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1.
H. Koch 《Hyperfine Interactions》1989,44(1-4):59-64
A short review on measured production rates for antideuterons and other light antinuclei (3H,3He,4He) is given. The physics interest in experiments with these particles is described. The main items are the production mechanisms,
antideuteron-atoms, antideuteron-induced possible quark/gluon phase transitions and the study of the properties (masses, magnetic
moments, ...) of these particles. The paper finishes with the discussion of production schemes for low energy antideuterons.
It turns out that with small modifications of the present
-production facility at CERN more than 107 antideuterons/day could be stored and used for experiments. 相似文献
2.
P. Kienle 《Hyperfine Interactions》2009,194(1-3):153-158
We present here a proposal to make use of the antiproton ion collider AIC of FAIR to breed cold antideuterons using the pionic fusion reactions $\overline{pp} \to \overline{d}\pi^{-}$ . An antideuteron yield of 1.4% per pair of antiprotons is reached. With a luminosity L?=?5.2×1028 cm???2 s???1 the expected antideuteron production rate is 23 s???1. Methods for improving the antideuteron yield and production rate are indicated. 相似文献
3.
A.A. Yukhimchuk V.A. Apasov Yu.I. Vinogradov A.N. Golubkov E.V. Gornostaev S.K. Grishechkin L.V. Drakin N.A. Zagoruiko V.N. Istratov P.D. Ishkov A.A. Kononenko G.I. Karyakin V.G. Klevtsov V.A. Klisch V.N. Lobanov A.P. Maksimenko S.S. Matveev A.E. Nikitin V.I. Pustovoy I.I. Sukhoi V.M. Solyankin B.N. Tenyaev V.M. Kharitonov 《Hyperfine Interactions》1999,119(1-4):341-344
A facility is described that allows safe handling of high tritium gas activity as dozens kilocuries in a regular laboratory
environment. It is used to make and deliver into the target a mixture of specific isotopic composition with the contamination
requirement of 10-7 v.f. for Z>1 elements, and recover it upon completion of operation. With this facility, efforts have been accomplished to investigate
into the muon catalyzed fusion on two targets – liquid tritium and high-pressure tritium types. Also, the operation range
was 0.1–120 MPa for pressure and 20–800 K for temperature and the amount of tritium used was about 100 kCi. The facility showed
reliability in operation without indications of radiation beyond the safety level.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
4.
H. Albrecht U. Binder G. Harder H. Hasemann A. Philipp W. Schmidt-Parzefall H. Schröder H.D. Schulz R. Wurth A. Drescher B. Gräwe U. Matthiesen H. Scheck J. Spengler D. Wegener R. Heller K.R. Schubert H. Gennow 《Physics letters. [Part B]》1985,157(4):326-332
The production of antideuterons has been observed in electron-positron annihilations at center-of-mass energies around 10 GeV. Antideuterons have been identified unambiguously by their energy loss in the drift chamber, their time-of-flight and the pattern of their energy deposition in the shower counters of the ARGUS detector. The production rate in the momentum range (0.6?1.8) GeV/c is (1.6?0.7+1.0) × 10?5 per hadronic event. 相似文献
5.
6.
Adler SS Afanasiev S Aidala C Ajitanand NN Akiba Y Alexander J Amirikas R Aphecetche L Aronson SH Averbeck R Awes TC Azmoun R Babintsev V Baldisseri A Barish KN Barnes PD Bassalleck B Bathe S Batsouli S Baublis V Bazilevsky A Belikov S Berdnikov Y Bhagavatula S Boissevain JG Borel H Borenstein S Brooks ML Brown DS Bruner N Bucher D Buesching H Bumazhnov V Bunce G Burward-Hoy JM Butsyk S Camard X Chai JS Chand P Chang WC Chernichenko S Chi CY Chiba J Chiu M Choi IJ Choi J Choudhury RK Chujo T 《Physical review letters》2005,94(12):122302
The production of deuterons and antideuterons in the transverse momentum range 1.1
相似文献
7.
