Conveners
Technical Session 02: Plenary Talk 01 & Track 01 Oral Presentations (1st half)
- M.K. Das (Tezpur University)
Description
HEP & Astro-particle, Astronomy and Astrophysics (& Plenary Talk 1)
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Victoria Puyam (Department of Physics, Manipur University)Track 01Oral
The neutrino mass models containing different scalars are constructed using $A_{4}\times Z_{4}$ discrete symmetry group. The mass matrices are developed in such a way that they can give necessary deviation from Tribimaximal mixing to generate non-zero $\theta_ {13}$. The resultant mass matrices are analyzed and compared to understand the contribution of $A_{4}$ singlet scalars to the mass...
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Mr Diptimonta Neog (Department of Physics, North Eastern Regional Institute of Science and Technology)Track 01Oral
Abstract: The studies of the Parton distribution function (PDFs) open a new way to a better understanding of the partonic quark-gluon structure of the nucleon. In the QCD study of high-energy processes, PDFs are essential. We study a few PDF sets with various Q2 ranges and momentum fraction x. All PDFs’ numerical values have been taken from the LHAPDF library, a user-friendly interface to PDF...
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Mr Ranjan Saikia (Tezpur University)Track 01Oral
Many deep inelastic scattering (DIS) experiments conducted on hadrons by leptons on the experimental site have produced important data on the distribution of partons within hadrons. Theoretical analysis of distribution at the various kinematical regions of small-$x$ (Bjorken's $x$) and $Q^2$ of DIS experiments is facilitated by the use of quantum chromodynamics (QCD) evolution equations. The...
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Mr Joydeep Thakur (University of North Bengal)Track 01Oral
We study the elliptic flow parameter $(v_2)$ and its event-by-event (e-by-e) fluctuation for the charged hadrons produced in $^{197}$Au+$^{197}$Au collisions at the nucleon-nucleon center of momentum energy $\sqrt{s_{\rm NN}} = 7.7$, $11.5$, $19.6$, $27.0$, $39.0$ and $62.4$ GeV of the STAR Beam Energy Scan (BES) program. We use A Multiphase Transport (AMPT) model in its string melting (SM)...
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Naba Jyoti Gogoi (PhD Research Scholar)Track 01Oral
Our presentation is based on the thermodynamic topology of the Euler-Heisenberg-AdS black hole and the higher-order Euler-Heisenberg-AdS black hole. This investigation is carried out by considering the generalized off-shell free energy approach, where black holes are conceptualized as defects in the thermodynamic space. Our study adopts the newly introduced residue method for this purpose. Our...
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Bhabana Kumar (Tezpur University)Track 01Oral
This paper present a comprehensive investigation into the construction of a neutrino mass model utilizing the $\Gamma (3)$ modular group, which exhibits an isomorphism with the $A_{4}$ symmetric group. The study focuses on developing a left-right asymmetric model by incorporating modular symmetry. An advantageous aspect of employing modular symmetry in our model is the elimination of need for...
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Jotin Gogoi (Tezpur University)Track 01Oral
We have studied neutrino masses and mixings by adding a scalar triplet $\eta$ to the particle content of minimal inverse seesaw. In order to realize this extension of minimal inverse seesaw we implement an isomorphic modular group $\Gamma(3)$ and a non-abelian discrete symmetry group $A_4$. The use of modular symmetry in our work helps us to reduce the number of flavons. We have also used...
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Dr Vivek Baruah Thapa (Bhawanipur Anchalik College)Track 01Oral
In this study, we investigate the influence of the nuclear symmetry energy slope on the equation of state (EoS) of dense matter with Δ-admixed exotic matter in neutron stars and its consequences for neutron star (NS) observable properties such as mass-radius
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relationships and tidal responses. The equation of state is formulated within the framework of covariant density functional theory,... -
Yumnam Monitar SinghTrack 01Oral
The neutrino oscillation parameters are numerically extracted through the diagonalization of a general Majorana neutrino mass matrix whose elements are randomly generated within certain range of allowed values. The allowed values of each element are determined by using the latest neutrino oscillation experimental data within 3$\sigma$. The latest Planck upper bound on the sum of three absolute...
