What accelerating voltage would be required for the electrons of an electron microscope if the microscope is to have the same resolving power as could be obtained using 100 keV gamma rays?
Assuming the minimum resolvable feature size is same as the `wavelength` of the light used in the microscope, I think this problem is about finding the required potential difference that builds up the corresponding wavelength for the electron...
Yeah I think you're right about that. I'm sorta in the middle of working some linear algebra stuff but I'll try to help in a few minutes if no one else comes to the rescue haha.
what i don't get is how the kinetic energy of gamma rays matters here wavelength of gamma rays shouldn't matter on the kinetic energy right ?
Well gamma rays is sorta a range of energy, there's not just one single wavelength that is gamma radiation. It's exactly the same reason why there are multiple radio stations, even though they're all using radio waves.
what does it mean to say ` 100 keV gamma rays` i know `100 keV electron` has a kinetic energy of `100keV`, but how to think of the same for gamma rays ?
There's really only one photon, but the photon can have different frequencies and polarizations. I think it becomes confusing because people think the speed of light is constant but frequency can change and that also seems to be like a speed. But the difference is like you're driving a car at a constant speed and the passenger is jumping up and down in their seat either faster or slower which is the frequency aspect of the photon.
for a photon of given frequency, the energy is fixed right ?
what does it mean to say ` 100 keV gamma rays` ?
They didn't have to say "gamma rays" they could have said 100 keV light and that would have been exactly the same. It's a little redundant but they're just trying to make you associate high energy with the waves in that region of the spectrum.
Ahh okay, gotcha! so the photon has an energy 100keV from this i can calculate the wavelength, nice :)
Alright I guess we should look at the de Broglie wavelength. There are two sorta nice ways to memorize it as a clump of stuff. \[p=\frac{h}{\lambda}\] There's the clear analogous formula: \[E=h \nu\] And then there's also the fact that you probably know the Heisenberg uncertainty relation \[\Delta p \Delta x \ge \frac{\hbar}{2}\] Knowing the units here, you can immediately feel assured that you have the debroglie relation correct since \(\lambda\) is wavelength and has units of distance and so does \(\Delta x\) by comparison. In spectroscopy we tend to use wavenumbers which are to wavelength as what frequency is to period, and that makes the equations look much more symmetric looking. We define wavenumbers as: \[\tilde \nu = \frac{1}{\lambda} \] Also, I'll include the angular versions since I think they are found a lot as well. \[p=h \tilde \nu = \hbar k\]\[E=h \nu=\hbar \omega\]
\(\lambda \approx 12.4pm\) looks good ?
That sounds pretty good, since gamma rays are high energy, they should have very short wavelength.
defining \(1/\lambda\) by a different variable looks nice...
then the electron must be accelerated a kinetic energy such that its wavelength becomes \(12.4pm\)
Yeah, normally it's written that way it means it has units of inverse centimeters. Literally you can understand wavenumbers as "number of waves per centimeter" since wavelength is normally "centermeters per length of wave". Sorry for the delay I got sidestepped thinking about the photoelectric effect but I realized we're using voltage to eject electrons not photons haha.
Nice, we're using voltage to accelerate already existing electrons i think...
Well alright so let's continue on, energy is just like we'd expect for an electron classically. It's on the plate and we gotta accelerate it off. So it has no kinetic energy from the start and it ends up with kinetic energy. There's gonna be a change in potential energy which is proportional to the change in voltage, since voltage is joules per charge. \[U_i+T_i = U_f+T_f\] I just explained :\[T_i=0\] and \[U_f-U_i = q\Delta V\] So we have: \[q\Delta V = T_f = \frac{p^2}{2m}\]
can i use the classical equation p^2/2m = KE ?
so when the electron goes through that potential difference, it gets the required kinetic energy
il plugin the numbers, one sec..
I hope it works, I'm gonna be right back real fast gonna make some tea.
\(p = 5.34*10^{-22}\) http://www.wolframalpha.com/input/?i=%286.62607004+*+10^%28-34%29%29%2F%281.24*10^%28-12%29%29
\[\Delta V = \dfrac{p^2}{2em} \approx 977kV\] http://www.wolframalpha.com/input/?i=%285.34*10^%28-22%29%29^2%2F%282*1.60217662*10^%28-19%29*9.10938356+*+10^%28-31%29++%29
I'm getting roughly 3.89 pm for the wavelength: http://www.wolframalpha.com/input/?i=(plancks+constant)%2Fsqrt(2*(mass+of+electron)*100keV)
Whoops I've done it backwards haha. I see what I've done, I plugged in the energy of the gamma ray looking for the wavelength but I need to find the energy given that the wavelength is the same haha.
No wonder I felt so backwards in plugging it in, so to clarify the general flow I should have gone through (which I'm just gonna assume you've done correctly) is: energy of photon -> wavelength of photon -> wavelength of electron -> energy of electron
hey should i treat 100keV as kinetic energy K = p^2/2m or the actual energy E = hf ?
correct answer is 9.76 kV hmm
im missing a 100 somewhere in my calculation..
