Conveners
Extended session: Quantum Physics, Quantum Optics and Quantum Information
- Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))
Extended session: Cosmology, Astrophysics, Gravity, Mathematical Physics
- Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))
Extended session: Heavy Ion Collisions and Critical Phenomena
- Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))
Extended session: Particle Physics
- Evgeny Zabrodin
Extended session: Heavy Ion Collisions
- Evgeny Zabrodin
Extended session: Interdisciplinary topics
- Istvan Papp
Extended session: Posters flash talks
- Anke Lei (CCNU)
Extended session: Cosmology, Astrophysics, Gravity, Mathematical Physics
- Istvan Papp
Extended session: Heavy Ion Collisions and Critical Phenomena
- Evgeny Zabrodin
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Alexander Migdal (NYU)12/12/2024, 13:30Talk
Duality of Turbulence to String Theory
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Jelena Strišković (Josip Juraj Strossmayer University of Osijek, Department of Physics, Osijek, Croatia)12/12/2024, 14:00Talk
The Large-Sized Telescopes (LSTs) are an important part of the forthcoming Cherenkov Telescope Array Observatory (CTAO), the future cornerstone of very high-energy gamma-ray astronomy. The first LST, LST-1, was inaugurated in late 2018 on La Palma, Canary Islands, began regular gamma-ray observations in November 2019 and has so far collected more than 2000 hours of observations. The LST-1...
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Pierros Ntelis (Aix Marseille University)12/12/2024, 14:20Talk
In this contributed talk, I will discuss how to embrace information by presenting important concepts of abstract information field theory, probabilities, and probabilistic dimensions, in the view of functors of actions theories and other abstract theories. I will present a collection of manifolds and metric systems with probabilistic notions, different flavors of an expanding sub-manifold to...
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Dr Debasish Das (Saha Institute of Nuclear Physics)12/12/2024, 14:40Talk
The early universe was in a high temperature and high density environment for a very brief period after the Big Bang.In order to recreate this state of matter in the laboratory, mini bangs are created by colliding heavy ions at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory and subsequently at the Large Hadron Collider (LHC) at CERN. In this talk I shall be...
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Dr Yogesh kumar (Hansraj College, University of Delhi)12/12/2024, 15:00Talk
We investigate equation of state (EoS) of quark gluon plasma (QGP) in the presence of dynamical magnetic fields. Since it is believe that the intense magnetic field generates at BNL and CERN, we study not only the static magnetic field but also dynamic magnetic fields in order to analyse the impact of these field on EoS. We found significant altering on EoS in the presence of a magnetized...
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Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))12/12/2024, 15:30Extended sessionTalk
The instantaneous luminosity of the Large Hadron Collider at CERN will be increased by about a factor of five with respect to the design value by undergoing an extensive upgrade program over the coming decade. The largest phase-1 upgrade project for the ATLAS Muon System was the replacement of the first station in the forward regions with the New Small Wheels (NSWs) which took place during the...
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Poonam Jain (Sri Aurobindo College, University of Delhi)12/12/2024, 15:50Talk
Our analysis focuses on the Superdeformed (SD) bands in the A~130 mass region using a modified Variable Moment of Inertia (VMI) model for a comprehensive examination of band-head spin and level spins. Due to the lack of experimental data for these bands, our model primarily aims to deduce the band-head spin. By utilizing this model, we can obtain quantitative results for γ-energies and spins...
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Mr Rishav Pandey (Larsen and Toubro Limited)12/12/2024, 15:50Talk
The space-time picture of hadron formation in high-energy collisions with nuclear targets is still poorly known. The tests of hadron formation was suggested for the first stage of SPD running. They will require measuring charged pion and proton spectra with the precision better than $10\%$. A research has been carried out to check feasibility of such studies at SPD. In this work,...
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Deepalakshmi chandrasekaran12/12/2024, 16:10Talk
This proposal describes the arrangement based on the Einstein de-Haas experiment. An externally applied magnetic field magnetized the ferrite core by giving microwave power frequency to the coil around the ferrite core. Ferromagnetic resonance is achieved due to the effect of the interaction of spin precession magnetic moments due to Zeeman splitting on the macroscopic magnetization of the...
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Prof. Shougaijam Somorendro Singh (University of Delhi, Delhi, India)12/12/2024, 16:10Talk
We calculate thermodynamic free energy under one loop correction at
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finite chemical potential. Due to the effect of the chemical potential in
this one loop correction, the formation of bubble droplet is obtained with
the value of quark and gluon parametrization in the range of
q = 1/8 and
8
q ?
g ? 18
q. However the stability of the droplet is able to obtain
in the range of some... -
Ramzi Suleiman12/12/2024, 16:30Talk
We extend previous results of a relativized Newtonian dynamics derived for the case of inertial rectilinear motion, to the case of a uniformly rotating disk. The results uncover a nonluminous component coexisting with the luminous component in a dynamical duality governed solely by rotation velocity. We apply the obtained results to infer the dynamics of luminous and nonluminous matter in a...
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SHARANG RAV SHARMA (IISER Tirupati)12/12/2024, 16:30Talk
Anisotropic flow parameters $(v_{n})$ are important observables as they provide insight into the collective expansion and transport properties of the medium produced in relativistic heavy-ion collisions. Among these parameters, directed flow ($v_1$) describes the collective sideward motion of produced particles in heavy-ion collisions. It is an important probe to study the in-medium dynamics...
