International Conference on Recent Issues in Nuclear and Particle Physics (RINP2)

Session

Plenary Session III

3 Feb 2019, 16:45

Lipika Auditorium, Visva-Bharati, Santiniketan

46. Nuclear Reactions using VEC: (1977 – 2017), A Journey over 4 decades

Prof. C. Bhattacharya (Variable Energy Cyclotron Centre, 1/AF, Bidhan Nagar, Kolkata, INDIA chandana@vecc.gov.in )

03/02/2019, 16:45

The Variable Energy Cyclotron (VEC), at Kolkata, recently completed its 40 years of operation in 2017. Several milestones have been achieved in experimental nuclear physics, using the light and heavy ions beams from this cyclotron during the last four decades. In this talk, an overview of the intense research activities carried out in nuclear reaction studies, using beams from cyclotron during...

70. MSSM with Non-Standard Soft Interactions

Prof. Utpal Chattopadhyay (School of Physical Sciences, Indian Association for the Cultivation of Science, Jadavpur, Kolkata 700032 India)

03/02/2019, 17:10

Non-holomorphic soft supersymmetry breaking interactions will be discussed in relation to MSSM. Unlike MSSM, it is possible to have a higgsino as a single component type of dark matter candidate while having a low electroweak fine-tuning. Muon g-2 may also be enhanced. We will also explore the bottom squark sector by studying the 2b plus missing transverse energy signal at the LHC. We will...

61. Weakly Bound Neutron-Rich Nuclei and Cosmic Phenomena

Prof. Ushasi Datta (Saha Institute Of Nuclear Physics )

03/02/2019, 17:35

The study of single particle and bulk properties of the neutron-rich nuclei constrains fundamental issues of Nuclear physics like limits of existence of the quantum many body system ( atomic nucleus) and equation of state of neutron-rich matter etc [1-7]. This information has also important impact in understanding cosmic phenomena, like neutron star, nucleosynthesis, evolution of star...

85. Looking for Extra Dimensions at the Large Hadron Collider

Anindya Datta (University of Calcutta)

A model of elementary particles defined in $4 +1$ space time dimensions
naturally provides a candidate for the dark Matter. The hall mark of such a model is the presence of Kaluza Klein excitations of our known Standard Model fields. We will discuss a possible search strategy of such a model at the Large Hadron Collider.