Conveners
Parallel: DM + neutrino: Day 2 Afternoon Session 1
- Arindam Chatterjee (Shiv Nadar Institution of Eminence (Deemed to be University))
Parallel: DM + neutrino: Day 2 Afternoon Session 2
- S Mitra
Parallel: DM + neutrino: Day 3 Afternoon Session 1
- Sukanta Dutta (SGTB Khalsa College, University of Delhi.)
Parallel: DM + neutrino: Day 3 Afternoon Session 2
- Mamta Dahiya (S.G.T.B. Khalsa College, University of Delhi)
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Anirban Karan19/12/2023, 14:30Talk
Though the Standard Model assumes the neutrinos to be massless, the phenomenon of neutrino oscillation shows that they have tiny but non-zero masses. Scotogenic models, in which neutrino masses are generated at one-loop level and remain tiny due to loop suppression, are very interesting in this regard. In these models, since the beyond Standard Model (BSM) particles entering inside the...
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Dr Khushboo Dixit (Centre for Astro-Particle Physics, University of Johannesburg)19/12/2023, 14:50Talk
Neutrino flavor oscillation is a widely studied physical phenomenon with significant implications for our understanding of particle physics and the search for physics beyond the standard model. Oscillation arises due to the mixing between flavor and mass eigenstates, and their evolution over time. It is a quantum system where flavor transitions are typically studied using probabilistic...
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Dr Purusottam Ghosh (Indian Association for the Cultivation Of Science, Kolkata)19/12/2023, 15:10Talk
In this talk, I will demonstrate how having two WIMPs, each with different masses, and mass splitting with the NLSP, generated at a collider through a decay chain, can result in double peaks in the missing energy or missing transverse momentum distribution of the multilepton signal. I will also outline a set of criteria to identify and segregate the second peak in the missing energy spectrum,...
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Ms Lipika Kolay (IIT Guwahati)19/12/2023, 15:30Talk
We constrain the parameter space of a simplified fermionic dark matter model with a spin-0 mediator from low energy processes. FCNC observables like neutral pseudoscalar meson mixing, rare decays of $ B_0, B_s^0, K $ meson, global fit of all the $ b \to s \ell \ell $ observables, invisible decays of B and K meson are considered along with FCCC observables like $ t \to b W_{\mu} $ anomalous...
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Nayan Das (Indian Institute of Technology, Guwahati)19/12/2023, 15:45Talk
We study a scenario where origin of dark matter is related to the Dirac nature of neutrino, known as the light Dirac neutrino portal dark matter (DNPDM). In such DNPDM set up, light dirac neutrinos take the role of mediating the interactions between dark matter (DM) and standard model (SM) bath. Here, we consider a UV complete model in gauged B-L framework extended by three species of right...
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Noel Jobu (Shiv Nadar University)19/12/2023, 16:30Talk
In this study, we propose a new version of the Scotogenic model, it is an economically appealing theoretical framework which addresses two problems of particle physics, neutrino mass generation and dark matter. The Scotogenic model generates neutrino mass via a $1$-loop Feynman diagram by extending the standard model by the $Z_2$ discrete symmetry.
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In our model, we extend the standard model... -
Mr Anirban Majumdar (Indian Institute of Science Education and Research - Bhopal)19/12/2023, 16:45Talk
In recent years, there has been a growing interest in the direct detection of sub-GeV dark matter, which is theoretically well-motivated. However, probing sub-GeV cold dark matter particles has posed a persistent challenge, as their typical momenta are insufficient to induce recoils above the thresholds of conventional direct detection experiments. Notably, even very strongly interacting dark...
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Soumen Kumar Manna19/12/2023, 17:00Talk
We show that Majoron, the pseudo-Nambu-Goldstone boson resulting from the spontaneous breaking of global lepton number symmetry, can present itself as a viable freeze-in type of dark matter in a mass range keV-GeV, thanks to the explicit higher dimensional Lepton number breaking operator. Interestingly, the proposal is restricted within the simplest extension of the Standard Model with two...
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Mr Sushant Yadav (IISER Bhopal, India)19/12/2023, 17:15Talk
The Dirac scotogenic model provides an elegant mechanism which explains small Dirac neutrino masses and neutrino mixing with a single symmetry simultaneously protecting the ''Diracness'' of the neutrinos and the stability of the dark matter candidate. In addition to exploring the phenomenology of dark matter, we will also investigate the implications for lepton flavor violation, the muon...
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Mr Dipankar Pradhan (IIT Guwahati)19/12/2023, 17:30Talk
In a two-component dark matter (DM) set-up, when DM$_1$ is in equilibrium with the thermal bath, the other one, DM$_2$, can be equilibrated only by the sizeable interaction with the DM$_1$, even without any connection with the visible-sector particles. We affirm that such DM candidates (DM$_2$) have unique `freeze-out' characteristics impacting the relic density, direct, indirect and collider...