Here, I think I confused you. You should treat it as E=hf since it's the energy of light. A microscope's resolving ability relies on the wavelength of the particles you shoot at it, whether they be photons or electrons. So first off, I'll call light energy as \(E_\ell\) to distinguish it from the electron energy \(E_e\). \[E_\ell = \frac{h c}{\lambda_\ell}\] In order to maintain that both the microscopes have the same resolving ability, \(\lambda_\ell = \lambda_e\) so now we can start to solve for \(E_e\) in terms of \(E_\ell\). From now on I'll just refer to the wavelength as \(\lambda\) since they are identical, that's the point of this problem. \[E_e= \frac{p^2}{2m} = \frac{h^2}{2m \lambda^2 }\] We can get \(\frac{h^2}{\lambda^2}\) from the light energy equation to make it a breeze to plug in. \[\frac{E_\ell^2}{ c^2} = \frac{h^2}{\lambda^2}\] \[E_e = \frac{E_\ell^2}{2mc^2}\] The takeaway from this problem is that \(c^2\) in the denominator is a huge number so correspondingly the energy required to make an electron microscope of the same resolving ability as a light microscope is MUCH less.
http://www.wolframalpha.com/input/?i=100keV%2F(2*(mass+of+electron)*(speed+of+light)%5E2)&t=crmtb01 Yeah I think I am missing some powers of 10s somewhere
Well, the weird thing is that the answer WA gives me has no units attached wtf
by that reasoning electron microscope is better than the corresponding light microscope of same resolvability
your derivation looks fine to me, il check why we are not getting the textbook answer...
In practice, that's not exactly true shooting photons and shooting electrons at things can have some pretty different results. But yeah electron microscopes are awesome lol.
can we really use gamma rays in microscope to see fine details of say some metal surface ?
Of course. How do you think we figured out the structure of DNA?
I actually really love the structure of DNA's from x-rays it has such a beautiful explanation. But x-rays are weaker than gamma rays, and I don't know about gamma rays since I only worked in an x-ray lab. I think gamma rays are so high energy it would be impractical though @ganeshie8
interesting.. so ppl are using gamma rays in microscopes is it, nice..
what kainui said is true; x-rays are much softer than gamma rays, so they are not one to one, but they turn out to be enough...
are you talking about x ray diffraction ?
x-ray crystallography actually, which is similar
applied x-ray diffraction
Ok guys I think you really need to learn this because this is probaly the most amazing thing I've ever learned when I was working in an x-ray lab. https://upload.wikimedia.org/wikipedia/en/b/b2/Photo_51_x-ray_diffraction_image.jpg and now look at the spring on the far left. http://www.yamahapart.com/Assets/YamahaPart/Images/workshop/suspension_principles/6_1_1_3_1_PS_gc_single_col.jpg Now if you see in the spring there is \\\\\\ and ////// These are the diffraction gratings of DNA's helix that forms the X pattern in the first picture.
my textbook says we need to use some crystal structures to see the diffraction phenomenon of xrays as we can't physically make apertures small enough for xrays to diffract..
if i understand correctly, in xray lab, you ppl are using DNA structure itself as a diffraction grating for xrays to diffract ?
by studying the distance between interference fringes etc you're guessing the actual structure of the DNA.... fascinating! idk how much nonsense i have talked in past two replies based on my bookish knowledge lol
Yeah, the zigzag you see from the profile of a spring is a pair of diffraction gratings and that's what we, human beings, did to figure out that we're made up of these little helices.
its so cool ! can u recommend any document that explains xray diffraction in a simple manner ?
i mean the applications of xray diffraction, like, to study crystal structures etc... my textbook really did a good job explaining the basics of xray diffraction, but it didn't bother to go through any applications..
Hmmm well you can study solid state chemistry from a physical chemistry textbook. I guess I should tell you, spectroscopy is the study of the interaction of light and matter and has like a billion applications in ways you had no idea even existed. Maybe look into Bragg's law? I don't have anything in particular off hand, I have some textbooks but I wouldn't suggest buying them.
Bragg's law is about polarization by reflection right ? My textbook has covered it already
it does a good job of explaining the physics, but it rarely mentions about the practical applications
x-ray diffraction is one application of it, you shoot xrays at a crystal, move the machine through an angle recording if it absorbed or not and you get peaks which correspond to looking at the different views which line up with the crystal lattice. Bravais lattices, Miller indices, and Fourier analysis is all part of this, maybe look into that as well?
Okay thanks! math behind these doesn't look pleasant haha I'll look up them when free :) i guess for now il continue w/ my QM :)
Yeah keep with it, work through the pain lol.
\[E_e = \frac{E_\ell^2}{2mc^2}\] http://www.wolframalpha.com/input/?i=%28100*10^3*1.602677*10^%28-19%29%29^2%2F+%282*9.10938356+*+10^%28-31%29*+299792458^2*1.60217662+*+10^%28-19%29%29
Is x ray diffraction that hard? Furthermore, what is happening here? The calculation should be relatively simple. 1 eV is the KE of a electron when accelerated through 1 V. A 100 eV gamma ray has the energy of the kinetic energy of electron accelerated through 100 V. Use the de Broglie wavelength formula (also known as TheBroccoli wavelength by my friend) to find the momentum needed for the electron to have the same wavelength as the photon, then calculate the kinetic energy using \(\dfrac{p^2}{2m}\). Finally change the unit back to eV if necessary.
lol
Join our real-time social learning platform and learn together with your friends!