"
[8marks]
[4marks]
superposition oftheindividualwaves.
(i) Considerthesuperposition of twomonochromaticcoherent
plane waves with
amplitudes0r ?fldazrospectively, and
phases
0r
and
$zrespectively,
Showthat
theintensityoftheresultantwaveisgivenby:
I = 11+t2 +2r[tfucosA, where 4 =
Q
[Bmarks]
Considernowthatthesetwowaveshave equalintensities/0,buttheytravelatan
anglewitheachother.Onewavetravelsalong the+z-direction,whiletheother
wavetravels at anangle0 withthez-axisin thexzplane,asshown below.Atthe
overlaponthexyplane,a sinusoidal
pattern ofbright anddarkfringesisformed.
(a) Show thatthephasedifferencebetweenthetwowaves measuredalongx
varies accordingto A = x4sing
t8marksl
(b) Fromthe resultof (i) aboveor othenruise,derive the equationthat
describestheintensityvariation inthex-directionofthisinterferencepattern.
[4marks]
(ii)