Conveners
Plenary: Plenary 1
- Shantanu Desai
Plenary: Plenary 2
- Saurabh Sandilya
Plenary: Plenary 3
- Narendra Sahu
Plenary: Plenary 4
- Bindu Bambah
Plenary: Plenary 5
- Amol Dighe
Plenary: Plenary 6
- Rukmani Mohanta
Plenary: Plenary 7
- Raghavan Rangarajan
Plenary: Plenary 8
- Santosh K Rai
Plenary: Plenary 9
- Saranya S Ghosh
Plenary: Plenary 10
- Priyotosh Bandyopadhyay
Plenary: Plenary 11
- Soma Sanyal
Plenary: Plenary 12
- E Harikumar
Plenary: Plenary 13
- Gagan B Mohanty
Plenary: Plenary 14
- Anjan Giri
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Prof. Dan Hooper (University of Wisconsin, Madison)10/14/24, 9:00โฏAM
I will discuss the state and of high-energy and multi-messenger astrophysics, and consider the exciting prospects for this field moving forward.
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L Sriramkumar10/14/24, 9:30โฏAM
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Krishnakumar M. A. (Radio Astronomy Centre, NCRA-TIFR, Ooty)10/14/24, 10:00โฏAMParallel talk
On June 29, 2023, the five regional PTAs, including the Indian pulsar timing array (InPTA) announced the evidence for the presence of gravitational waves (GWs) in the nano-Hz frequency regime. This was the first evidence for GWs outside the frequency range of those detected by the ground-based observatories. Currently the international PTA community is gearing towards the analysis of the data...
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Matthias Danninger10/14/24, 11:00โฏAM
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Brij Kishor Jashal (IFIC Valencia, RAL Oxford and TIFR Mumbai,)10/14/24, 11:30โฏAMPlenary
The Large Hadron Collider beauty (LHCb) experiment has played a pivotal role in advancing our understanding of particle physics, particularly in the study of heavy quarks and their interactions. This talk will present the latest highlights from LHCb, including groundbreaking results in the areas of flavor physics, CP violation, and rare decays. We will discuss recent measurements that...
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Takashi Yamanaka10/14/24, 12:00โฏPM
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Bipul Bhuyan10/14/24, 12:25โฏPM
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John Ellis10/14/24, 2:15โฏPM
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Pravata Mohanty10/14/24, 2:45โฏPM
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Mala Das10/14/24, 3:10โฏPM
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Shailaja Mohanty10/14/24, 3:35โฏPM
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Sara Rebecca Gozzini10/14/24, 4:30โฏPM
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Venktesh Singh10/14/24, 4:50โฏPM
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Dr Aparajita Mazumdar (Los Alamos National Laboratory)10/14/24, 5:10โฏPMParallel talk
Whether the neutrino is a Majorana particle, i.e., whether it is its own antiparticle, remains an important open problem in modern physics. The observation of the hypothesized second order weak decay, Neutrinoless Double Beta Decay (0$\nu\beta\beta$) would conclusively establish the Majorana nature of neutrinos. It would also demonstrate lepton number violation and could provide insight into...
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Srubabati Goswami10/15/24, 9:00โฏAM
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Frank Deppisch10/15/24, 9:30โฏAM
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Prof. Sanjib Kumar Agarwalla (Institute of Physics, Bhubaneswar, Odisha, India)10/15/24, 10:00โฏAMPlenary
The IceCube Neutrino Observatory is a flagship cubic-kilometer neutrino detector made up of transparent, natural Antarctic ice at the South Pole, which is instrumented with digital optical modules to detect Cherenkov light emitted during interactions of neutrinos with energies spanning more than 10 orders of magnitude. It is a unique multidisciplinary facility that has produced several...
