Upper limits for charm production in 150 GeV p-Be interactions

Bailey, R.; Becker, H.; Belau, E.; Böhringer, T.; Bosman, M.; Cerrada, M.; Chabaud, V.; Damerell, C.; Daum, C.; Dijkstra, H.; Dwuraźny, A.; Gillman, A. R.; Gilmore, R.; Görlich, L.; Hajduk, Z.; Hardwick, C.; Hoogland, W.; Hyams, B.; Klanner, R.; Lütjens, G.; Lütz, G.; Malos, J.; Männer, W.; Polok, G.; Różańska, M.; Rybicki, K.; Seebrunner, H. J.; Spierenburg, W.; Stierlin, U.; Tapper, R. J.; Tiecke, H.; Turała, M.; Vermeulen, J. C.; Waltermann, G.; Weilhammer, P.; Wickens, F. J.; Wiggers, L.; Wylie, A.; Żeludziewicz, T.

doi:10.1016/0550-3213(84)90082-8

Cited by 15 publications

(17 citation statements)

References 13 publications

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“…A second example involves the dilation of muon lifetime when muon decay is measured in a storage ring [8,9]. The hypothesis of locality implies that τ μ = γτ 0 μ , where τ 0 μ is the lifetime of the muon at rest and γ is the Lorentz factor corresponding to the circular motion of muons in the storage ring.…”

Section: Postulate Of Localitymentioning

confidence: 99%

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Nonlocal special relativity

Mashhoon¹

2008

Ann. Phys.

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In the special theory of relativity, Lorentz invariance is extended in Minkowski spacetime from ideal inertial observers to actual observers by means of the hypothesis of locality, which postulates that accelerated observers are always pointwise inertial.A critical examination of the locality assumption reveals its domain of validity: it is true for pointwise coincidences, but is in conflict with wave-particle duality. To remedy this situation, a nonlocal theory of accelerated systems is presented that reduces to the standard theory in the limit of small accelerations. Some of the main consequences of nonlocal special relativity are briefly outlined.

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Section: Postulate Of Localitymentioning

confidence: 99%

“…in accordance with (9). To generate all such kernels that are antisymmetric in their first and second pairs of indices from the Minkowski metric tensor η αβ , the Levi-Civita tensor αβγδ (with 0123 = 1) and the acceleration tensor φ αβ (τ ) is still a rather daunting task.…”

Section: Nonlocal Electrodynamicsmentioning

confidence: 99%

Nonlocal special relativity

Mashhoon¹

2008

Ann. Phys.

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“…Right: The inclusive cross section for Λ + c baryon production at x F > 0. The experimental data are from [25], [28] - [29] (CERN, FNAL, BIS-2), point (X) is from our experiment. Dashed lines are for predictions of two versions of QCD model [25].…”

Section: Resultsmentioning

confidence: 99%

Charmed particles production in pA-interactions at 70 GeV

Ryadovikov

2016

EPJ Web Conf.

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“…In the storage ring experiments for g µ −2 such as CERN [14] and BNL E821 [15], the muon anomalous magnetic moment a µ(EXP) was determined from the relation…”

Section: Storage Ring Experiments To Measure Muon G-2 In the Earth's Gmentioning

confidence: 99%

The general relativistic effects on the magnetic moment in Earth’s gravity

Ohira

2018

Progress of Theoretical and Experimental Physics

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The magnetic moment of free fermions in the Earth's gravitational field has been studied on the basis of the general relativity. Adopting the Schwarzschild metric for the background spacetime, the dipole coupling between the magnetic moment and the magnetic field has been found to be dependent of the gravity in the calculation up to the post-Newtonian order O(1/c 2 ). The gravity-dependence can be formulated by employing the effective value of the magnetic moment as a gravity-dependent quantity µ eff m = (1 + 3φ/c 2 ) µ m commonly for the cases of minimal coupling, non-minimal coupling and their mixture. The gravitationally induced anomaly is found to be canceled in the experimental values of the anomalous magnetic moment measured in the Penning trap and storage ring methods.

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Upper limits for charm production in 150 GeV p-Be interactions

Cited by 15 publications

References 13 publications

Nonlocal special relativity

Nonlocal special relativity

Charmed particles production in pA-interactions at 70 GeV

The general relativistic effects on the magnetic moment in Earth’s gravity

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