An electromagnetic field carries momentum as well as energy. In vacuum, its SI momentum density iswhere is the Poynting vector. Thus the field momentum in a region is . [ref]
The Feynman Lectures on Physics, Volume II by Richard Feynman and others. Section 27–6, equations 27.21–27.22, momentum density and energy flux
For a directed vacuum plane wave, , so a pulse with total energy carries momentum . Complete absorption transfers that momentum to matter. Reversing the pulse at a stationary perfect mirror transfers twice as much normal momentum, explaining radiation pressure.
Conservation joins field momentum to the mechanical momentum of matter and momentum crossing the chosen boundary. Changing a field can therefore accelerate matter even when no material particle carries the momentum across the intervening space. Static configurations can also contain nonzero field momentum; the vacuum formula does not require radiation. [ref]
The Feynman Lectures on Physics, Volume II by Richard Feynman and others. Section 27–6, charge-magnet example and return of stored angular momentum
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