2018
DOI: 10.1007/s10751-018-1536-9
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Hyperfine spectroscopy of hydrogen and antihydrogen in ASACUSA

Abstract: The ASACUSA collaboration at the Antiproton Decelerator of CERN aims at a precise measurement of the antihydrogen ground-state hyperfine structure as a test of the fundamental CPT symmetry. A beam of antihydrogen atoms is formed in a CUSP trap, undergoes Rabi-type spectroscopy and is detected downstream in a dedicated antihydrogen detector. In parallel measurements using a polarized hydrogen beam are being performed to commission the spectroscopy apparatus and to perform measurements of parameters of

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Cited by 23 publications
(14 citation statements)
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References 33 publications
(45 reference statements)
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“…107) In the case of the p charge-to-mass ratio, 146) the length of the bar is well defined, while the right end is the cyclotron frequency, which is proportional to the magnetic field. 147) For a more rigorous comparison, one possible way is to convert to the upper limit of the SME coefficients. 126) In order for free-fall to be practically observable, a good guess would be to expect g"t to be comparable to, or larger than, v T , where g is the gravitational acceleration (F 9.8 m/s 2 ), "t the observation time and v T a typical velocity due to thermal motion of antihydrogen atoms.…”
Section: Gravitational Interaction Between Matter and Antimattermentioning
confidence: 99%
See 2 more Smart Citations
“…107) In the case of the p charge-to-mass ratio, 146) the length of the bar is well defined, while the right end is the cyclotron frequency, which is proportional to the magnetic field. 147) For a more rigorous comparison, one possible way is to convert to the upper limit of the SME coefficients. 126) In order for free-fall to be practically observable, a good guess would be to expect g"t to be comparable to, or larger than, v T , where g is the gravitational acceleration (F 9.8 m/s 2 ), "t the observation time and v T a typical velocity due to thermal motion of antihydrogen atoms.…”
Section: Gravitational Interaction Between Matter and Antimattermentioning
confidence: 99%
“…16 summarize several particle properties related to the advancements of cold antimatter research. 37 , 107 , 126 , 145 147 ) The latest values discussed in §6 are listed together with the data in Review of Particle Physics 2018. 37 ) The magnetic moments of the antiproton and the proton are now known to agree like 0.3 8.3 , a three orders of magnitude improvement that given in Ref.…”
Section: High Precision Measurementsmentioning
confidence: 99%
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“…The ASACUSA-CUSP (Atomic Spectroscopy And Collisions Using Slow Antiprotons) antihydrogen experiment based at the Antiproton Decelerator facility of CERN aims to perform precise tests of CPT symmetry by measuring the ground-state hyperfine structure (GS-HFS) of antihydrogen atoms and comparing it with that of hydrogen. 1 A brief account on the status of ASACUSA's antihydrogen program can be found within these proceedings. 2 The currently applied Rabi-type beam-spectroscopy method can be made more precise by the implementation of Ramsey's technique of using two separated oscillatory fields.…”
Section: Antihydrogen Spectroscopy Program Of Asacusamentioning
confidence: 99%
“…By operating at sufficiently high B ext (e.g., 23/69/115 µT as in Ref. 15) the systematic shifts and related uncertainties can easily be kept below ∼ 10 ppb, an acceptable level for the anticipated first-stage results on H. A measurement of a single pair of a π 1 and σ 1 transitions in this regime of B ext provides a reliable way to determine the zero-field splitting from a calculation, 15 i.e., without extrapolating to zero field by a fit. Thus, the present apparatus is well suited for a first Rabi-type SME-sensitive H hyperfine-structure measurement.…”
Section: Interference Effect and Future Measurements And Devicesmentioning
confidence: 99%