Malus law in quantum mechanics

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SUMMARY

The discussion centers on Malus's law in quantum mechanics, specifically regarding the intensity of polarized light passing through a polarizer at a 45-degree angle. When sending the state |y> = 1/sqrt{2}( |H> + |V> ) into the polarizer, the intensity loss depends on the diagonal basis chosen. The intensity of light transmitted through the polarizer can be calculated using the formula | |^2. For objects with different spins, the polarization vector must be rotated into the polarizer's basis, which involves understanding angular momentum operators and their role in rotations.

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  • Understanding of quantum mechanics concepts, particularly polarization and Malus's law.
  • Familiarity with quantum state notation, such as kets and basis transformations.
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  • Study the derivation and implications of Malus's law in quantum mechanics.
  • Learn about the mathematical representation of polarization states and their transformations.
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  • Read Sakurai's Modern Quantum Mechanics for a deeper understanding of polarization and spin systems.
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Students and professionals in quantum mechanics, physicists studying light polarization, and anyone interested in the mathematical foundations of quantum state transformations.

AlexHT
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Hi,

For example, if I were to send |y> = 1/sqrt{2}( |H> + |V> ) photons into a polarizer with a 45 degre angle from horizontal, would the beam loose intensity? How can I calculate it on my own?


EDIT: The picture below illustrate what is happening. I am changing the base from x-y to a diagonal base. Do I loose intensity?
 

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No. Or rather, it depends on which diagonal you're talking about. One will allow |H>+|V> through and completely block |H>-|V> ; the other will do the reverse. You can pretty much see what happens here just by looking at things: the lower-left to upper-right diagonal clearly corresponds to |H>+|V> -- that line is given by c (\hat{x}+\hat{y}) ,\ c \in R after all -- and so a polarizer along that lines corresponds to a projection onto |H>+|V>. The intensity of light getting through is given by | <\mbox{light}|\mbox{polarizer}>|^2 where light is the normalized polarization vector of the light, and polarizer is the normalized vector of the polarizer.

In a more general situation -- I mean when you're dealing with polarization of objects which are not spin-1 like light -- what you'd want to do is rotate the object's polarization vector into the basis of the polarizer. To do this you need to know how the object transforms under rotations; that can be found by exponentiating the angular momentum operators (which are the generators of rotations.) If this sounds like gobbedy-gook, you can study a good (grad-level) quantum mechanics textbooks. They will go into this in some depth. IIRC Sakurai's Modern Quantum Mechanics is particularly good on this topic. For a spin-m object polarized perpendicularly to the plane of the polarizer, this turns out to be pretty simple; you get roughly the same result as for light, except the rotation angle that shows up is proportional to m*theta, ie

|\mbox{rotated ket}> = \left( \begin{array}{cc} \cos(m\theta) & \sin(m\theta) \\ -\sin(m\theta) & \cos(m\theta) \end{array} \right) |\mbox{original ket}>
 

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