1996
DOI: 10.1086/176780
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Indirect Investigation of the D + 6Li Reaction at Low Energies Relevant for Nuclear Astrophysics

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Cited by 94 publications
(88 citation statements)
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“…The occurrence of the QF mechanism at low energies has been pointed out in a number of papers [1,[26][27][28]. We will see how applying the conditions on the momentum distribution of the spectator, as discussed in Ref.…”
Section: The Methodsmentioning
confidence: 89%
See 1 more Smart Citation
“…The occurrence of the QF mechanism at low energies has been pointed out in a number of papers [1,[26][27][28]. We will see how applying the conditions on the momentum distribution of the spectator, as discussed in Ref.…”
Section: The Methodsmentioning
confidence: 89%
“…In the last decades strong efforts were devoted to the development and application of indirect methods in nuclear astrophysics. Among the most used indirect methods, an important role is played by the Trojan Horse Method (THM) which has been applied to several reactions in the past decade [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17] at the energies relevant for astrophysics (typically smaller than few hundred keV's), which usually are far below the Coulomb barrier, of the order of MeV's. Many tests have been made to fully explore the potentiality of the method and extend as much as possible its applications: the target/projectile break-up invariance [18], the spectator invariance [19,20] and the possible use of virtual neutron beams [21,22].…”
Section: Introductionmentioning
confidence: 99%
“…The first measurement using the Trojan horse method (THM) [25][26][27] with an RI beam has been performed at CRIB [28]. The measurement was to study the 18 F(p, α) 15 O reaction at low energies relevant to astrophysics via the three body reaction 2 H( 18 F, α 15 O)n. The 18 F(p, α) 15 O reaction rate is particularly responsible for the 511-keV γ ray emission in nova explosion phenomena.…”
Section: Indirect Measurementsmentioning
confidence: 99%
“…A list of typical parameters of RI beams produced at CRIB is found in [4]. New RI beams recently developed at CRIB are 16 N (1 × 10 6 pps), 10 Be (2 × 10 4 pps), 15 O (1 × 10 6 pps), and 26 Al (1 × 10 5 pps). The low-energy RI beams at CRIB are particularly suitable for studies on astrophysical reactions and nuclear resonant structure, as discussed below.…”
Section: Introductionmentioning
confidence: 99%
“…In order to overcome the experimental problems connected to these measurements, new experimental techniques as well as indirect methods where proposed and used in many experiments over the last decades. One of these indirect methods, the Trojan Horse method (THM) [1][2][3][4][5][6][7][8][9][10][11][12][13], that will not be discussed here, has proved to be particularly flexible and reliable and it allowed for the measurement of the cross sections of various reactions of astrophysical interest. Nonetheless when reactions induced by Radioactive Ion Beams (RIBs) are considered, the yield is so low that even using indirect method the total detection efficiency becomes an issue.…”
Section: Introductionmentioning
confidence: 99%