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Electronic accumulation of extremely cold positrons in ultrahigh vaccum
- Source :
- Physica Scripta. :337-340
- Publication Year :
- 1995
- Publisher :
- IOP Publishing, 1995.
-
Abstract
- Many cold positrons in ultrahigh vacuum are required to produce cold antihydrogen, to cool highly stripped ions, and to study ultracold plasmas. Up to 3.5 × 104 such positrons have now been accumulated into the ultrahigh vacuum of a 4.2 K Penning trap, at a rate exceeding 103/hr. Both the accumulation rate (per high energy positron incident at the trap), and the number accumulated, are much larger than ever before realized at low temperatures in high vacuum. Cooling of high energy positrons (from 22Na decay) in a tungsten crystal near the trap, together with purely electronic trapping and damping, are key to the efficient accumulation and to projected improvements.
- Subjects :
- Condensed Matter::Quantum Gases
Physics
Astrophysics::High Energy Astrophysical Phenomena
Ultra-high vacuum
chemistry.chemical_element
Plasma
Trapping
Tungsten
Condensed Matter Physics
Penning trap
Atomic and Molecular Physics, and Optics
Ion
Crystal
chemistry
Physics::Accelerator Physics
Physics::Atomic Physics
Atomic physics
Antihydrogen
Mathematical Physics
Subjects
Details
- ISSN :
- 14024896 and 00318949
- Database :
- OpenAIRE
- Journal :
- Physica Scripta
- Accession number :
- edsair.doi...........4d8b9e5ea5a0e2f7ccbd4c988d54369c
- Full Text :
- https://doi.org/10.1088/0031-8949/1995/t59/046