Immanuel Estermann, O. C. Simpson and Otto Stern used gravitational deflection to measure atomic speeds. Stern describes scanning a hot-wire surface ionization detector through a cesium beam and recording ion electric current.[ref] Their 1947 paper reports potassium and cesium beams; a deficit of slow arrivals increased with oven pressure, supporting a source-slit collision explanation.[ref]
First consider an original point-launch model, with horizontal speed , zero initial vertical velocity, flight distance , and uniform gravitational acceleration . Downward displacement follows from flight time :
Slow particles fall farther. However, a detector scan counts arrivals per interval of height, not per interval of speed. Change of variables for probability densities supplies the Jacobian determinant:
Here denotes the effusive beam speed distribution; the unadorned constant in denotes gravitational acceleration. The integral of is one: substituting reduces it to . Its mode is . Simply mapping the most probable arrival speed into a fall distance instead gives . The peaks differ because equal height bins cover unequal speed intervals.
Figure 1.
Effusion changes the arrival speed distribution, and a detector-height scan requires another Jacobian determinant
. Original calculated distributions with chosen , , and . These are not historical measurements. Details.
For those chosen parameters, , so the detector-height probability density peaks near . A detector covering only accepts the fraction
At this is about , even before allowing for imperfect detection. Discarding the remainder changes the observed normalization.
Real slits transmit a range of launch heights and vertical velocities. Their geometrical response must be combined with the gravitational deflection and detector width; the point-launch formula is not an exact reduction of the historical apparatus. In the point-launch model, an initial vertical velocity would add to . Source collisions, detector efficiency and alignment can also distort a profile. Varying oven pressure helps distinguish such source losses from an incorrect thermal distribution; inferring a source temperature from the peak alone ignores both selection and the detector's coordinate transformation.
Molecular beam Created 2026-10-14 Updated 2026-10-18
A directed stream of molecules used to prepare samples for spectroscopy.
A molecular beam also includes a stream of chemical atoms, then called an atomic beam. An oven supplies particles; aligned slits restrict their directions, and a vacuum limits subsequent collisions. Narrowing the directions does not by itself make every particle's speed equal. This gives a useful separation of tasks: prepare a path, select or measure speed, apply an interaction, and read the resulting particle counts or deflection.
The advantage is unusually tangible. A magnetic field can separate spin components in the Stern-Gerlach experiment; even gravity can sort a beam by flight time. The effusive beam speed distribution explains which particles leave the source, while gravity deflection of an atomic beam explains how that distribution becomes a pattern on a detector.
Figure 1.
Two ways of measuring molecular beam speeds: rotating openings and gravitational flight
. Original functional schematics, not historical apparatus drawings. The lower panel exaggerates the fall for visibility; all numerical settings used in the text are chosen model inputs. Details.
Speed distribution 2026-10-18
A speed distribution is the probability distribution of the magnitude of velocity. When it has a probability density function , the fraction of particles with speeds between and is , and . The Maxwell speed distribution describes an equilibrium ideal gas; the effusive beam speed distribution weights that population by its rate of arrival.