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5:23 AM
@JohnRennie good morning. You free
 
@harambe morning :-)
I'm just going to make a coffee then I need about 15 minutes to do some work.
 
Okay. See you around an hour
 
ayc
@JohnRennie morning!..Are you free?
 
@ayc in about 15 minutes ...
 
ayc
@JohnRennie I'll be waiting ..Just ping me
 
ayc
5:58 AM
@JohnRennie This is my question:we know that magnetic field does no work on a charge moving with constant velocity.So the speed of the particle remains constant.But its velocity vector changes.That means it is accelerating.In this case,since the charge is undergoing an acceleration would it emit EMW?
 
@ayc yes. This type of radiation is known as Bremsstrahlung or synchrotron radiation. For example accelerators like the LHC emit this type of radiation when they use magnetic fields to make particles go in a circle.
 
ayc
@JohnRennie Oh yeah.We talked about it yesterday.I forgot
 
@ayc actually I had forgotten as well :-)
 
ayc
@JohnRennie See you with a new doubt.Thank you !
 
6:19 AM
@JohnRennie hi. Are you free now
 
@harambe yes
 
Q34
I set mv^2/4=10.2eV
I converted every to joules and tried to get the answer
But it's not matching.. Is this correct
 
This is basically the same as that neutron-H atom problem we looked at yesterday.
The ionisation energy is 13.6eV, so in the COM frame the collision energy has to be 13.6eV i.e. the KE of the atoms has to be 6.8eV.
OK so far?
 
Wait I was using excitation energy instead of iionisation energy
I get my mistake
@JohnRennie can't we use total kinetic energy of the atoms to be 13.6 ev
And calculate velocity from there
 
No. Can you guess why not?
 
6:31 AM
Some energy is used in excitation energy
 
The collision must conserve momentum.
 
Okay
 
That means atom A cannot come in with energy 13.6eV, ionise atom B and come to a halt. That would not conserve momentum
The requirement that momentum be conserved places a constraint on how much of the incoming atom's energy can be used to ionise the other atom.
This is why it is best to work in the COM frame then transform back to the lab frame for the final result.
In fact the problem is trivially easy if you do it that way ...
 
@JohnRennie So I write the total kinetic energy is coming frame
And then equate it to 13.6 ev
 
is coming is your phone autocorrect of in COM ?
 
6:35 AM
Yes....
COM frame
 
Look at it this way ...
If the incoming atom has a speed $v$ then in the COM frame the two atoms have speeds $+v/2$ and $-v/2$. Yes?
 
Yes
 
And KE is proportional to v^2 so in the COM frame the KE of the incoming particle is 1/4 of its value in the lab frame.
 
Yes
 
Now, in the COM frame the total momentum is zero, so the two atoms can come in with equal and opposite speeds, use all their KE to ionise one of the atoms and come to a stop. This conserves momentum so it is allowed. So in the COM frame the minimum total KE is 13.6eV.
 
6:39 AM
Yea
So I calculate velocity now and convert it into lab frame
 
That means both atoms have a KE of 6.8eV, and we've just worked out that in the lab frame the KE of the incoming atom is four times greater i.e. 27.2eV.
 
Ok
 
So you can just use $\tfrac{1}{2}mv^2 = 27.2eV$ in the lab frame.
 
Got it
 
Not that only half the KE can be used to ionise the atom. That's the conservation of momentum imposing a constraint on the collision.
 
6:45 AM
How did you conclude half
 
The initial KE is 27.2eV. Half of this, 13.6eV, is used to ionise the atom, and the remaining 13.6eV goes into the KE of the atoms after the collision.
 
@JohnRennie Finally I also got the answer
 
@harambe cool :-)
 
@JohnRennie in inelastic collision, only momentum is conserved and we can't use energy equation right
 
@harambe correct
Well, energy is still conserved but you have to count all the energy including the energy that goes into exciting the atoms or whatever.
So you can still use the energy equation provided you count all the energy. Just counting the KE won't work.
 
