INDRA, a 4π charged product detection array at GANIL

Pouthas, J.; Borderie, B.; Dayras, R.; Plagnol, E.; Rivet, M. F.; Saint‐Laurent, F.; Steckmeyer, J.C.; Auger, G.; Bacri, C.O.; Barbey, S.; Barbier, A.; Benkirane, A.; Benlliure, J.; Berthier, B.; Bougamont, E.; Bourgault, P.; Box, P.; Bzyl, R.; Cahan, B. D.; Cassagnou, Y.; Charlet, D.; Charvet, J. L.; Chbihi, A.; Clerc, T.; Copinet, N.; Cussol, D.; Engrand, M.; Gautier, J.M.; Huguet, Y.; Jouniaux, O.; Laville, J.L.; Botlan, P. Le; Leconte, Antoine; Légrain, R.; Lelong, Ph.; Guay, M. Le; Martina, L.; Mazur, C.; Mosrin, P.; Olivier, L.; Passerieux, J.P.; Pierre, S.; Piquet, B.; Plaige, E.; Pollacco, E.; Raine, B.; Richard, A.; Ropert, J.; Spitaels, C.; Stab, L.; Sznajderman, D.; Tassan‐Got, L.; Tillier, J.; Tripon, M.; Vallerand, P.; Volant, C.; Volkov, P.; Wieleczko, J. P.; Wittwer, G.

doi:10.1016/0168-9002(94)01543-0

Cited by 252 publications

(136 citation statements)

References 34 publications

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“…The charged particle array is arranged in 12 concentric rings around the beam axis. The eight forward rings have the same geometrical design as the INDRA detector, but have less granularity [7]. In those rings, the individual segments are fronted by ionization chambers (IC) filled with 30 Torr of CF 4 gas.…”

Section: Methodsmentioning

confidence: 99%

Tracing the evolution of temperature in near Fermi energy heavy ion collisions

et al. 2005

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The kinetic energy variation of emitted light clusters has been employed as a clock to explore the time evolution of the temperature for thermalizing composite systems produced in the reactions of 26A, 35A and 47A MeV 64 Zn with 58 Ni, 92 Mo and 197 Au. For each system investigated, the double isotope ratio temperature curve exhibits a high maximum apparent temperature, in the range of 10-25 MeV, at high ejectile velocity. These maximum values increase with increasing projectile energy and decrease with increasing target mass. The time at which the maximum in the temperature curve is reached ranges from 80 to 130 fm/c after contact. For each different target, the subsequent cooling curves for all three projectile energies are quite similar. Temperatures comparable to those of limiting temperature systematics are reached 30 to 40 fm/c after the times corresponding to the maxima, at a time when AMD-V transport model calculations predict entry into the final evaporative or fragmentation stage of de-excitation of the hot composite systems. Evidence for the establishment of thermal and chemical equilibrium is discussed.

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Section: Methodsmentioning

confidence: 99%

Tracing the evolution of temperature in near Fermi energy heavy ion collisions

et al. 2005

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“…The experiment has been performed taking advantage of the coupling of the 4π detector INDRA [9,10] and the VAMOS spectrometer [11]. The INDRA multidetector, designed to study the deexcitation properties of hot nuclei produced during a heavy ions collision, has a structure in rings centered on the beam axis.…”

Section: Methodsmentioning

confidence: 99%

Exploring isospin effects on the level density parameter

Marini

Rivet

Borderie

et al. 2010

EPJ Web of Conferences

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“…Therefore it is necessary to take into account the secondary decay before comparing to the experimental data. We performed an experiment at GANIL using the VAMOS spectrometer [18] coupled to the INDRA 4π array [19]. Four reactions have been studied combining Ca isotopes, 40,48 Ca + 40,48 Ca at E/A = 35MeV [7].…”

Section: Symmetry Energy From the Isotopic Distributionsmentioning

confidence: 99%