Categories
Time and Frequency

Measuring the thermal expansion of ULE glass

Here's an experiment I've done recently:


(Time-lapse of ca 18 hour experiment. Bottom left is a spectrum-analyzer view of the beat-note signal. Top left is a frequency counter reading of the beat-note. Bottom right is a screen showing the a camera-view of the output-beam from the resonator)

This is a measurement of the thermal expansion of a fancy optical resonator made from Corning "Ultra Low Expansion" (ULE) glass. This material has a specified thermal expansion of 0.03 ppm/K around room temperature. This thermal expansion is roughly 800-times smaller than Aluminium, around 400-times smaller than Steel, and 40-times better than Invar - a steel grade specifically designed for low thermal expansion.

Can we do even better? Yes! Because ULE glass has a coefficient of thermal expansion (CTE) that crosses zero. Below a certain temperature it shrinks when heated, and above the zero-crossing temperature it expands when heated (like most materials do). This kind of behavior sounds exotic, but is found is something as common as water! (water is heaviest at around 4 C). If we can use the ULE resonator at or very close to this magic zero-crossing temperature it will be very very insensitive to small temperature fluctuations.

So in the experiment I am changing the temperature of the ULE glass and looking for the temperature where the CTE crosses zero (let's call this temperature T_ZCTE). The effect is fairly small: if we are 1 degree C off from T_ZCTE we would expect the 300 mm long piece of ULE glass to be 200 pm (picometers) longer than at T_ZCTE. That's about the size of a single water-molecule, so this length change isn't exactly something you can go and measure with your digital calipers!

Here's how it's done (this drawing is simplified, but shows the essential parts of the experiment):

ule_resonator_drawing

We take a tuneable HeNe laser and lock the frequency of the laser to the ULE-cavity. The optical cavity/resonator is formed between mirrors that are bonded to the ends of the piece of ULE glass. We can lock the laser to one of the modes of the cavity, corresponding to a situation where (twice) the length of the cavity is an integer number of wavelenghts. Now as we change the temperature of the ULE-glass the laser will stay locked, and as the glass shrinks/expands the wavelength (or frequency/color) of the laser will change slightly.

Directly measuring the frequency of laser light isn't possible. Instead we take second HeNe laser, which is stabilized to have a fixed frequency, and detect a beat-note between the stabilized laser and the tuneable laser. The beat-note will have a frequency corresponding to the (absolute value of the) difference in frequency between the two lasers. Now measuring a length-change corresponding to the size of a single water-molecule (200 pm) shouldn't be that hard anymore!

Let's say the stabilized laser has a wavelength of \lambda_1 = 632.8 \,\mathrm{nm} (red light). Its frequency will be \nu_1 = {c \over \lambda_1} = 474083438685209 \,\mathrm{Hz} (that's around 474 THz). When the tuneable laser is locked to the cavity we force its wavelength to agree with \lambda_2 = {2L\over m} where m is an integer and L is the length of the cavity. I've drawn only a small number of wavelengths in the figure, but a realistic integer is m=948167. We get \lambda_2 = 632.7999181579 \,\mathrm{nm} and \nu_2 = {c \over \lambda_2} = 474083500000000 \,\mathrm{Hz}, very nearly but not quite the same wavelength/frequency as the stabilized laser. Now our photodiode which measures the beat-note will measure a frequency of \nu_{beat} = | \nu_1-\nu_2 | = 61.314 \,\mathrm{ MHz}.

How does this change when the ULE glass expands by 200 pm? When we heat or cool the cavity by 1 degree C the length changes to 300 mm + 200 pm, and the wavelength of the tuneable laser will change to
\lambda_3 = 632.7999185797\,\mathrm{nm}. Now our beat-note detector will show \nu_{beat} = | \nu_1-\nu_3 | = 60.998 \,\mathrm{ MHz}. That's a change in the beat-note of more than 300 kHz - easily measurable!

That's how you measure a length-change corresponding to the diameter of a water molecule!

Why do this? Some of the best ultra-stable lasers known are made by locking the laser to this kind of ULE-resonator. Narrow linewidth ultra-stable lasers are interesting for a host of atomic physics and other fundamental physics experiments.

See also: Janis Alnis playing with two ultra-stable lasers.

Update 2013 August: I made a drawing in inkscape of the experimental setup.

cte_setup_drawing

This figure shows most (if not all?) of the important components of this experiment. The AOM is not strictly required but I found it useful to shift the tuneable HeNe laser by +80 MHz to reach a TEM-00 mode of the ULE resonator. Not shown is a resonance-circuit (LC-tank) between the 2.24MHz sinewave-generator and the EOM. The EOM was temperature controlled by a TEC with an NTC thermistor giving temperature feedback.

Categories
Telescope Making

Mirror grinding

To keep the mirror edge from chipping and breaking we are putting a bevel on it. Most guides tell you to do that with a sharpening stone which is made from carborundum bonded into a stone-like material. I thought doing the bevel by hand with the stone was much too slow, so I tried it with a diamond-bit on a dremel:

This works much faster and a 1-2 mm bevel can be made in a few minutes. After the bevel grinding you see our 'grind-o-matic' machine. It's driven by a 90 W DC motor with a 30:1 gear-head connected to a 12 mm steel axle which supports an aluminium disk on which the mirror or tool sits. There's a sheet of plastic to keep the wood and floor dry.

After about 2 hours of grinding with nr. 60 carborundum we achieved 1 mm of sagitta. A drop of glycerol in the grinding slurry helps to avoid stiction between the mirror and the tool. For a 240 mm diameter F/6 mirror the target sagitta is 2.5 mm so there is still some work to do.