6:54 AM
Okay
@JohnRennie Quoting from wiki
In nuclear physics, an inelastic collision is one in which the incoming particle causes the nucleus it strikes to become excited or to break up
Does that mean all inelastic collisions in nuclear physics, the kinetic energy is spent in exciting the atoms
 
Energy is always conserved, so if energy "disappears" in a collision then that energy must be going somewhere. The question is where can the energy be going?
In the case of something colliding with a nucleus the only place energy can be going is into exciting the nucleus.
 
What about ionising
 
You don't ionise nuclei ...
 
Oh lol
Got it
 
Don't confuse atomic collisions, like the problem we've just done, with nuclear collisions. Excitations of nuclei happen at energies of many MeV while for atoms it's at most a few keV for the innermost electrons in heavy atoms.
 
7:10 AM
@JohnRennie the atomic collisions we have discussed till now we're all inelastic, right
 
@harambe yes. An elastic collision is one in which the total final KE is equal to the total initial KE. If some KE gets used up in exciting or ionising atoms then by definition that collision is inelastic.
 
Q35
The collision is inelastic when kinetic energy is spent in exciting
The excitation energy is 10.2 eV
And the frame is COM too
 
Yes, so the question is very easy.
 
So the atoms can stop and it will not affect the momentum
Got it
@JohnRennie got the answer but why have they written the collision may be inelastic or perfect
Can the collisions vary between perfect or non perfect
 
A partially inelastic collision is one in which some but not all of the KE is used to excite the atom. A completely inelastic collision is one in which all of the KE is used in exciting the stom.
 
7:44 AM
@JohnRennie in. Photo electric experiment, the electrons that are ejected due to incident light gain kinetic energy because of incident light. Does this mean all electrons near the surface come out with kinetic energy equal to the energy provided by incident light on metal or can the electrons still lose energy even if itnis near the surface
 
The PE experiment is more complicated than it appears at first sight.
When a photon produces a photoelectron that electron is travelling in the same direction as the incident photon i.e. downwards into the metal.
 
Okay
 
For a photoelectron to be ejected from the surface the initial electron has to collide with something and rebound back towards the surface. Or it might transfer its energy to a different electron that then escapes the surface.
This is a rather improbable event, and in fact the vast majority of the initial photoelectrons never escape. Only about one in a million, or at best 1 in 100,000, photons actually produces a photoelectron from the surface.
 
Okay but what about the free electron of the metal
They can gain energy from photon collision.. I read this in my textbook
 
By free electrons I assume you mean the electrons in the conduction band, and yes for visible light all the photoelectrons come from the conduction electrons.
But my previous statement still holds. When a photon transfers energy to a conduction electron conservation of momentum means that conduction electron starts moving in the same direction as the photon.
 
7:53 AM
Okay
 
Anyhow, the collisions involved in making the electron bounce back towards the surface are partially elastic to some extent. That means some or all of the energy of the photon can be lost in those collisions.
The result is that the photoelectrons that come from the surface have a range of kinetic energies from a maximum of $h\nu - \phi$ right down to zero.
 
What does this $h\nu - \phi$ represent here
 
$h\nu$ is the energy of the incident photon and $\phi$ is the work function of the metal.
 
Okay
@JohnRennie Why is The frequency of the photon with energy equal to work function is called threshold frequency.
 
If we take the PE outside the metal to be zero (as usual) then the topmost electrons in the metal lie at an energy of $-\phi$. That is is always costs an energy $\phi$ to remove an electron even if we don't give the electron any KE at all. You can think of $\phi$ as being the ionisation energy of the metal.
 
8:03 AM
Okay
 
That means if $h\nu < \phi$ the photon cannot eject an electron, just like photons with an energy less than 13.6eV cannot ionise a hydrogen atom.
 
@JohnRennie that would explain my previous question too
Okay
 
Ah, sorry, I didn't realise you hadn't done the work function yet.
 
