Superconducting Radio Frequency - Cryogenics

Cryogenics

A significant part of SRF technology is cryogenic engineering. The SRF cavities tend to be thin-walled structures immersed in a bath of liquid helium having temperature 1.6 K to 4.5 K. Careful engineering is then required to insulate the helium bath from the room-temperature external environment. This is accomplished by:

  • A vacuum chamber surrounding the cold components to eliminate convective heat transfer by gases.
  • Multi-layer insulation wrapped around cold components. This insulation is composed of dozens of alternating layers of aluminized mylar and thin fiberglass sheet, which reflects infrared radiation that shines through the vacuum insulation from the 300 K exterior walls.
  • Low thermal conductivity mechanical connections between the cold mass and the room temperature vacuum vessel. These connections are required, for example, to support the mass of the helium vessel inside the vacuum vessel and to connect the apertures in the SRF cavity to the accelerator beamline. Both types of connections transition from internal cryogenic temperatures to room temperature at the vacuum vessel boundary. The thermal conductivity of these parts is minimized by having small cross sectional area and being composed of low thermal conductivity material, such as stainless steel for the vacuum beampipe and fiber reinforced epoxies (G10) for mechanical support. The vacuum beampipe also requires good electrical conductivity on its interior surface to propagate the image currents of the beam, which is accomplished by about 100 µm of copper plating on the interior surface.

The major cryogenic engineering challenge is the refrigeration plant for the liquid helium. The small power that is dissipated in an SRF cavity and the heat leak to the vacuum vessel are both heat loads at very low temperature. The refrigerator must replenish this loss with an inherent poor efficiency, given by the product of the Carnot efficiency ηC and a "practical" efficiency ηp. The Carnot efficiency derives from the second law of thermodynamics and can be quite low. It is given by

 \eta_C =
\begin{cases} \frac{T_{cold}} {T_{warm} - T_{cold}}, & \mbox{if } T_{cold} < T_{warm} - T_{cold} \\ 1, & \mbox{otherwise}
\end{cases}

where

Tcold is the temperature of the cold load, which is the helium vessel in this case, and
Twarm is the temperature of the refrigeration heat sink, usually room temperature.

In most cases Twarm =300 K, so for Tcold150 K the Carnot efficiency is unity. The practical efficiency is a catch-all term that accounts for the many mechanical non-idealities that come into play in a refrigeration system aside from the fundamental physics of the Carnot efficiency. For a large refrigeration installation there is some economy of scale, and it is possible to achieve ηp in the range of 0.2–0.3. The wall-plug power consumed by the refrigerator is then

,

where

Pcold is the power dissipated at temperature Tcold .

As an example, if the refrigerator delivers 1.8 K helium to the cryomodule where the cavity and heat leak dissipate Pcold=10 W, then the refrigerator having Twarm=300 K and ηp=0.3 would have ηC=0.006 and a wall-plug power of Pwarm=5.5 kW. Of course, most accelerator facilities have numerous SRF cavities, so the refrigeration plants can get to be very large installations.

The temperature of operation of an SRF cavity is typically selected as a minimization of wall-plug power for the entire SRF system. The plot to the right then shows the pressure to which the helium vessel must be pumped to obtain the desired liquid helium temperature. Atmospheric pressure is 760 Torr (101.325 kPa), corresponding to 4.2 K helium. The superfluid λ point occurs at about 38 Torr (5.1 kPa), corresponding to 2.18 K helium. Most SRF systems either operate at atmospheric pressure, 4.2 K, or below the λ point at a system efficiency optimum usually around 1.8 K, corresponding to about 12 Torr (1.6 kPa).

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