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Julia Harz10/15/24, 11:00โฏAM
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Sudip Jana10/15/24, 11:30โฏAM
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Chandan Hati10/15/24, 12:00โฏPM
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Subhendu Rakshit10/15/24, 12:25โฏPM
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Sukanta Bose10/16/24, 9:00โฏAM
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Chelsea Bartram10/16/24, 9:30โฏAM
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Ramon Miquel10/16/24, 10:00โฏAM
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Bhupal Dev10/16/24, 11:00โฏAM
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Soumya Mohanty10/16/24, 11:30โฏAM
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Jan Hamann10/16/24, 12:00โฏPM
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Suchita Kulkarni10/16/24, 12:25โฏPM
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Sanjay Swain10/17/24, 9:00โฏAM
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Zeeshan Ahmed10/17/24, 9:30โฏAM
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Shouvik Roy Chowdhury10/17/24, 10:00โฏAM
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Qader Dorosti10/17/24, 11:10โฏAM
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Jong-Chul Park10/17/24, 11:40โฏAM
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Anish Ghoshal10/17/24, 12:05โฏPMPlenary
We will discuss interpretation of the nHz stochastic gravitational wave background (SGWB) seen by NANOGrav and other Pulsar Timing Array (PTA) Collaborations in the context of supermassive black hole (SMBH) binaries. The frequency spectrum of this stochastic background is predicted more precisely than its amplitude. We will discuss how Dark Matter friction can suppress the spectrum around nHz...
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Nirmal Raj10/17/24, 12:30โฏPM
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Kenny Ng10/17/24, 2:15โฏPM
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Seodong Shin10/17/24, 2:40โฏPM
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Mohamed Rameez10/17/24, 3:05โฏPM
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Maura Ramirez Quezada10/17/24, 3:30โฏPM
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Rahul Srivastava10/17/24, 4:25โฏPM
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Marco Taoso10/17/24, 4:50โฏPM
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Valentina De Romeri10/17/24, 5:10โฏPM
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Shohei Nishida10/18/24, 9:00โฏAMPlenary
Belle II is a flavor physics experiment at the asymmetric electron-positron collider SuperKEKB at KEK in Japan. Belle II aims to record an order of magnitude more data than the previous Belle experiment. Belle II started operation in 2019 and has accumulated 530 fb${}^{-1}$ of data to date. I will present recent results from Belle II with a focus on BSM searches, including the first evidence...
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Michael Schmidt10/18/24, 9:30โฏAM
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Myriam Mondragรณn10/18/24, 10:00โฏAM
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Ranjan Laha10/18/24, 11:00โฏAM
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Gaurav Tomar10/18/24, 11:25โฏAM
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Eung Jin Chun10/18/24, 11:50โฏAM
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Sridhara Dasu10/18/24, 12:15โฏPM
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Eung Jin Chun
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Eung Jin Chun
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Suchita Kulkarni
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Jan Hamann (The University of New South Wales)Plenary
How can we decide which cosmological model is the most probable? In a Bayesian approach to statistics, this question can be readily answered using the framework of Bayesian model selection: namely by calculating a model's evidence. However, the numerical evaluation of the evidence can be a numerically difficult task.
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I will introduce a new, efficient machine-learning approach to this... -
Dr Sudip Jana (Max-Planck-Institut fรผr Kernphysik)Plenary
After a brief introduction to neutrino electromagnetic properties, I will focus on the correlation between neutrino magnetic moment and neutrino mass mechanism. Then, I will discuss that the models that induce large neutrino magnetic moments while maintaining their small masses naturally also predict observable shifts in the charged lepton anomalous magnetic moment by showing that the...
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Anish Ghoshal
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Dr Gaurav Tomar (IIT Patna)Parallel talk
Recently, the Migdal effect has been used along with nuclear direct detection experiments to constrain dark matter models in the sub-GeV region, providing a complementary approach to electron and standard nucleus scattering analyses. By utilizing the Migdal effect with data from the XENON1T and DarkSide-50 experiments, we constrained the electromagnetic interactions of dark matter with visible...
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Shailaja Mohanty
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Shailaja Mohanty (Institute for Astroparticle Physics, Karlsruhe Institute of Technology)Parallel talk
Neutrinos are known to have non-zero masses, as shown by oscillation observations, but their absolute mass scale remains unknown. Observational cosmology and neutrinoless double beta decay experiments derive sub-eV upper limits. Complementing these efforts with a model-independent approach based on beta-decay kinematics, the Karlsruhe Tritium Neutrino (KATRIN) experiment provides the most...