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Vidhi Jain12/12/2024, 17:20Poster presentation
Black holes, enigmatic cosmic entities with immense gravitational pull, remain among the most intriguing objects in astrophysics. Traditional strategies of studying them face severe obstacles in their extreme environments. This paper proposes a pioneering approach to enhance astronomical exploration of black holes using tethered probes equipped with modular sensor suites and robust backup...
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Ahsan Mehmood Khan (University of Science and Technology of China (CN))12/12/2024, 17:30Poster presentation
The study of QGP formation in RHIC experiments provides insight into the
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strong force that binds quarks and gluons, also enriching our knowledge about the conditions of the early universe. Several measurements from both small and large collision systems, examining the same observables such as strangeness enhancement across different energies, suggest QGP-like behavior in all these systems.... -
Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))12/12/2024, 17:40Extended sessionPoster presentation
Thermal model analysis of the particle source in small collision systems.
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Dr Vipul Bairathi (Instituto de Alta Investigación, Universidad de Tarapacá)12/12/2024, 17:50
Thermal model investigation of central d+Au collisions at RHIC
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Mr Keshav Jindal (Department of Physics, Hansraj College, University of Delhi)12/12/2024, 18:00Poster presentation
We study the expansion of a quark-gluon plasma (QGP) droplet in the early universe using a phenomenological model. This model employs the Friedmann approach to compute the equation of state for the QGP. Studying the behavior of the QGP droplet at non-zero chemical potentials during the early universe is challenging. Our analysis explores temperature and other thermodynamic observables,...
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Anke Lei (CCNU)12/12/2024, 18:10Poster presentation
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Rashika Rai12/12/2024, 18:20Poster presentation
We employ a phenomenological model to scrutinize the diphoton signal, a highly regarded and widely explored probe that serves as one of the premier indirect signatures of quark-gluon plasma (QGP) in relativistic heavy-ion collisions. Theoretical considerations indicate the potential existence of a finite chemical potential at RHIC, LHC, and in astrophysical environments. The existence of...
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Abdelaziz HANAIA (phD student)12/12/2024, 18:30Poster presentation
in our research, we find the solutions of klein-gordan and dirac equations considering the dunkl deformation, applying certain potentiels; using mathematical methods we solve using spherical coordinates.
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Dr Vipul Bairathi (Instituto de Alta Investigación, Universidad de Tarapacá)12/12/2024, 18:40Talk
Understanding the sources controlling the longitudinal distribution of produced particles in relativistic heavy-ion collisions is crucial for characterizing the shape of the Quark-Gluon Plasma (QGP). Previous measurements on forward-backward multiplicity correlations, directed flow, and flow decorrelations have provided strong model-dependent constraints on emission profiles of initial state...
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Mr Swapnil SinghTalk
This study examines the formation of dark matter as a result of Primordial Spacetime Cavitation, driven by Inflaton Field Perturbations. Our theoretical framework integrates early universe dynamics with quantum field theory to explain the emergence of subatomic voids within the spacetime fabric. These cavitated regions, resulting from perturbations in the inflaton field, persist as stable or...
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Ms nour Abdulameer (Wigner Fizikai Kutatóközpont)Talk
This study investigates the outcomes of laser-induced crater formation experiments, focusing on data evaluation to understand the underlying physical mechanisms and material responses. By employing high-powered laser pulses on various target materials, craters of different sizes and characteristics were generated. Detailed analysis of the crater morphology was conducted using advanced imaging...
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Ms Anju Sharma (Aligarh Muslim University)Talk
Exploring the QCD phase diagram and searching for the critical point is one of the primary goals of relativistic heavy-ion collisions. It is believed that near the critical point, the fluctuations in conserved quantities and larger number density fluctuation near the critical point region are strong indicators of the phase transition. Under thermodynamic limits, the correlation length diverges...
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Sibaram Behera (IISER Tirupati)Talk
In heavy-ion collisions, the production mechanism of light (anti-)nuclei can be explained by either the thermal model or the coalescence model. By studying the yields and yield ratios of the light (anti-)nuclei, we can gain a better understanding of their production mechanisms and the properties of the expanding system during freeze-out. Additionally, it has been proposed that the enhancement...
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Şeyda Demirok (Sabancı University)Talk
The long-term evolution of the neutron stars with fallback disks depends on their initial conditions, namely the initial period of the star, P0, the mass of the disk, Md, and the magnetic dipole field at the poles of the star, B0. There are three basic evolutionary paths characterized by the sequences of the rotational phases (weak propeller or strong propeller) that can be followed by a...
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Divyesh Viththani (PDPIAS)Talk
Our study investigates the gravitational field surrounding a charged, non-vacuum, non-rotating, spherically symmetric compact object with mass M and charge Q. Our investigation is based on a static solution to the Einstein-Maxwell field equations. We have shown the characteristics of perihelion precession within the orbits governed by the charged naked singularity spacetime. We uncover novel...
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Michael Schernau (Instituto De Alta Investigación, Universidad de Tarapacá (CL))Talk
Performance of the Small-strip Thin Gap Chambers in the New Small Wheels of ATLAS
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Jelena Strišković (Josip Juraj Strossmayer University of Osijek, Department of Physics, Osijek, Croatia)Talk
Some candidates for the theory of quantum gravity allow for Lorentz invariance violation (LIV). If Lorentz's invariance is violated, it may cause an observable effect on the light curve and spectra of very high energy (VHE, E > 100 GeV) photons coming from cosmic sources. One of the possible consequences of the LIV is in-vacuo dispersion which implies that the photon group velocity is energy...
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