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PuK - Process Technology & Components 2024

A technical trade magazine with a history of more than 60 years.

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Vacuum technology<br />

Vacuum systems<br />

gravitational wave hits the plane in<br />

which the arms of the interferometer<br />

lie, one arm (or both, depending on<br />

the direction of incidence) is periodically<br />

shortened and lengthened. This<br />

changes the conditions for optical<br />

superposition, i. e. destructive interference,<br />

which produces a signal at<br />

the so-called dark finge. This is what<br />

makes the gravitational wave visible,<br />

or rather audible. LIGO is based on<br />

the same principle. At the two LIGO<br />

sites in the US states of Washington<br />

and Louisiana, great care is taken to<br />

ensure that the highly sensitive mirrors<br />

and their reflective properties<br />

are not affected by dirt. Therefore,<br />

only dry, hydrocarbon-free pumps<br />

are used to create the necessary vacuum.<br />

The pumping stations used consist<br />

of dry screw pumps and magnetically<br />

levitated turbopumps. This is<br />

the only way to achieve the limit of<br />

< 1 monolayer in 10 years on the mirrors.<br />

In addition to cleanliness, low vibration<br />

plays an important role.<br />

To ensure that new and more<br />

gravitational wave signals can be detected<br />

in the future, continuous improvements<br />

are needed to reduce<br />

interference. Detectors on Earth are<br />

limited in particular by the suspension<br />

and regulation of the mirrors in a<br />

vacuum. This suspension is necessary<br />

to isolate the mirrors from disturbances<br />

such as seismic waves. At the<br />

same time, however, it must allow the<br />

mirrors to be perfectly positioned. In<br />

particular, the next generation of detectors,<br />

such as the European Einstein<br />

Telescope [5], will be even more sensitive<br />

at lower frequencies and therefore<br />

require mirror suspensions with<br />

improved control and less noise. In<br />

order to develop the necessary technologies,<br />

smaller laboratories are trying<br />

to simulate the environmental<br />

conditions for the development of<br />

better instruments and components<br />

as accurately as possible, also in order<br />

not to reduce the observation<br />

times in the large detectors.<br />

As part of the “Quantum Universe”<br />

Cluster of Excellence (EXC2121:<br />

German Research Foundation - project<br />

number 390833306), the research<br />

group headed by Prof. Dr. Oliver<br />

Gerberding at the University of Hamburg<br />

is working on improving optomechanical<br />

sensors. Pfeiffer Vacuum the system, a second optical table is<br />

GmbH is supporting the working mounted on a side wall of the vacuum<br />

chamber and enables the trans-<br />

group with a special vacuum system.<br />

The vacuum system developed mission of laser light from the outside<br />

to the inside via transparent<br />

and manufactured within the project<br />

“VatiGrav” (vacuum chamber with flanges in the same plane as both<br />

seismic isolation of an optical test experimental tables. For easy access<br />

platform, funded by the University of to the chamber and the experiment<br />

Hamburg/State of Hamburg and the table inside, there are doors on both<br />

German Research Foundation, DFG, sides of the vacuum chamber. There<br />

project number 455096128) fulfills is a single large door at the front to<br />

several functions at once with its size make the entire interior volume accessible<br />

for experiments. This can<br />

of approx. 1.5 m long, 2 m wide and<br />

2.5 m high. The stainless-steel vacuum also be used to remove the internal<br />

chamber with a free internal dimension<br />

of 1.74 x 1.02 x 1.51 m (LxWxH) the vacuum chamber is divided and<br />

optical table if required. The rear of<br />

serves as a container for the experimental<br />

setups of Prof. Gerberding’s via two separate doors.<br />

allows access to the experiment table<br />

research group. For this purpose, the In addition to the dual functions<br />

vacuum chamber is equipped with of test chamber and vibration damping,<br />

the vacuum system is responsi-<br />

an optical table, which rests on passive<br />

vibration dampers on the chamber<br />

floor and on which the laser in-<br />

are performed under vacuum condible<br />

for ensuring that the experiments<br />

terferometry experiments and the tions. For this purpose, two oil-free<br />

pendulum systems can be set up. The ACP 40 multistage Roots pumps from<br />

purpose of the passive dampers is to Pfeiffer Vacuum are installed in the<br />

allow low-vibration experiments under<br />

vacuum conditions. In addition, in an adjacent room of the laboratory<br />

vacuum chamber. These are located<br />

the vacuum chamber itself rests on and are connected to the chamber by<br />

active vibration dampers that use internal<br />

sensor and control technology The two pumps are used to gener-<br />

approximately 4 m of vacuum piping.<br />

to ensure that vibrations and oscillations<br />

from the environment are sup-<br />

Once the pre-vacuum pressure of<br />

ate the pre-vacuum in the chamber.<br />

pressed and do not affect the experiments.<br />

Frequencies above 2 Hz are the ATH 3204 M turbomolecular<br />

about 1e-1 mbar has been reached,<br />

absorbed with over 90 % damping. pump located on the chamber ceiling<br />

This isolation concept is based on can be switched on to achieve even<br />

correspondingly more complex systems<br />

at LIGO [6] and in other spe-<br />

magnetically levitated turbomolecu-<br />

lower pressures. The ATH 3204 M is a<br />

cial laboratories around the world. To lar pump from Pfeiffer Vacuum and<br />

couple experimental setups outside has a maximum pumping speed of<br />

Fig. 2: Vacuum chamber with seismic isolation of an optical test platform<br />

PROCESS TECHNOLOGY & COMPONENTS <strong>2024</strong><br />

43

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