@JohnRennie even if energy of photon is greater than work function, what if by the time it reaches the surface electron, it's energy gets reduced below work function due to succesive collisions with other electrons
 
@harambe I think, but don't know for sure, that the most probably scattering event for the photon is to transfer all its energy to an electron in one go. So as a general rule photons don't get partially scattered and lose a bit of energy before their final collision.
 
8:10 AM
Okay. Got it
In the graphic of current vs frequency, why are they independent
Greater frequency means more electrons will come from surface of metal
With more energy of course
 
Remember that as long as the frequency is above the threshold one photon = one photoelectron. If you change the frequency but keep the number of photons constant then the number of photoelectrons will be constant.
NB in most PE experiments the current just measures the number of photoelectrons per second. The current is not dependent on the photoelectron energy.
 
Okay got it
 
That graph is actually rather misleading.
If you keep the intensity constant then the number of photons per second decreases as we increase the frequency. This is simply because each photon has more energy, $hf$, so for a fixed energy higher $f$ means fewer photons.
 
8:26 AM
@JohnRennie didn't get it
If frequentcy is increased then photos will have more energy. How will this relate to intensity which depends on number of photons
 
Suppose we keep the light intensity constant as we change the frequency. The intensity is power per unit area i.e. joules per second per square metre.
So the number of photons per second per square metre is the intensity divided by the photon energy $hf$.
 
Oh okay
 
That's why graph C is a bit misleading. The obvious way to do the experiment would be to keep the intensity constant as you increase the frequency. If you do that then the current will be proportional to 1/f.
The graph must be keeping the number of photons per second per unit area constant i.e. it is increasing the intensity as the frequency is increased.
 
 
1 hour later…
9:38 AM
@JohnRennie absorbing photon is a positive work or negative
I think positive because energy is increasing
 
I'm not it's really work in the usual sense of the word.
 
Okay
 
9:52 AM
Q4
I found the energy of the photon
Then I divided it by the power
Didn't get the answer.. Am I missing something
 
Well, you divide the power by the photon energy not the other way around. I assume thats what you meant.
What did you take as the power?
 
Yea I divided power by energy
10 W
 
So I should do 60 percent of energy or power
 
The lamp consumes 10W of electricity, and it is 60% efficient, so the power of the light produced is 10 x 0.6 = 6W.
 
9:58 AM
Okay so the photon is the energy emmited front this energy?
Electric energy I mean
 
Yes. Divide 6W by the photon energy to get the number of photons per second.
 
Got the answer
 
Cool :-)
 
How to calculate for cubic metere
 
The first step is to calculate the number of photons emitted per square metre per second at the Earth's surface.
 
10:11 AM
Intensity/Energy
 
Does that say Earth's surface? You managed to get the word PRO right over it.
 
Yes
It says earth
 
OK, so you calculated the number of photons/sec/m^2 in part (a). Yes?
 
Yes
 
In one second a photon travels $c$ metres, so in one second the contents of a volume 1m x 1m x c metres of photons hit every square metre on the Earth. Yes?
 
10:15 AM
Yes
@JohnRennie on second thought I can't visualise it
 
Consider a box 1m x 1m x c metres standing on the Earth. Every photon inside that box will hit the Earth in the next second.
 
Okay
 
And only the photons inside that box can hit the Earth in the next second, because any photon farther away than $c$ metres will take more than a second to reach the Earth.
 
Okay
 
So all the photons that hit a square metre of the Earth in on second fill a box of volume 1 x 1 x c.
 
10:21 AM
Okay
 
In part (a) you calculated the number of photons per second per square metre hitting the Earth. Call the number $N$. All these $N$ photons are contained in a box of volume 1 x 1 x $c$, so the number density (number of photons per cubic metre) is $N/c$.
 
Got it
@JohnRennie doubt
 
@harambe yes?
 
Sun light from sun takes roughly 8 minutes to reach earth. How would photons travel there in 1 sec
With speed c
 
I wasn't counting all the photons in transit between the Sun and the Earth. I was only counting all the photons in a box of height 1 light second above the Earth.
 
