Do Magnetic Fields Affect Photons in Binary Pulsars?

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The discussion centers on the effects of magnetic fields on photons in binary pulsars, sparked by a lecture from Victoria Kaspi. The original poster questions the notion that magnetic fields can block radio light from background objects, suggesting that this might relate to vacuum polarization. Responses indicate that pulsar magnetospheres can contain plasma, which may dampen radiation through cyclotron absorption. The concept of plasma frequency is introduced, explaining that high plasma density can suppress electromagnetic transmission. The poster expresses gratitude for the insights and plans to seek further clarification from physicists at future lectures.
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My wife and I attended the Perimeter Institute for theoretical physics. We watched the public lecture called: THE COSMIC GIFT OF NEUTRON STARS by VICTORIA KASPI. I thought it was a decent lecture (perimeter has had some outstanding ones in the past). On the way to work this morning I was pondering something she said. She talked about and showed an animation of a binary pulsar where the magnetic field was essentially "blocking" the radio light from the background object. Herein lies my question; I was under the impression magnetic fields do not effect photons in that way. The animation clearly wasn't showing a warping of space time. Was this referring to vacuum polarization? Or some other effect? I attempted a google search and came up fairly inconclusive.Can anyone help me out?

Here is a link to the video (which isn't in their video library yet)
I hope links are allowed!

The part I'm referring to is at the 46 minute mark.
Their video library with past public lectures can be found here:
http://perimeterinstitute.ca/video-library?qt-videos=1#qt-videos

Thanks!

Ben

edit: I completely forgot! Congratulations to Victoria for her recent award!
 
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I can't claim expertise here, but in the absence of any other responses I'll give you my educated guess made after some copious googling.

Apparently, pulsar magnetosphere can host plasma. Either trapped from solar wind of a companion star, or created locally in some process.

Radiation passing through magnetosphere can then be damped via cyclotron absorption.
 
It's possible that it's neutral atoms too. In the insane magnetic field of a magnetar, the electron clouds get squeezed and stretched. Atoms become long cylinders and I supposed that they'd seem denser to a passing photon?
 
If I had to guess, I'd say it's not the magnetic field in the magnetosphere that matters at all, it's just the plasma. There is something called the "plasma frequency", which is typically in the radio range, and is the frequency below which no radio waves can propagate through the plasma. The field from the radio wave creates charge separation which cancels that field, a bit like what a Faraday cage does. The plasma frequency gets higher at higher density (it scales with the square root of density), so all you need to completely suppress the electromagnetic transmittance from the pulsar is a high enough plasma density in the way.
 
Wow, Thanks for the responses' everyone! I have some more googling to do! At the perimeter public lectures they have physicists in the lobby that you can quiz when you arrive. I may have a couple more questions for them this time!

Thanks
Ben
 
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