31NeNeon
Z:  
Z = 10N = 21
N:  

Setting ID1 Yield 2
[pps/pnA]
Measurement
date
Beam Target Brho01
[Tm]
F1 slit
L [mm]
F1 slit
R [mm]
Data from
1008.14e-32014-12-0948Ca 345MeVBe 20mm8.8380120.0120.0 ---
2451.30e-12008-12-1448Ca 345MeVBe 15mm8.2000120.0120.0Nucl. Instrum. Methods Phys. Res., Sect. B 317, 756 (2013)



Publication
Title Journal First Author
Magicity versus Superfluidity around 28O viewed from the Study of 30FPhys. Rev. Lett. 133, 082501 (2024)J. Kahlbow
Deformation-Driven p-Wave Halos at the Drip Line: 31NePhys. Rev. Lett. 112, 142501 (2014)T. Nakamura
Interaction cross sections for Ne isotopes towards the island of inversion and halo structures of 29Ne and 31NePhys. Lett. B 707, 357 (2012)M. Takechi
Electric dipole response of halo nucleiPhys. E 43, 820 (2011)T. Nakamura
Measurements of nuclear radii for neutron-rich Ne isotopes 28−32NeNucl. Phys. A 834, 412 (2010)M. Takechi
Halo Structure of the Island of Inversion Nucleus 31NePhys. Rev. Lett. 103, 262501 (2009)T. Nakamura

Experiment
Proposal No. Spokesperson Start-Date End-Date Beam Course
DA16-01D. S. Ahn2017-03-302017-04-0248Ca 345 MeV/u ZeroDegree
NP1406-SAMURAI27N. Kobayashi2016-11-192016-11-2248Ca 345 MeV/u SAMURAI
NP0802-RIBF55T. Nakamura2008-12-152008-12-2148Ca 345 MeV/u ZeroDegree
NP0702-RIBF08-02T. Otsubo2008-12-092008-12-1848Ca 345 MeV/u ZeroDegree


 Annotations:
1 Detailed BigRIPS setting is shown in the linked page.
2 The list of primary beam intensities is given in this page.
3 Error is only statistical one. Systematic error is estimated within 30%, which comes from uncertainly of primary beam intensity.


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