10:34 AM
Okay got it
 
10:49 AM
@JohnRennie (c)
I multiplied intensity by area of earth
Then divieded that by energy of photon
Answers not matching
 
The question asks how many photons per second the Sun emits, not how many photons per second hit the Earth.
 
Oh dang
 
I sure it's not really necessary to say, but it is important to read the question carefully. In the exam you don't have someone like me around to correct you.
 
Yes you are right.
@JohnRennie any idea how to solve this part then
I can't seem to think one
 
11:05 AM
@harambe you've already calculated the number of photons per square metre per second at the Sun Earth distance. Yes?
 
Yes
 
How many square metres are there at the Sun-Earth distance?
(it's not a trick question)
@harambe hello?
 
Thinking
 
@harambe Call the Sun-Earth distance $r$. What is the surface that is everywhere a constant distance $r$ from the Sun?
 
Eh?
Am I supposed to say earth's surface
 
11:12 AM
We are asked to find the total number of photons per second coming from the Sun. So if we consider a surface around the Sun with the Sun at the centre we just just have to work out how many photons per second pass through this surface.
OK so far?
 
Ok....
 
And the total number of photons per second passing through the surface will be the number of photons per square metre at the surface times the area of the surface.
 
Yes
 
Like that, where I've just drawn some random surface with the Sun in the middle.
(the Sun is the yellow circle)
But calculating the area and the photon intensity for a random surface like that is going to complicated. It would be far easier if it was a more symmetrical surface ...
 
Like sphere
 
11:19 AM
Yes, like a sphere. Maybe a sphere with a radius equal to the Sun-Earth distance since we have already calculated the photon intensity at the Sun-Earth distance ...
 
Okay
 
11:35 AM
@JohnRennie got it
 
@harambe Cool :-) The idea is simple when you've been introduced to it. The same technique is used extensively in electrostatics where we call the surface a Gaussian surface.
 
Yeah
 
12:34 PM
Q20
Can you explain to me what does does electric field do here
 
Light, or indeed any EM wave, is an oscillating electric field. So when the question talks about the electric field going to zero this is just a complicated way of telling you the frequency of the light.
 
@JohnRennie de broglie wavelength is associated with particle nature or light behaves as particles
And einstein gave wave nature, right
 
I'm not sure what you are asking
 
Leave that xd.I was actually trying to ask something weird
 
If you're wondering about wave particle duality then it's a surprisingly simple idea but it requires you to have a basic grasp of quantum field theory.
 
12:42 PM
@JohnRennie quantum field theory is in the course major physics students, right
 
@harambe it's usually an option that the mathematically inclined students might want to in their final year of a degree. QFT is really hard to understand rigorously. The maths involved is super scary. However it's not too hard to get a rough idea of what is going on.
 
@JohnRennie is schrondinger equation also solved in QFT
I remember my teacher saying the math required 1-2 day solving
 
No, the Schrodinger equation is non-relativistic quantum mechanics and it's actually not that hard. Most JEE students will have enough maths to be able to handle it.
Quantum field theory is a whole new level of complexity!
If you did physics at university you would study the Schrodinger equation as a first year course.
 
Sid
@harambe You will study Schrodinger's equation in first semester
(Of any University)
 
@Sid okay. I wonder why my teacher said that then
 
Sid
12:53 PM
@harambe They probably didn't want to consume valuable time explaining you guys about it.
 
@harambe even basic QM involves some ideas that are hard to get your head round. The maths isn't that hard but the concepts are.
Actually the same is true of special relativity. The maths is just basic calculus and JEE students will know this. But the ideas involved are very ... erm ... odd! :-)
 
Sid
(You will also read about Special relativity in first year of any Uni)
 
Wow. There is a chapter on special relativity in hcv too
 
Beware of "one chapter" introductions to special relativity as they tend to oversimplify.
 
@JohnRennie got it
 
ayc
1:40 PM
anyone?
 