Md. Monirul Haque Hironari Yamada Ahsa Moon Mami Yamada 《Journal of synchrotron radiation》2009,16(2):299-306
The performance of the far‐infrared (FIR) beamline of the 6 MeV tabletop synchrotron light source MIRRORCLE‐6FIR dedicated to far‐infrared spectroscopy is presented. MIRRORCLE‐6FIR is equipped with a perfectly circular optical system (PhSR) placed around the 1 m‐long circumference electron orbit. To illustrate the facility of this light source, the FIR output as well as its spectra were measured. The optimum optical system was designed by using the ray‐tracing simulation code ZEMAX. The measured FIR intensity with the PhSR in place is about five times higher than that without the PhSR, which is in good agreement with the simulation results. The MIRRORCLE‐6FIR spectral flux is compared with a standard thermal source and is found to be 1000 times greater than that from a typical thermal source at ~15 cm?1. It is also observed that the MIRRORCLE‐6FIR radiation has a highly coherent nature. The broadband infrared allows the facility to reach the spectral range from 10 cm?1 to 100 cm?1. MIRRORCLE‐6FIR, owing to a large beam current, the PhSR mirror system, a large dynamic aperture and small ring energy, can deliver a bright flux of photons in the FIR/THz region useful for broadband spectroscopy. 相似文献
8.
Fuke H Maeno T Abe K Haino S Makida Y Matsuda S Matsumoto H Mitchell JW Moiseev AA Nishimura J Nozaki M Orito S Ormes JF Sasaki M Seo ES Shikaze Y Streitmatter RE Suzuki J Tanaka K Tanizaki K Yamagami T Yamamoto A Yamamoto Y Yamato K Yoshida T Yoshimura K 《Physical review letters》2005,95(8):081101
We performed a search for cosmic-ray antideuterons using data collected during four BESS balloon flights from 1997 to 2000. No candidate was found. We derived, for the first time, an upper limit of 1.9 x 10(-4) (m2s sr GeV/nucleon)(-1) for the differential flux of cosmic-ray antideuterons, at the 95% confidence level, between 0.17 and 1.15 GeV/nucleon at the top of the atmosphere. 相似文献
9.
S. M. Kalebin V. S. Artamonov D. A. Liakin G. V. Rukolaine I. L. Karpikhin S. V. Barabin V. V. Konovalov 《Physics of Atomic Nuclei》2002,65(2):255-260
An experiment aimed at testing the equivalence of the inertial and the gravitational mass is considered in which use is made of a facility including a vacuum chamber with two coupled oscillators (a pendulum and dynamical damper that form a vibrational system featuring two degrees of freedom) and falling onto the Sun. The layout of the facility and its basic parameters are presented. The pendulum and the dynamical damper have the same natural frequency, which is equal to the frequency of their rotation about the Sun. This frequency is dependent on the date of the experiment and can be calculated on the basis of the time equation. In the proposed facility, the amplitude of oscillations of the damper is 1.2×10?5 rad, which is much greater than the value of 10?7 rad previously achieved in the experiment that tested the equivalence principle to the highest precision of about 10?12. This precision can be considerably improved. The result is presented that was obtained from a measurement during the solar eclipse in Moscow on August 11, 1999. 相似文献
10.
Yu. V. Tokarev M. L. Kaiser P. Rodrigues V. A. Alimov Yu. I. Belov G. N. Boiko G. P. Komrakov N. V. Muravyova A. V. Rakhlin 《Radiophysics and Quantum Electronics》1999,42(8):705-714
We present experimental results on reception of VHF signals of the transmitting facility “Sura” of the Radiophysical Research
Institute by the NASA spacecraft WIND. The experiments were performed during daytime during the summer seasons 1997–1998.
The dependence of power and spectral characteristics of the VHF radio waves on the power of the sounding radiation is analyzed.
