Quasicontinuum ridges in 173,174W

M. Cromaz; J. DeGraaf; T. E. Drake; D. Ward; A. Galindo-Uribarri; V. P. Janzen; D. C. Radford; N. C. Schmeing; S. Flibotte; S. M. Mullins; J. Rodriguez; S. Pilotte

doi:10.1103/PhysRevC.54.2055

Quasicontinuum ridges in ^173,174W

M. Cromaz, J. DeGraaf, T. E. Drake, D. Ward, A. Galindo-Uribarri, V. P. Janzen, D. C. Radford, N. C. Schmeing, S. Flibotte, S. M. Mullins, J. Rodriguez, S. Pilotte

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3 Scopus citations

Abstract

A strong quasicontinuum ridge with a spacing of 58.1 ± 0.3 keV was observed in ¹⁷³W and ¹⁷⁴W when populated at high spin. The ridge is a factor of 4 times more intense than that of the sum of discrete bands over the same range of rotational frequencies. The strength of the ridge may be due to the large number of nearly degenerate proton orbitals lying above the Z = 73 gap occurring at a deformation β₂≈0.3.

Original language	English
Pages (from-to)	2055-2058
Number of pages	4
Journal	Physical Review C - Nuclear Physics
Volume	54
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevC.54.2055
State	Published - Oct 1996
Externally published	Yes

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10.1103/PhysRevC.54.2055

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title = "Quasicontinuum ridges in 173,174W",

abstract = "A strong quasicontinuum ridge with a spacing of 58.1 ± 0.3 keV was observed in 173W and 174W when populated at high spin. The ridge is a factor of 4 times more intense than that of the sum of discrete bands over the same range of rotational frequencies. The strength of the ridge may be due to the large number of nearly degenerate proton orbitals lying above the Z = 73 gap occurring at a deformation β2≈0.3.",

author = "M. Cromaz and J. DeGraaf and Drake, {T. E.} and D. Ward and A. Galindo-Uribarri and Janzen, {V. P.} and Radford, {D. C.} and Schmeing, {N. C.} and S. Flibotte and Mullins, {S. M.} and J. Rodriguez and S. Pilotte",

year = "1996",

month = oct,

doi = "10.1103/PhysRevC.54.2055",

language = "English",

volume = "54",

pages = "2055--2058",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

number = "4",

}

TY - JOUR

T1 - Quasicontinuum ridges in 173,174W

AU - Cromaz, M.

AU - DeGraaf, J.

AU - Drake, T. E.

AU - Ward, D.

AU - Galindo-Uribarri, A.

AU - Janzen, V. P.

AU - Radford, D. C.

AU - Schmeing, N. C.

AU - Flibotte, S.

AU - Mullins, S. M.

AU - Rodriguez, J.

AU - Pilotte, S.

PY - 1996/10

Y1 - 1996/10

N2 - A strong quasicontinuum ridge with a spacing of 58.1 ± 0.3 keV was observed in 173W and 174W when populated at high spin. The ridge is a factor of 4 times more intense than that of the sum of discrete bands over the same range of rotational frequencies. The strength of the ridge may be due to the large number of nearly degenerate proton orbitals lying above the Z = 73 gap occurring at a deformation β2≈0.3.

AB - A strong quasicontinuum ridge with a spacing of 58.1 ± 0.3 keV was observed in 173W and 174W when populated at high spin. The ridge is a factor of 4 times more intense than that of the sum of discrete bands over the same range of rotational frequencies. The strength of the ridge may be due to the large number of nearly degenerate proton orbitals lying above the Z = 73 gap occurring at a deformation β2≈0.3.

UR - http://www.scopus.com/inward/record.url?scp=0030509565&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.54.2055

DO - 10.1103/PhysRevC.54.2055

M3 - Article

AN - SCOPUS:0030509565

SN - 0556-2813

VL - 54

SP - 2055

EP - 2058

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 4

ER -

Quasicontinuum ridges in ^173,174W

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