1:59 PM
Hello, anyone? @JohnRennie or @sammygerbil
 
2:11 PM
First doubt, when Pn junction diode is reverse biased, the voltage is along the direction of electric field of the depletion region. Then why does the 'voltage drop across the depletion region'?
This is what is given in my book.
 
 
2 hours later…
3:49 PM
@Blue Hi, are you free?
 
Anonymous
Does this help?
 
Anonymous
@Dante Unfortunately not. If you have any specific question, ping me with it. I'll try to answer it by tomorrow.
 
Ok, unfortunately I don't have any specific question.
But thanks for the video!
 
4:28 PM
I have a small doubt in errors and measurements. The statement says:
For example, in the experiment on finding the focal length of a convex lens, the object lens(u) is found by subtracting the positions of the object needle and the lens. If the optical bench has a least count of 1 mm, the error in each position will be 0.5 mm. So, the error in the value of u will be 1 mm. The doubt I have is, how is error in each position 0.5 mm? Isn't the error directly the least count(unless otherwise mentioned). So, 1 mm + 1 mm = 2 mm for (u).
 
@sammygerbil Please ping me when you are here for problems.
@Dante its given properly in RnH too.
 
Hmm, I don't have unfortunately :/
 
@Dante its given in HCV to
 
I see, I read it from NCERT, not clear enough, will read it in HCV now.
 
 
1 hour later…
5:40 PM
@JohnRennie hi!
 
@EshaManideep hi
 
I have this question, I have a laser light run by some solar cell, but I now I focus the parallel beam onto a parabolic reflector which converges the light rays to a very small point, and now I can put an object at that focus and heat it to whatever temperature I can by reducing the area, ultimately greater than that of sun, the against SLT.
What is wrong with my argument??
 
9
A: Is it possible to focus the radiation from a black body to make something hotter than that black body?

anna vIf you use complicated routes redefining "focusing" towards generating the temperature, yes. Physicists at CERN's Large Hadron Collider have broken a record by achieving the hottest man-made temperatures ever - 100,000 times hotter than the interior of the Sun. Scientists there collided...

 
As your object heats up it starts emitting light. The same lenses that focussed the light from the Sun (or whatever) send the light from the object back to the Sun. The end result is that the fraction of light from the Sun that goes into heating the object decreases as the object gets hotter.
 
@Abcd Available now (but going out for about 30 minutes in 1 hour.)
 
5:51 PM
@JohnRennie Alright, do u remember a question I asked u few days ago about focusing sun rays through a lens....
 
@EshaManideep sorry, no.
 
@sammygerbil A parallel beam of sodium light of wavelength $5890 $ A is incident on a thin glass plate of $\mu = 1.5$ such that angle of refraction is $60^\circ$. The smallest thickness of the plate which will make it dark by reflection is?
@JohnRennie Do you know about resolving power of optical instruments?
 
@JohnRennie Alright let me send the question again.
 
@Abcd possibly, it depends on exactly what you want to know.
 
@JohnRennie i will ask in morning coz you are going rn probably?
 
5:55 PM
Yes, I'm going soon. I'll be around as usual tomorrow.
 
Sun rays are focused with a lens of diameter d and focal length f to the black side of a thin plate. The one side of the plate is perfectly black and the other side is perfectly white. Angular diameter of the sun is aloha and it's intensity on the surface of the earth is I. I using thermodynamic arguments find the maximal focal length-to-diameter ratio of a lens.
 
@JohnRennie i cant understand my textbook, there are no good youtube videos on it. Thats why i need to understand the concepts and stuff. (tomorrow)
@sammygerbil The unusual part of the problem is that in all problems I have done so far, incidence and refraction, reflection was normal
@sammygerbil Given the $\mu$, Isn't 60 degree a very large angle of refraction?
 
I did this one by finding the image diameter and equating the images area into t^4 to the power falling on it and the temperature of it equalling the sun
 
OK ...
 
Wait,...
Nonsense 😂, ignore it. I sorry for wasting your time
 
6:01 PM
No problem :-)
 
@Abcd Yes it is too big. Maximum angle of refraction should be 41 degrees (=critical angle).
 