We find that, in a wide range of effective powers of the VHF radiation from about 40 kW to 160 MW, the phenomena observed
in the radiation received onboard WIND (such as focusing, scintillations, or frequency deviations of signals) does not usually
depend on the operation mode of the “Sura” facility. At the same time, broadening of the radiation pattern of the facility
and decrease of the mean level of the received signal by about 6 dB toward the direction of maximum of the radiation pattern
were observed at the peak radiation power of the facility. The experimental results are compared to present concepts on effects
of self-focusing instability and nonlinear defocusing of VHF radio waves in the ionospheric plasma.
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 42, No. 8, pp. 799–809, August 1999. 相似文献
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12.
B. Alper H. Bℷgild P. Booth F. Bulos L.J. Carroll G. von Dardel G. Damgaard B. Duff F. Heymann J.N. Jackson G. Jarlskog L. Jonsson A. Klovning L. Leistam E. Lillethun G. Lynch G. Manning M. Prentice J.M. Weiss 《Physics letters. [Part B]》1973,46(2):265-268
Measurements have been performed on production of particles with mass 1.5 GeV/c2 and charge for θlab = 62.5° and . At pT = 0.7 GeV/c the relative rate of production of antideuterons to π? is (5 ± 1) × 10?5. The deuteron to antideuteron ratio is 3.7 ± 1.2. No new stable particle has been amongst 0.7 × 108 charged particles entering our detector. 相似文献
13.
Dip N. Mahato R. H. Pink S. R. Badu R. H. Scheicher Archana Dubey H. P. Saha Lee Chow Mahendra K. Mahanti M. B. Huang T. P. Das 《Hyperfine Interactions》2007,174(1-3):15-20
The LPCTrap facility is coupled to the low-energy beam line LIRAT of the SPIRAL source at GANIL (France). The facility comprises
an RFQ trap for beam preparation and a transparent Paul trap for in-trap decay studies. The system has been tested for several
ion species. The Paul trap has been fully characterized for 6Li+ and 23Na+ ions. This characterization together with GEANT4 simulations of the in-trap decay setup (Paul trap and detection system)
has permitted to predict the effect of the size of the ion cloud on the decay study of 6He+. 相似文献
14.
Haikun Yue Dong Li Chenre Wang Xiaofei Li Dezhi Chen Kaifeng Liu Chi Zhou Ruimin Pan 《等离子体物理论文集》2015,55(9):658-663
An Radio‐Frequency (RF) Inductively Coupled Plasma (ICP) ion source test facility has been successfully developed at Huazhong University of Science and Technology (HUST). As part of a study on hydrogen plasma, the influence of three main operation parameters on the RF power necessary to ignite plasma was investigated. At 6 Pa, the RF power necessary to ignite plasma influenced little by the filament heating current from 5 A to 9 A. The RF power necessary to ignite plasma increased rapidly with the operation pressure decreasing from 8 Pa to 4 Pa. The RF power necessary to ignite plasma decreased with the number of coil turns from 6 to 10. During the experiments, plasma was produced with the electron density of the order of 1016m–3 and the electron temperature of around 4 eV. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
15.
J. Formánek 《Czechoslovak Journal of Physics》1981,31(11):1256-1264
The problem of annihilation of fast antideuterons in complex nuclei is analyzed semi-quantitatively in the framework of a simple probabilistic model. Sensitivity of the annihilation cross section to two-particle nuclear distribution is scrutinized.Dedicated to Professor Ivan Úlehla on the occasion of his sixtieth birthday. 相似文献
16.