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Saurabh Niyogi (Harish-Chandra Research Institute)19/12/2023, 17:45
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Vicky Singh Thounaojam (Indian Institute of Technology, Hyderabad)20/12/2023, 14:30Talk
In this work, we explore the intriguing possibility of connecting self-interacting dark matter (SIDM) with the recently observed exceptionally bright and long-duration gamma-ray burst (GRB221009A). The proposed minimal scenario involves a light scalar mediator, simultaneously enabling dark matter (DM) self-interaction and explaining the observed very high energy photons from GRB221009A...
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Sujit Kumar Sahoo (Indian Institute of Technology Hyderabad)20/12/2023, 14:45Talk
We study the possibility of generating light Dirac neutrino mass via scotogenic mechanism where singlet-doublet fermion dark matter (DM) plays non-trivial role in generating one-loop neutrino mass, anomalous magnetic moment of muon $(g-2)_\mu$ as well as additional relativistic degrees of freedom $\Delta{N_{\rm eff}}$ within reach of cosmic microwave background (CMB) experiments. We show that...
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Mr Dibyendu Chakraborty (Shiv Nadar Institution of Eminence)20/12/2023, 15:00Poster
Extra dimensional models are very popular and useful framework to address
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many important problems in particle physics. On the other hand extension of the Standard Model (SM) with an extra U(1)Lmu−Ltau gauge group is a great motivation to solve muon (g-2) anomaly (recently 5.1 sigma deviation). Here we considered an extra dimensional U(1)Lmu − Ltau model where only the Kaluza-Klein (KK) modes... -
Dipendu Bhandari20/12/2023, 15:15Talk
We propose that electroweak baryogenesis (EWBG) scenario can be operative with the help of an additional SM scalar singlet which is not only responsible for making the electroweak phase transition strongly of first order but also acts as a mediator between the SM and a dark sector. The dark sector is equipped with a singlet-doublet fermion framework that, apart from explaining the observed...
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Mr Prabhat Butola (Homi Bhabha National Institute, Mumbai & The Institute of Mathematical Sciences, Chennai)20/12/2023, 15:30Talk
In a scattering process in a thermal plasma, thermal fluctuation alongside with quantum fluctuation affects the annihilation cross section of particles. This is important in the context to dark matter annihilation cross section since the relic densities are now being more precisely measured. We investigate the effect of thermal fluctuation on the annihilation cross section of a $SU(2) \times...
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Syed Adil Pasha (Shiv Nadar Institution of Eminence, Greater Noida)20/12/2023, 15:45Talk
The lightest Neutralino is a good Dark Matter (DM) candidate
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in the R-parity conserving Minimal Supersymmetric Standard Model (MSSM). In this work, we consider light Higgsino-like Neutralino as the Lightest
Stable Particle (LSP), thanks to a relatively small $\mu$ parameter. We then estimate the prominent radiative corrections to the Neutralino-Neutralino-Higgs boson vertices.
We show that... -
Mr Ranjeet Kumar (Department of Physics, Indian Institute of Science Education and Research - Bhopal)20/12/2023, 16:30Talk
Modular symmetries offer a dynamic approach to understanding the flavour structure of leptonic mixing. Using the modular $\mathcal{A}_4$ flavour symmetry integrated in a type-II seesaw, we propose a simple and minimalistic model that restricts the neutrino oscillation parameter space and, most importantly, introduces a sum rule in the physical neutrino masses. When combined with the mass...
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Arindam Basu (SRM University AP Andhra Pradesh)20/12/2023, 16:45Talk
We study the two-component boosted dark matter (DM) scenario in a neutrinophilic two-Higgs doublet model (ν2HDM), which comprises one extra Higgs doublet with a MeV scale CP-even scalar H. This model is extended with a light (∼ 10 MeV) singlet scalar DM ϕ3, which is stabilized under the existing Z2 symmetry and can only effectively annihilate through scalar H. As the presence of a light H...
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Rahul Dhyani (Shiv Nadar Institution of Eminence (Deemed to be University))20/12/2023, 17:00Talk
Cosmological observations offer valuable methods for probing various characteristics of Dark Matter (DM). We examine the cosmological implications of higher-dimensional Non-Relativistic Effective Field Theory (EFT) operators for Dark Matter(DM) - electron interactions. We focus on velocity-independent operators and simultaneously incorporate DM-electron scattering and DM annihilation into...
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Pratick Sarkar (Indian Association for the Cultivation of Science)20/12/2023, 17:15Poster
In this study, we examine the phenomenon of photon axion conversion occurring in the spacetime surrounding a black hole. Observations of the black hole in the center of the M87 galaxy (M87 * ) through the Event Horizon Telescope imaged polarized synchrotron emission at 230 GHz on event horizon scales. Specifically, we focus on the potential existence of a magnetic field around the supermassive...
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