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Pranjal Sarmah (Dibrugarh University)Track 01Oral
Isotropy and homogeneity are the two assumptions on which the standard cosmology stands. However, some observational deviations from the standard cosmological predictions have made the researchers more interested in anisotropic cosmological models. Locally rotationally symmetric Bianchi type I (LRS-BI) metric is one of the simplest yet prominent candidates to study the anisotropic...
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Happy BorgohainTrack 01Oral
Abstract:
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After classifying all the possible texture zeros in light Dirac neutrino mass matrix in diagonal charged lepton basis, we studied the phenomenology of the texture zeros that are compatible with recent neutrino data. We consider the general (non-Hermitian) nature of the neutrino mass matrix which leads to more possibilities and freedom due to additional CP phases, mixing angles not... -
Dr Atanu Nath (Tihu College, Tihu)Track 01Oral
The muon anomalous magnetic moment, denoted as aμ=(g−2)/2, serves as a crucial low-energy observable, offering an exceptional avenue for precision measurement and computational evaluation. This parameter stands as a rigorous litmus test for the Standard Model (SM) of particle physics and provides a sensitive window into potential new physics beyond the SM framework. Recent concerted efforts...
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Mr Swaraj Pratim Sarmah (Dibrugarh University)Track 01Oral
While the origins of ultra-high energy (UHE) cosmic rays remain shrouded in uncertainty, several important milestones have been reached in recent years in the experimental study of cosmic rays with energy above $10^{18}$ eV. Within the vast expanse of intergalactic space, turbulent magnetic fields (TMFs) are believed to pervade, and these fields could exert a significant influence on the...
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Dr Manoranjan DuttaTrack 01Oral
The cold, collisionless dark matter (DM) postulated in the $\Lambda CDM$ model leads to several small scale anomalies such as the cusp-core problem, the missing satellites problem and the too big to fail problem. Self-interacting dark matter (SIDM), a promising alternative type of dark matter, not only alleviates the small scale anomalies, but also matches with highly accurate large scale...
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3. Spectral and temporal properties of GX 17+2 utilizing a simultaneous view from AstroSat and NICERDr Biplob Sarkar (Department of Applied Sciences, School of Engineering, Tezpur University)Track 01Oral
We report the analysis of the Z-track neutron star (NS) low-mass X-ray binary (LMXB) GX 17+2 using the simultaneous data from the AstroSat (LAXPC/SXT) and NICER mission data. On segmenting the hardness intensity diagram (HID) into three slices—horizontal branch (HB), hard apex (HA), and normal branch (NB)- we investigate the variability of the source and its spectral state evolution throughout...
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Bidyut Hazarika (Research Scholar,Department of Physics,Dibrugarh University)Track 01Oral
In this work, we study the thermodynamic topology of a superfluid black hole solution in Horava gravity known as the Horava Lifshitz (HL) black hole in canonical ensemble. This exotic black hole solution belongs to a special class of of black holes whose thermodynamics exhibit a line of (continuous) second order phase transitions known as $\lambda$ phase transitions akin to those observed in...
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Ms Ankita Kakoti (Tezpur University)Track 01Oral
In this work, the Left-Right Symmetric Model (LRSM) has been realized with the modular group of level 3, that is, $\Gamma(3)$ and weight 2, which is isomorphic to non-abelian discrete symmetry group $A_4$. As, it is a well known fact there are physics beyond the Standard Model framework, where several phenomenological studies can be carried out. In our present work, we are concerned about the...
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Mr Hrishi Bora (Tezpur University), Prof. Ng. K. Francis (Tezpur University), Mr Animesh Barman (Tezpur University)Track 01Poster
We formulate and discuss the neutrino mass matrices for the present neutrino oscillation data. The matrices are discussed numerically in the framework of the $\Delta(54)$ flavor model with the double inverse seesaw mechanism for Majorana neutrinos. We introduced Vector like (VL) fermions which are all Standard Model gauge singlets. We use extra symmetry to constrain the unwanted terms in our...
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