2017
DOI: 10.1016/j.phpro.2017.09.051
|View full text |Cite
|
Sign up to set email alerts
|

Direct Reaction Measurements Using GODDESS

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

10
84
0

Year Published

2018
2018
2024
2024

Publication Types

Select...
5
2
1

Relationship

1
7

Authors

Journals

citations
Cited by 19 publications
(94 citation statements)
references
References 6 publications
10
84
0
Order By: Relevance
“…The commissioning experiment exploited 134 Xe beams with ≈1 mg/cm 2 CD 2 targets to measure excitations in 135 Xe including candidates for 2f7/2 and 3p3/2 excitations above the N=82 shell gap. Preliminary results have been reported [13] and show gamma-ray events in coincidence with protons well above the neutron separation energy, the surrogate (n,n'γ) excitation region. ORRUBA can also be coupled to GRETINA [15] and a new LaBr3(Ce)-based Hybrid Array of Gamma-Ray Detectors (HAGRiD) currently being developed under the leadership of the University of Tennessee [16].…”
Section: Developing Techniques To Measure (Dpγ) Reactions With Ribsmentioning
confidence: 91%
See 1 more Smart Citation
“…The commissioning experiment exploited 134 Xe beams with ≈1 mg/cm 2 CD 2 targets to measure excitations in 135 Xe including candidates for 2f7/2 and 3p3/2 excitations above the N=82 shell gap. Preliminary results have been reported [13] and show gamma-ray events in coincidence with protons well above the neutron separation energy, the surrogate (n,n'γ) excitation region. ORRUBA can also be coupled to GRETINA [15] and a new LaBr3(Ce)-based Hybrid Array of Gamma-Ray Detectors (HAGRiD) currently being developed under the leadership of the University of Tennessee [16].…”
Section: Developing Techniques To Measure (Dpγ) Reactions With Ribsmentioning
confidence: 91%
“…We are part of the Gammasphere ORRUBA: Dual Detectors for Experimental Structure Studies (GODDESS) collaboration [13] that has developed the techniques to couple the Oak Ridge Rutgers University Barrel Array (ORRUBA) of position-sensitive silicon strip detectors [14] to the Gammasphere array of up to 110 Compton-suppressed HPGe detectors at the ATLAS accelerator at Argonne National Laboratory. The commissioning experiment exploited 134 Xe beams with ≈1 mg/cm 2 CD 2 targets to measure excitations in 135 Xe including candidates for 2f7/2 and 3p3/2 excitations above the N=82 shell gap.…”
Section: Developing Techniques To Measure (Dpγ) Reactions With Ribsmentioning
confidence: 99%
“…13 (top) in the under-depleted case (80 V) with the condition that the multiplicity is equal to 1. The signal from the protons, deuterons and tritons on one side and from 4 He and then Li isotopes on the other side align on an almost parabolic shape. The punchthroughs of the protons, deuterons, tritons appear as a straight line and are mixed up.…”
Section: Pulse Shape Discrimination and Effect Of Strip Lengthmentioning
confidence: 97%
“…The measurement of the light ejectiles only will not be sufficient to identify the populated states and coupling with gamma-rays detectors will be crucial. This is the reason for which the new generation of Silicon arrays like GODDESS [4], T-REX [5] and GRIT [6] are designed to be coupled with state-of-the-art gamma arrays.…”
Section: Introductionmentioning
confidence: 99%
“…To realize (d, pγ) reaction studies with radioactive ion beams, the Gammasphere ORRUBA: Dual Detectors for Experimental Structure Studies (GODDESS) [299] was commissioned with the Oak Ridge Rutgers University Barrel Array (ORRUBA) of position-sensitive silicon strip detectors augmented with annular arrays of end cap detectors. Preliminary results [300] with the N=80 134 Xe beam showed population of a candidate for the 3p 3/2 3/2 − state important for DSD capture and the gamma-decay probability data at high excitation energy that would be needed for a surrogate (n, γ) analysis, should statistics be sufficient.…”
Section: Recent and Planned Experiments With Radioactive Ionsmentioning
confidence: 99%

FRIB and the GW170817 Kilonova

Aprahamian,
Surman,
Frebel
et al. 2018
Preprint