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SUMMARY:LOW ENERGY INCOMPLETE FUSION REACTIONS: PROBING OF ENTRANCE CHANEE
 L EFFECTS
DTSTART;VALUE=DATE-TIME:20220715T120000Z
DTEND;VALUE=DATE-TIME:20220715T122000Z
DTSTAMP;VALUE=DATE-TIME:20260414T112356Z
UID:indico-contribution-398@events.sinp.msu.ru
DESCRIPTION:Speakers: ANUJ KUMAR JASHWAL (BAREILLY COLLEGE\, BAREILLY)\nDu
 ring last couple of years\, the probability of incomplete fusion in heavy 
 ion induced reactions for both strongly bound and loosely bound projectile
 s has been observed at energies as low as 4 – 5 MeV/A [1 – 4]. The HI 
 induced reactions are important in basic research for the fundamental unde
 rstanding of reaction mechanism and to test the validity of various parame
 ters existing in available nuclear reaction models [5 – 7]. The importan
 ce of measured cross-section data has been found in applied research\, mor
 e particularly\, in reactor technology for nuclear energy generation and w
 aste management. Although the dynamics of the multiplicity of processes li
 ke complete fusion (CF)\, incomplete fusion (ICF)\, and pre-compound (PCN)
  emission in heavy ion (HI) interactions at low projectile energies depend
  on various entrance channel parameters\, moreover the projectile energy a
 nd angular momentum of the compound nucleus systems are some of the key pa
 rameters\, which play significant role in the characterization of such pro
 cesses in HI reactions. The entrance channel mass asymmetry\, alpha Q-valu
 e\, neutron thickness\, coulomb factor (ZpZt) and target deformation are s
 ome important entrance channel parameters\, that affects the probability o
 f incomplete fusion in heavy ion reactions. In the present work an attempt
  has been made to have an exclusive study on aforementioned entrance chann
 el parameters on 12C\, 13C\, 16O\, 18 O and 14N induced reactions with var
 ious target systems. It is observed that proper account of these entrance 
 channel parameters is very much essential to conclusively explain the inco
 mplete fusion reactions. \n\n1. K. Kumar\, T. Ahmad\, S. Ali\, I. A. Rizvi
 \, A. Agarwal\, R. Kumar\, and A. K. Chaubey\, Phys. Rev. C 89\, 054614(20
 14).\n2. S. Mukherjee\, A. Sharma\, S. Sodaye\, A. Goswami\, and B. S. Tom
 ar\, Int. J. Mod. Phys. E 15\, 237 (2006). \n3. Z. T. Dai\, D. Q. Fang\, Y
 . G. Ma\, X. G. Cao\, G. Q. Zhang\, and W. Q. Shen\, Phys. Rev. C 91\, 034
 618 (2015).\n4.  A. Agarwal et al.\, Phys. Rev. C 105\, 034609 (2022). M. 
 Goeppert-Mayer\, Phys. Rev. 78\, 16 (1950).\n5. M. Crippa\, E. Gadioli\, P
 . Vergani\, G. Ciavola\, C. Marchetta and M. Bonardi\, Z. Phys. A 350 (199
 4) 121.\n6. M. Cavinato\, E. Fabrici\, E. Gadioli\, E. Gadioli Erba\, P. V
 ergani\, M. Crippa\, G. Colombo\, I. Redaelli  and M. Ripamonti\, Phys. Re
 v. C 52  (1995) 2577.\n7. D. J. Parker\, J. Asher\, T. W. Conlon and I. M.
  Naqib\, Phys. Rev. C 30 (1984) 143.\n\nhttps://events.sinp.msu.ru/event/8
 /contributions/398/
LOCATION: Физический ф-т\, СФА
URL:https://events.sinp.msu.ru/event/8/contributions/398/
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