@sammygerbil Is the problem wrong?
@sammygerbil when I used snell's law , sin i was coming out to be greater than 1 which aint possible
 
@Abcd Yes. That angle of refraction cannot happen. The question is faulty. Probably not worth continuing with it.
 
@sammygerbil one more
@sammygerbil I tried 20th three times in exam and got answer as $2\sqrt 2$, can you please see what answer you are getting?
 
@Abcd (You could change the angle of refraction to something physically possible, and see if you can solve the problem then. You will not be able to match the answer given, but you can still learn from the problem.)
 
6:09 PM
@sammygerbil let me try 20 again in front of you
See:
 
@sammygerbil one of my batchmates claims to have got the answer w/out calculating sin i
@sammygerbil he also says incidince angle isnt needed to solve it
20:
$R = \lambda N$
$N = N_o e^{-kt}$
$\lambda =\dfrac{\ln 2}{t_{1/2}}$
$\implies \lambda_1 = \dfrac{\ln 2}{2}$
 
@Abcd Ask for his solution.
 
$\implies \lambda_2 = \dfrac{\ln 2}{4}$
$R_1 = \lambda_1N_o e^{- \ln 2}$
$R_2 = \lambda_2 N_oe^{-ln 2/ 2} $
$\lambda_1 / \lambda_2 = 2$
$R_1/ R_2 = 2 e^{- \ln 2/ 2}$
$R_1/R_2 = \dfrac{2}{\sqrt 2}$
$R_1/ R_2 = \sqrt 2$
Damn ittttttttttttttttt
Why doesnt it come in the exam hall.
@sammygerbil Problem 17 please
Dont know how to solve that one.
Language of question aint clear.
 
@Abcd Use the Lens-Maker's Equation?
 
6:24 PM
@sammygerbil whats the diagram, language isnt clear to me'
 
Lens has air on one side, water on the other. Rays which are parallel on the air side come to a focus in the water. Where is that focus?
 
@sammygerbil He sent this to me^
Me: Send solution
He: It's hidden somewhere here *laughing emoji* (sic)
@sammygerbil His solution on the bottom right corner, you can see $2\mu x = \lambda$ stuff there.
@sammygerbil I think I can see his mistake, he is considering it normal incidence on the glass surface, isn't he? But the path difference would change for $60^\circ$ refraction angle
 
@Abcd I wonder if he gave the examiner the same solution...
 
@sammygerbil We aren't supposed to get the solutions checked or show them to anyone. We just have to mark the right answer and move ahead in online mode. And bubble the circle in offline - OMR mode... That's why tricks and stuff work and help a lot
@sammygerbil Have I spotted his mistake correctly?
 
@Abcd Don't know, can't read it.
 
6:32 PM
@sammygerbil let me rotate and send
@sammygerbil clear now^ ?
 
@Abcd I can see working for several questions there, but not #17.
 
@sammygerbil let me circle and send lol
 
@Abcd I need to go out now. Back in about 30 mins.
 
@sammygerbil please ping when back
 
6:56 PM
my question got shut down
im not sure why
-2
Q: Orbit velocity satellite question, is this question ill defined

johnI am attempting to solve this question but I feel that the question may be ill defined. The question is in two images, the first image and second image. I have tried many attemps at this but nothing seems to make sense. The question seems to be talking about entering an orbit starting from the su...

i wasnt asking for an answer, just a direction
the question could be ill defined, thats all i wanted to know. jeez, why was it put on hold
thanks for all the help
 
@Abcd back
 
@sammygerbil I think user John's messages are better suited for h-bar. Please move them there so that his plea can get some attention.
oh no, he has posted the same thing in both rooms
so leave it
 
7:12 PM
@Abcd I think it is suitable for this room.
 
@sammygerbil well, he was asking the reason why his question was put on hold, not a solution to his problem so I thought...
 
