The 44Ti(α, p) reaction and its implication on the 44Ti yield in supernovae

A. A. Sonzogni; K. E. Rehm; I. Ahmad; F. Borasi; D. L. Bowers; F. Brumwell; J. Caggiano; C. N. Davids; J. P. Greene; B. Harss; A. Heinz; D. Henderson; R. V.F. Janssens; C. L. Jiang; G. McMichael; J. Nolen; R. C. Pardo; M. Paul; J. P. Schiffer; R. E. Segel; D. Seweryniak; R. H. Siemssen; J. W. Truran; J. Uusitalo; I. Wiedenhöver

doi:10.1103/PhysRevLett.84.1651

The ⁴⁴Ti(α, p) reaction and its implication on the ⁴⁴Ti yield in supernovae

A. A. Sonzogni
, K. E. Rehm
, I. Ahmad
, F. Borasi
, D. L. Bowers
, F. Brumwell
, J. Caggiano
, C. N. Davids
, J. P. Greene
, B. Harss
, A. Heinz
, D. Henderson
, R. V.F. Janssens
, C. L. Jiang
, G. McMichael
, J. Nolen
, R. C. Pardo
, M. Paul
, J. P. Schiffer
, R. E. Segel

D. Seweryniak, R. H. Siemssen, J. W. Truran, J. Uusitalo, I. Wiedenhöver

Racah Institute of Physics

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

50 Scopus citations

Abstract

Cross sections for the ⁴⁴Ti(α, p)⁴⁷V reaction which significantly affects the yield of ⁴⁴Ti in supernovae were measured in the energy range 5.7MeV ≤ E_c.m. ≤ 9 MeV, using a beam of radioactive ⁴⁴Ti. The cross sections and the deduced astrophysical reaction rates are larger than the results from theoretical calculations by about a factor of 2. The implications of this increase in the reaction rate for the search of supernovae using space-based gamma detectors are discussed.

Original language	English
Pages (from-to)	1651-1654
Number of pages	4
Journal	Physical Review Letters
Volume	84
Issue number	8
DOIs	https://doi.org/10.1103/PhysRevLett.84.1651
State	Published - 2000

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Sonzogni, A. A., Rehm, K. E., Ahmad, I., Borasi, F., Bowers, D. L., Brumwell, F., Caggiano, J., Davids, C. N., Greene, J. P., Harss, B., Heinz, A., Henderson, D., Janssens, R. V. F., Jiang, C. L., McMichael, G., Nolen, J., Pardo, R. C., Paul, M., Schiffer, J. P., ... Wiedenhöver, I. (2000). The ⁴⁴Ti(α, p) reaction and its implication on the ⁴⁴Ti yield in supernovae. Physical Review Letters, 84(8), 1651-1654. https://doi.org/10.1103/PhysRevLett.84.1651

@article{3aae2f04ab9c411597d926c9af5a1e3f,

title = "The 44Ti(α, p) reaction and its implication on the 44Ti yield in supernovae",

abstract = "Cross sections for the 44Ti(α, p)47V reaction which significantly affects the yield of 44Ti in supernovae were measured in the energy range 5.7MeV ≤ Ec.m. ≤ 9 MeV, using a beam of radioactive 44Ti. The cross sections and the deduced astrophysical reaction rates are larger than the results from theoretical calculations by about a factor of 2. The implications of this increase in the reaction rate for the search of supernovae using space-based gamma detectors are discussed.",

author = "Sonzogni, \{A. A.\} and Rehm, \{K. E.\} and I. Ahmad and F. Borasi and Bowers, \{D. L.\} and F. Brumwell and J. Caggiano and Davids, \{C. N.\} and Greene, \{J. P.\} and B. Harss and A. Heinz and D. Henderson and Janssens, \{R. V.F.\} and Jiang, \{C. L.\} and G. McMichael and J. Nolen and Pardo, \{R. C.\} and M. Paul and Schiffer, \{J. P.\} and Segel, \{R. E.\} and D. Seweryniak and Siemssen, \{R. H.\} and Truran, \{J. W.\} and J. Uusitalo and I. Wiedenh{\"o}ver",

year = "2000",

doi = "10.1103/PhysRevLett.84.1651",

language = "אנגלית",

volume = "84",

pages = "1651--1654",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "8",

}

Sonzogni, AA, Rehm, KE, Ahmad, I, Borasi, F, Bowers, DL, Brumwell, F, Caggiano, J, Davids, CN, Greene, JP, Harss, B, Heinz, A, Henderson, D, Janssens, RVF, Jiang, CL, McMichael, G, Nolen, J, Pardo, RC, Paul, M, Schiffer, JP, Segel, RE, Seweryniak, D, Siemssen, RH, Truran, JW, Uusitalo, J & Wiedenhöver, I 2000, 'The ⁴⁴Ti(α, p) reaction and its implication on the ⁴⁴Ti yield in supernovae', Physical Review Letters, vol. 84, no. 8, pp. 1651-1654. https://doi.org/10.1103/PhysRevLett.84.1651

TY - JOUR

T1 - The 44Ti(α, p) reaction and its implication on the 44Ti yield in supernovae

AU - Sonzogni, A. A.

AU - Rehm, K. E.

AU - Ahmad, I.

AU - Borasi, F.

AU - Bowers, D. L.

AU - Brumwell, F.

AU - Caggiano, J.

AU - Davids, C. N.

AU - Greene, J. P.

AU - Harss, B.

AU - Heinz, A.

AU - Henderson, D.

AU - Janssens, R. V.F.

AU - Jiang, C. L.

AU - McMichael, G.

AU - Nolen, J.

AU - Pardo, R. C.

AU - Paul, M.

AU - Schiffer, J. P.

AU - Segel, R. E.

AU - Seweryniak, D.

AU - Siemssen, R. H.

AU - Truran, J. W.

AU - Uusitalo, J.

AU - Wiedenhöver, I.

PY - 2000

Y1 - 2000

N2 - Cross sections for the 44Ti(α, p)47V reaction which significantly affects the yield of 44Ti in supernovae were measured in the energy range 5.7MeV ≤ Ec.m. ≤ 9 MeV, using a beam of radioactive 44Ti. The cross sections and the deduced astrophysical reaction rates are larger than the results from theoretical calculations by about a factor of 2. The implications of this increase in the reaction rate for the search of supernovae using space-based gamma detectors are discussed.

AB - Cross sections for the 44Ti(α, p)47V reaction which significantly affects the yield of 44Ti in supernovae were measured in the energy range 5.7MeV ≤ Ec.m. ≤ 9 MeV, using a beam of radioactive 44Ti. The cross sections and the deduced astrophysical reaction rates are larger than the results from theoretical calculations by about a factor of 2. The implications of this increase in the reaction rate for the search of supernovae using space-based gamma detectors are discussed.

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U2 - 10.1103/PhysRevLett.84.1651

DO - 10.1103/PhysRevLett.84.1651

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AN - SCOPUS:0001174588

SN - 0031-9007

VL - 84

SP - 1651

EP - 1654

JO - Physical Review Letters

JF - Physical Review Letters

IS - 8

ER -

The ⁴⁴Ti(α, p) reaction and its implication on the ⁴⁴Ti yield in supernovae

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