Search for Perpendicular Plane Anomaly in pd Breakup at Ep = 13 MeV

S. Kimura; K. Sagara; K. Ishibashi; S. Tanaka; K. Ohnaka; Y. Maeda

doi:10.1007/s00601-013-0691-4

Search for Perpendicular Plane Anomaly in pd Breakup at E_p = 13 MeV

S. Kimura, K. Sagara, K. Ishibashi, S. Tanaka, K. Ohnaka, Y. Maeda

Applied Nuclear Physics

Research output: Contribution to journal › Article › peer-review

Abstract

Space Star (SS) anomalies in nd and pd breakup reactions below 20 MeV were reported since 1989, but their origin has not been found yet. We have considered two conditions for the SS anomalies: condition (a) where three outgoing nucleons form an equilateral triangle and condition (b) in which the triangle is perpendicular to the beam axis. The condition (b) was investigated by our previous systematic experiments on pd breakup. In the present study, we started systematic experiments for the condition (a).

Original language	English
Pages (from-to)	1293-1296
Number of pages	4
Journal	Few-Body Systems
Volume	54
Issue number	7-10
DOIs	https://doi.org/10.1007/s00601-013-0691-4
Publication status	Published - Aug 2013

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics

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10.1007/s00601-013-0691-4

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title = "Search for Perpendicular Plane Anomaly in pd Breakup at Ep = 13 MeV",

abstract = "Space Star (SS) anomalies in nd and pd breakup reactions below 20 MeV were reported since 1989, but their origin has not been found yet. We have considered two conditions for the SS anomalies: condition (a) where three outgoing nucleons form an equilateral triangle and condition (b) in which the triangle is perpendicular to the beam axis. The condition (b) was investigated by our previous systematic experiments on pd breakup. In the present study, we started systematic experiments for the condition (a).",

author = "S. Kimura and K. Sagara and K. Ishibashi and S. Tanaka and K. Ohnaka and Y. Maeda",

year = "2013",

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doi = "10.1007/s00601-013-0691-4",

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journal = "Few-Body Systems",

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T1 - Search for Perpendicular Plane Anomaly in pd Breakup at Ep = 13 MeV

AU - Kimura, S.

AU - Sagara, K.

AU - Ishibashi, K.

AU - Tanaka, S.

AU - Ohnaka, K.

AU - Maeda, Y.

PY - 2013/8

Y1 - 2013/8

N2 - Space Star (SS) anomalies in nd and pd breakup reactions below 20 MeV were reported since 1989, but their origin has not been found yet. We have considered two conditions for the SS anomalies: condition (a) where three outgoing nucleons form an equilateral triangle and condition (b) in which the triangle is perpendicular to the beam axis. The condition (b) was investigated by our previous systematic experiments on pd breakup. In the present study, we started systematic experiments for the condition (a).

AB - Space Star (SS) anomalies in nd and pd breakup reactions below 20 MeV were reported since 1989, but their origin has not been found yet. We have considered two conditions for the SS anomalies: condition (a) where three outgoing nucleons form an equilateral triangle and condition (b) in which the triangle is perpendicular to the beam axis. The condition (b) was investigated by our previous systematic experiments on pd breakup. In the present study, we started systematic experiments for the condition (a).

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JO - Few-Body Systems

JF - Few-Body Systems

IS - 7-10

ER -

Search for Perpendicular Plane Anomaly in pd Breakup at E_p = 13 MeV

Abstract

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