Program - Brookhaven National Laboratory
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[3] and theoretically predicted [4,5] relative increased neutron multiplicity for the heavy fragments with<br />
higher incident neutron energies has been studied. The impact is found to be noticeable on post-neutron<br />
mass yields, which are the relevant quantities for a-priori waste assessments. The fission cross sections for<br />
240,242 Pu at threshold and in the plateau region are being investigated within the ANDES project [6]. The<br />
results show some discrepancies (up to 12 %) to the ENDF/B-VII evaluation mainly for 242 Pu around 1<br />
MeV, where the evaluation exhibits a resonance-like structure not observed in the present work. The requested<br />
target accuracy in design studies of innovative reactor concepts like Gen-IV is in the range of a few<br />
percent. In order to be able to respond to requests for measurements of prompt neutron and gamma-ray<br />
emission [7,8] in fission IRMM has also invested in setting up a neutron and gamma-ray detector array. The<br />
neutron array is called SCINTIA and has so far been tested with 252 Cf(SF). For gamma-ray multiplicity<br />
and spectrum measurements lanthanum- and cerium-halide detectors are being used, and first quantitative<br />
results for 252 Cf(SF)and 235 U(nth, f) will be reported.<br />
[1] E. Birgersson et al., Nucl. Phys. A817, 1 (2008). [2] A. Al-Adili et al., Nucl. Instr. Meth. A624,<br />
684 (2010). [3] A. Naqvi et al., Phys. Rev. C34, 21 (1986). [4] K.-H. Schmidt and B. Jurado, Phys.<br />
Rev. C83, 061601 (2011). [5] C. Manailescu et al., Nucl. Phys. A867, 12 (2011). [6] ANDES project,<br />
http://www.andes-nd.eu/. [7] G.Rimpault in P.Rullhusen (Ed.), Proceedings of the Workshop on Nuclear<br />
Data Needs for GenerationIV, Antwerp, Belgium, WorldScientific, ISBN981- 256-830-1, 2006, April 2005,<br />
p.46. [8] G.Rimpault, A.Courcelle, D.Blanchet, Comment to the HPRL:ID H.3 and H.4, /http://www.oecdnea.org/html/dbdata/hprl/tmp/HPRLgammafission.pdf.<br />
RA 2 11:00 AM<br />
Dynamical Scission Model<br />
N. Carjan, M. Rizea<br />
<strong>National</strong> Institute of Physics and Nuclear Engineering ”Horia Hulubei”, PO Box MG-6, 077125,<br />
Bucharest-Magurele, Romania<br />
The sudden approximation has been recently used to calculate microscopic scission-properties during the<br />
low-energy fission of 236 U [1,3]. The purpose of the present paper is to go beyond this mathematical<br />
approximation and consider the real physical situation in which the scission process, i.e., the transition<br />
from two fragments connected by a thin neck (αi) to two separated fragments (αf ) takes place in a short<br />
but finite time interval ∆T . For this we follow the evolution from αi to αf of all occupied neutron states<br />
by solving numerically the two-dimensional time-dependent Schrödinger equation with time-dependent<br />
potential. Calculations are performed for mass divisions from AL = 70 to AL = 118 (AL being the light<br />
fragment mass). The exact duration of the neck rupture is unknown. ∆T is therefore taken as parameter<br />
having values from 0.25 × 10 −22 to 9 × 10 −22 sec. The resulting scission neutron multiplicities νsc and<br />
primary fragments’ excitation energies E ∗ sc are compared with those obtained in the frame of the sudden<br />
approximation (that corresponds to ∆T = 0). As expected, shorter is the transition time more excited<br />
are the fragments and more neutrons are emitted, the sudden approximation being an upper limit. For<br />
∆T = 10 −22 sec, which is a realistic value, the time dependent results are 20% below this limit. For<br />
transition times longer than 6 × 10 −22 sec the adiabatic limit is reached. The spatial distribution of the<br />
neutron emission points at scission is also calculated as function of the transition time ∆T . Together with<br />
the current density, it provides a detailed picture of the emission mechanism and a hint for the angular<br />
distribution of the scission neutrons with respect to the fission axis. Finally, the contributions of the light<br />
and of the heavy fragments to νsc and to E ∗ sc are estimated.<br />
[1] N. Carjan, P. Talou, O. Serot, Nucl. Phys. A 792(2007) 102 [2] N. Carjan, M. Rizea, Phys. Rev. C 82<br />
(2010) 014617 [3] N. Carjan, F.-J. Hambsch, M. Rizea, O. Serot, Phys. Rev. C 85 (2012) 044601<br />
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