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Shohei Nishida
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Eung Jin Chun (Korea Institute for Advanced Study)Plenary
We propose a scenario where a heavy RHN DM can be produced by a thermal effect undergoing a resonance at high temperature in the early Universe
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Aparajita Mazumdar
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Aparajita Mazumdar
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Brij K Jashal
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Sanjib Kumar Agarwalla
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Dan HooperPlenary
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Anjan Giri
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Dr Valentina De Romeri (IFIC CSIC/UV (Valencia, Spain))Parallel talk
If produced in the early Universe with an initial mass of โผ 10^15 g, PBHs are expected to evaporate at the present time producing sizable fluxes of particles in their last instants. These โexplodingโ black holes will emit bursts of Standard Model particles as well as new degrees of freedom, if present. We explore the possibility that HNLs mixing with the active neutrinos are emitted in the...
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Prof. Frank DeppischPlenary
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Pravata Kumar Mohanty (Tata Institute of Fundamental Research)Plenary
The GRAPES-3 experiment setup at an altitude of 2200 m in Ooty, India, employs a dense array of plastic scintillator detectors complemented with a large-area tracking muon detector. It is designed to observe shower particles which mostly include gamma rays, electrons and muons produced by interactions of primary cosmic rays and gamma rays in Earthโs atmosphere. Recently, GRAPES-3 successfully...
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Dr Marco Taoso (Istituto Nazionale di Fisica Nucleare, Torino, Italy)Parallel talk
The coupling of axion and axion-like particles (ALPs) to two photons leads to radiative decays of axion dark matter and axion-photon conversion in an external magnetic field. We discuss two methods to search for these signals exploiting astrophysical data. The first is based on MUSE spectroscopic optical observations of a sample of five classical and ultra-faint dwarf spheroidal galaxies.
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Suchita Kulkarni (University of Graz)Plenary
I will take a brief overview of the recent developments in the field of strongly interacting dark matter. I will discuss new ways to generate dark matter relic density as well as discuss associated detection strategies.
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Anupam Mazumdar
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Venktesh Singh (Central University of South Bihar Gaya (India))Parallel talk
The TEXONO collaboration has been producing world-class results related to reactor neutrinos and dark matter for more than two decades. In this conference, I will discuss the results obtained by the TEXONO experiment based on neutrino-nucleus coherent scattering and will discuss in detail the current status and future plans of the collaboration.
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Pratika Dayal
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Mala DasParallel talk
The InDEx (Indian Dark matter search Experiment) is aimed to search the dark matter directly by the recoil nucleus formed due to the elastic scattering of WIMP with the nuclei of superheated droplet detector. The superheated droplet detector has been installed at Jaduguda Underground Science Laboratory (JUSL) at UCIL, Jaduguda mine, Jharkhand at 555m deep underground. The active...
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MA Krishnakumar
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Sara Rebecca Gozzini
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Sara Rebecca GozziniParallel talk
KM3NeT is a multi-purpose neutrino observatory under construction in the Mediterranean Sea. It is composed of two Cherenkov detectors with different designs: ORCA, a compact and dense detector optimised for the high-statistic measurement of atmospheric neutrino physics in the 1-100 GeV energy range, and ARCA, instrumenting a cubic kilometre to catch fluxes of extraterrestrial neutrinos from...
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Prof. Nirmal Raj (Indian Institute of Science)Parallel talk
I identify the maximum cross sections probed by single-scatter ``WIMP'' searches in dark matter direct detection. Due to Poisson fluctuations in scatter multiplicity, these ceilings scale logarithmically with mass for heavy dark matter and often lie in regions probed by multiscatter searches. I will present a generalized formula for single-scatter event rates, and use it to recast WIMP...
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Qader Dorosti Hasankiadeh (Universitaet Siegen (DE))Plenary
The Pierre Auger Observatory, the worldโs largest cosmic-ray detector, continues to make significant advances in the study of ultra-high-energy cosmic rays (UHECRs). By utilizing a hybrid detection system of surface and fluorescence detectors, the Observatory has made substantial contributions to our understanding of UHECR origins, composition, and energy spectrum, offering a consistent...
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