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Pedro Alvarez28/08/2023, 21:35
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Aritra Kumar Gon (Tata Institute of Fundamental Research)28/08/2023, 21:35
We introduce a new pairwise estimator for observing the polarised kinetic Sunyaev Zeldovich (pkSZ) effect arising from the transverse peculiar velocity of galaxy clusters. The pkSZ effect is a second-order effect in the peculiar velocities of the clusters and has a frequency spectrum that can be decomposed into y-type and blackbody components, whereas the unpolarised linear kSZ effect has a...
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Polo Infante28/08/2023, 21:35
Reionization of hydrogen in the intergalactic medium (IGM) is a landmark in structure formation. Redshift z ~ 7 is the frontier in Lyalpha and reionization studies and appears to be in the middle of reionization. In the “LAGER” project (Lyman-Alpha Galaxies in the Epoch of Reionization), we take deep narrowband images to identify Lyalpha emission at z ~ 7. In this poster we present several...
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Christian Beck (Queen Mary, University of London)28/08/2023, 21:35
Motivated by the recent developments of cosmological models that are based on generalized entropies rather than Boltzmann-Gibbs entropy, we consider stochastically quantized self-interacting scalar fields as suitable models for dark energy. These fields shift information and effectively maximize Tsallis entropy with entropic index q=3. Second quantization effects lead to new and unexpected...
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Yi-Kuan Chiang28/08/2023, 21:35
The widely used Milky Way dust reddening map, the Schlegel, Finkbeiner, & Davis (1998, SFD) map, was found to contain extragalactic large-scale structure (LSS) imprints (Chiang & Ménard 2019). Such contamination is inherent in maps based on infrared emission, which pick up not only Galactic dust but also the cosmic infrared background (CIB). When SFD is used for extinction correction,...
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Valentina Cesare (Istituto Nazionale di Astrofisica (INAF) - Osservatorio Astrofisico di Catania)28/08/2023, 21:35
We test Refracted Gravity (RG) [1] by investigating the dynamics of disk galaxies in the Disk Mass Survey (DMS) [2,3,4] and of three elliptical E0 galaxies in the SLUGGS survey [3,4,5] without the aid of dark matter. RG reproduces the rotation curves, the vertical velocity dispersions, and the observed Radial Acceleration Relation (RAR) of DMS galaxies and the root-mean-square (RMS) velocity...
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Vipin kumar Sharma (Department of Physics, University of Lucknow, India)28/08/2023, 21:35
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Oksana Iarygina (Nordita)28/08/2023, 21:35
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Natasha Lavis (SARAO, University of the Witwatersrand)28/08/2023, 21:35
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Johnatan Osvaldo Román Herrera28/08/2023, 21:35
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Mousumi Das28/08/2023, 21:35
We present a study to measure the the shape of dark matter halos of gas rich galaxies that have extended HI disks. We have assumed that the halo axes ratios in the disk plane are approximately so that q=c/a measures the halo prolateness or oblatelness. We have applied our model to a sample of 20 nearby galaxies that are gas rich and close to face-on. We have used the stacked HI velocity...
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Luis Ureña-López28/08/2023, 21:35
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Abdel Nasser Tawfik (ENHEP Egyptian Network of High Energy Physics (EG)), Prof. Abdel Nasser Tawfik (Future University in Egypt (FUE)), Abdel Tawfik (ECTP)
Aiming at unifying General Relativity (GR) and Quantum Mechanics (QM), we apply Born reciprocity and the Relativistic Generalized Uncertainty Principle (RGUP). A novel estimation of the fundamental tensor in discretized curved spacetime is thereby suggested. To this end, Riemann geometry is extended to incorporate the distance-momentum duality symmetry and implement the minimum measurable...
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Chandra Shekhar Murmu
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