B. Bayanov A. Burdakov A. Kuznetsov A. Makarov S. Sinitskii Yu. Sulyaev S. Taskaev 《Radiation measurements》2010,45(10):1462-1464
An innovative accelerator-based neutron source for boron neutron capture therapy has started operation at the Budker Institute of Nuclear Physics, Novosibirsk. This facility is based on a compact vacuum insulation tandem accelerator designed to produce proton current up to 10 mA. Epithermal neutrons are proposed to be generated by 1.915 MeV protons bombarding a lithium target using 7Li(p,n)7Be threshold reaction.In the article, techniques to detect neutron and gamma-rays at the facility are described. Gamma radiation is measured with NaI and BGO gamma-spectrometers. The total yield of neutrons is determined by measuring the 477 keV γ-quanta from beryllium decay. For the rough analysis of the generated neutron spectrum we used bubble detectors. As the epithermal neutrons are of interest for neutron capture therapy the NaI detector is used as activation detector. We plan to use a time-of-flight technique for neutron spectra measurement. To realize this technique a new solution of short time neutron generation is proposed. 相似文献
17.
Ph. Velten G. Ban D. Durand X. Fl��chard E. Li��nard F. Mauger A. M��ry O. Naviliat-Cuncic D. Rodr��guez J. C. Thomas 《Hyperfine Interactions》2011,199(1-3):29-38
The LPCTrap experiment is devoted to the precise measurement of the ??-?? angular correlation parameter, a ?|? , in the pure Gamow-Teller decay of 6He+. This experiment is motivated by the search of the presence of tensor type contributions in the weak interaction. The radioactive source is confined in a transparent Paul trap installed at LIRAT, the low energy beam line of the SPIRAL facility. The ??-?? correlation is studied by measuring the time of flight of the recoil ions detected in coincidence with the ?? particles. During the last experiment, a total of 4 × 106 coincidence events have been recorded which would enable to determine the coefficient with a statistical uncertainty of 0.5%. The status of the analysis is presented in this contribution. 相似文献
18.
M. Andersson C. Bargholtz Kj. Fransson L Holmberg K. Lindh L. M⇘rtensson I. Sitnikova P. E. Tegnér P. Thörngren Engblom G. Weiss K. Wilhelmsen Rolander 《Acta Physica Hungarica A》1997,6(1-4):37-43
The isobaric analogue state of the ground state of the halo nucleus6He,6Li* has been studied in a pionic fusion experiment at the CELSIUS storage ring facility in Uppsala, Sweden. This was the first of two proposed experiments with the aim to study the high momentum part of the wave functions of the halo nuclei6He and6Li (0+, T=1). The Li nuclei were produced in inverse kinematics reactions with alpha particles incident on a deuterium cluster jet target. The6Li ions were detected in a zero-degree spectrometer situated in the fourth quadrant of the CELSIUS ring. The measurement was done for three different beam energies corresponding to 5.4, 2.2 and 1.5 MeV above threshold in the c.m. The cross-sections slowly increase with beam energy from 95 nb at the lowest energy to about 250 nb at 5.4 MeV above threshold. 相似文献
19.
B. V. Antokhonov S. F. Berezhnev D. Besson N. M. Budnev R. Wischnevski O. A. Gress A. N. Diachok A. V. Zablotsky A. V. Zagorodnikov N. N. Kalmykov N. I. Karpov V. A. Kozhin E. E. Korosteleva A. V. Korobchenko L. A. Kuzmichev A. Chiavassa B. K. Lubsandorzhiev R. R. Mirgazov M. I. Panasyuk L. V. Pankov V. V. Prosin V. S. Ptuskin Yu. A. Semeney A. A. Silaev A. A. Silaev Jr. A. V. Skurikhin M. Stokham O. A. Chvalaiev B. A. Shaibonov Jr. J. Snyder Ch. Spiering I. V. Yashin 《Bulletin of the Russian Academy of Sciences: Physics》2011,75(3):367-370
A new array for studying ultra-high energy cosmic rays was inaugurated in 2009 in the Tunka Valley, about 50 km from Lake Baikal. Having an area of 1 km2, the new facility allows us to study cosmic rays with energies of 1015–1018 eV via the a unified method for registering Cherenkov radiation from extensive air showers (EASes) and is making a substantial contribution to understanding the origin of ultra-high energy cosmic rays. We describe the current state of the experiment, the new methodological approach, our initial results, and the plans for further development of the array. 相似文献