7:25 PM
@john Re: why the question was closed. The main site is not a Problem Solving Site. It is intended for conceptual questions only (although algebraic calculation questions sometimes get through if they are interesting). You failed to identify a conceptual difficulty.
@Abcd True, the issue of why the question was put on hold would be better in the h-bar. But I think @john has posted here to get an answer to the question which was closed. ie What (if anything) is wrong with his calculation?
 
@sammygerbil Ok,please see interference question now
 
@Abcd Your benchmate has not used normal incidence in his calculation. The rays which are reflected from the upper and lower interfaces are parallel and interfere destructively if they are in anti-phase. There is a phase difference due to the different optical path lengths, and there is a phase change on reflection from the upper surface (but not the lower).
 
7:46 PM
However, for the same reason that the angle of refraction cannot be 60 degrees, the ray which is reflected from the upper surface cannot emerge from the flat plate - it is incident at greater than critical angle, so it suffers total internal reflection at the upper surface as well as at the lower surface.
Correction : You are right. He has used normal incidence.
Suppose the light is incident at angle $i$ and refracted at angle $r$. Then $\sin i =n\sin r$.
Suppose the thickness is $t$ and the distance between points at which one ray enters and emerges from the plate (after reflection from the bottom face) is $d$. Then $2t=x\cos r$ and $d=x\sin r$ where $x$ is the path length of the ray in the glass plate.
 
8:07 PM
@sammygerbil he says that he has not used normal incidence
@sammygerbil he says that x is slant length only
 
@Abcd ok. I don't follow what he has done.
 
@sammygerbil he has an argument for angle of refraction too
@sammygerbil he says that medium 1 is not specified.
but we took it as $\mu_1 = 1$
 
 
1 hour later…
9:35 PM
@sammygerbil still here?
@sammygerbil The amplitude of electric field of an EM wave travelling along z axis is 2 V /m. The average magnetic field is:
A) 13.29 * 10^-12
B) 8.86 * 10 ^-12
C) 17.72 * 10^-12
D) 4.43 * 10^{-12}
@sammygerbil am getting C using $\dfrac{1}{2}\epsilon_o E^2$
But Answer is B
 
@Abcd A factor of 2 difference...
How are you using $\frac12 \epsilon_0 E^2$?
 
@sammygerbil energy density of magnetic field = energy density of electric field in EM wave
 
@Abcd So what relation have you got between $E$ and $B$?
 
@sammygerbil $E = Bc$
@sammygerbil aint that relation useless here, why do you need it
 
@Abcd I don't know, but I don't see how you got your answer from it.
 
9:48 PM
11 mins ago, by Abcd
@sammygerbil am getting C using $\dfrac{1}{2}\epsilon_o E^2$
@sammygerbil I got my answer as option C using this^^^
$u = \dfrac 12 \epsilon_o E^2$
Then I used:
5 mins ago, by Abcd
@sammygerbil energy density of magnetic field = energy density of electric field in EM wave
 
@Abcd What is your calculation?
 
@sammygerbil sorry question has average density of magnetic field
@sammygerbil Now happy? ^^^
@sammygerbil Note that $\epsilon_o = 8.85 \times 10^{-12}$, $E= 2$
 
@Abcd Yes.
Just trying to refresh my memory on this topic.
 
@sammygerbil I think E in formula is not $E_o$, :(
otherwise it would mean $E_o$ all the time in space
which aint true.
E_o is oscillating
from symmetry we should add a factor of 1/2
or $E \to E_{rms}$
@sammygerbil Now am I correct, and is the use of symmetry correct?
 
@Abcd $E$ is amplitude I think. I don't follow your symmetry argument.
 
9:58 PM
@sammygerbil $E_o$ means amplitude
2 mins ago, by Abcd
@sammygerbil I think E in formula is not $E_o$, :(
2 mins ago, by Abcd
otherwise it would mean $E_o$ all the time in space
@sammygerbil Proof that E is not amplitude^ . What do you say about it?
 
@Abcd I don't follow this reasoning.
 
05:00 - 22:0022:00 - 23:00

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