Appearance of Nuclear Shell Effects and Initial Charge (mass) Asymmetry in the Formation of Products of Heavy Ion Collisions

Bibcode
2011IJMPE..20..406N
DOI
10.1142/S021830131101779X
Nasirov, Avazbek; Fazio, Giovanni; Giardina, Giorgio; Mandaglio, Giuseppe; Manganaro, Marina; Muminov, Akhtam
Bibliographical reference

International Journal of Modern Physics E, Volume 20, Issue 02, pp. 406-414 (2011).

Advertised on:
2011
Number of authors
6
IAC number of authors
0
Citations
1
Refereed citations
1
Description
The role of the entrance channel in the formation of the reaction products is discussed. The excitation functions of evaporation residues for the 50Ti+249Cf and 54Cr+248Cm reactions are compared.
Type
Refereed

It may interest you

  • Refereed
    Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b
    The spectral signatures of optical absorbers, when combined with those of infrared molecules, play a critical role in constraining the cloud properties of exoplanet atmospheres. We aim to use optical transmission spectroscopy to confirm the tentative color signature previously observed by multiband photometry in the atmosphere of hot Jupiter HAT-P
    Kang, Huiyi et al.

    Advertised on:

    7
    2024
    Bibcode
    2024A&A...687A...9K
    Citations
    0
  • Refereed
    The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ∼ 2
    Aims: We provide an in-depth analysis of the COSMOS-Web ring, an Einstein ring at z ≈ 2 that we serendipitously discovered during the data reduction of the COSMOS-Web survey and that could be the most distant lens discovered to date. Methods: We extracted the visible and near-infrared photometry of the source and the lens from more than 25 bands
    Mercier, W. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024A&A...687A..61M
    Citations
    0
  • Refereed
    Migration and Evolution of giant ExoPlanets (MEEP). I. Nine Newly Confirmed Hot Jupiters from the TESS Mission
    Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA's TESS
    Schulte, Jack et al.

    Advertised on:

    7
    2024
    Bibcode
    2024AJ....168...32S
    Citations
    0