ASACUSA experiment

ASACUSA receives antiproton beams from the AD and ELENA decelerator. These beams are decelerated to 0.01 MeV energy using a radiofrequency decelerator and the antiprotons are stored in the MUSASHI traps. The positrons to form antihydrogen atoms are obtained from ${\displaystyle {\ce {Na^{22}}}}$ radioactive source and stored in a positron accumulator. The mixing of antiprotons and positrons forms polarised and cold antihydrogen inside a double-Cusp trap. The polarised antihydrogen atoms from this system then enter the spectrometer where the measurements are done.[11]

ASACUSA team at beam setup preparation in September 2018

Hyperfine spectroscopy measurements on H beams in flight have been made using a Rabi experiment. The collaboration plans to conduct similar measurements on
H
in flight.[12][13]

ASACUSA team preparing beam setup for the ELENA beams in September 2018.

Anticipating completion of ELENA, with the aim of making spectral measurements of previously undetected atomic resonances in antiprotonic helium, a new 6 m electrostatic beamline was constructed to transport
p
s to a cryogenic target. [13] (Previous experiments, including the antiprotonic helium spectral measurements of March 2022 used a 3 m Radio-frequency Quadrupole to decelerate
p
s from the Antiproton Decelerator. [14][8][15]) 0.1 MeV ELENA
p
s entering the beamline are focussed to a width of ${\displaystyle \leq }$1 mm and pass through an aperture (30 mm length and 8 mm diameter). The transverse horizontal and vertical dimensions of the beam are determined by beam monitors consisting of a grid of gold-coated tungsten-rhenium wires with grid spacing of 20 μm.[14] (There are 3 such monitors along the beamline, one of which is ${\displaystyle \leq }$ 300 mm upstream of the cryogenic chamber.[13]) Further along the beamline, there is a configuration of 3 quadrupole magnets to counteract
p
beam expansion and 2 more apertures of diameters 30 mm and 16 mm. A beam emerging from the apertures is focussed to 3 mm diameter and impinges on a 6 mm diameter titanium window in an OFHC copper flange mounted on the cryogenic target chamber wall.[13] Acrylic and lead fluoride Čerenkov detectors monitor the beamline for
p
annihilations. The beamline pressure is 0.8 mb, much higher than the ELENA beamline pressure of ${\displaystyle \sim 10^{-9}}$ mb. The pressure difference is maintained by three 500 L/s titanium ion and 4 turbomolecular pumps.[13]

The helium targets are contained in a 35 mm diameter vessel made of titanium (gaseous or supercritical phase with 70% He-I) or OFHC copper (He-I and He-II) mounted on a liquid helium constant-flow cryostat. The vessel is enclosed within copper thermal shielding: an inner shield cooled by coolant helium vapour and an outer shield cooled by liquid nitrogen. A configuration of manometers and temperature sensors provide data used to characterize the state of the helium in the chamber. Pressures ${\displaystyle \geq }$ 1 MPa can be sustained.[8] The chamber is accessible to antiprotons through an annealed titanium window of diameter 75 μm or 50 μm vacuum brazed into the chamber wall.[8] Opposite this, a 28-mm diameter, 5-mm thick UV-grade sapphire window transmits laser light, antilinear to an incident particle beam.[8] Two 35-mm diameter Brewster windows made of fused silica (SiO
₂) mounted on flanges on opposite sides of the chamber walls perpendicular to the beam axis transmit laser light.[13][8] Near the cryostat, beneath the beampipe, is positioned a 300 ${\displaystyle \times }$ 200 ${\displaystyle \times }$ 20 mm${\displaystyle ^{3}}$ Čerenkov detector. Particles emerging from the cryostat, such as pions from
p
-
p
annihilations emit Čerenkov radiation in the detector which is detected by a photomultiplier.[8]