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Imaging the cosmic 21 cm signal will map out the first billion years of our Universe. The resulting 3D lightcone (LC) will encode the properties of the unseen first galaxies and physical cosmology. Here, we build on previous work using…

宇宙学与河外天体物理 · 物理学 2022-02-17 David Prelogović , Andrei Mesinger , Steven Murray , Giuseppe Fiameni , Nicolas Gillet

We consider the gravitational lensing produced by long cosmic strings formed in a GUT scale phase transition. We derive a formula for the deflection of photons which pass near the strings that reduces to an integral over the light cone…

天体物理学 · 物理学 2009-10-30 Andrew A. de Laix

We study photoabsorption reaction and real Compton scattering (RCS) within the color dipole model. We rely on a photon wave function derived in the instanton vacuum model, and on the energy dependent phenomenological elastic dipole…

高能物理 - 唯象学 · 物理学 2009-09-24 B. Z. Kopeliovich , Ivan Schmidt , M. Siddikov

We find exact conditions for the enhancement or suppression of internal and/or scattered fields and the determination of their spatial distribution or angular momentum through the combination of simple fields. The incident fields can be…

光学 · 物理学 2015-06-16 Benjamin Hourahine , Francesco Papoff

The theoretical and experimental aspects of particle production from the strong equivalent photon fluxes present at high energy hadron colliders are reviewed. The goal is to show how photons at hadron colliders can improve what we have…

高能物理 - 唯象学 · 物理学 2010-01-27 Joakim Nystrand

This document describes the concept of a primary electron beam facility at CERN, to be used for dark gauge force and light dark matter searches. The electron beam is produced in three stages: A Linac accelerates electrons from a…

加速器物理 · 物理学 2018-06-01 T. Åkesson , Y. Dutheil , L. Evans , A. Grudiev , Y. Papaphilippou , S. Stapnes

In this paper we study the direct production of the diphoton resonance $X$ which has been suggested by 2015 data at the LHC, in $e^+e^-\to X\gamma/XZ$ processes at the ILC. We derive an analytic expression for the scattering amplitudes of…

高能物理 - 唯象学 · 物理学 2016-11-23 Junping Tian , Keisuke Fujii , Hiroshi Yokoya

Scanning real-life scenes with modern registration devices typically give incomplete point cloud representations, mostly due to the limitations of the scanning process and 3D occlusions. Therefore, completing such partial representations…

计算机视觉与模式识别 · 计算机科学 2021-02-12 Przemysław Spurek , Artur Kasymov , Marcin Mazur , Diana Janik , Sławomir Tadeja , Łukasz Struski , Jacek Tabor , Tomasz Trzciński

We present our recently developed {\em galcon} approach to hydrodynamical cosmological simulations of galaxy clusters - a subgrid model added to the {\em Enzo} adaptive mesh refinement code - which is capable of tracking galaxies within the…

宇宙学与河外天体物理 · 物理学 2015-05-18 Yinon Arieli , Yoel Rephaeli , Michael L. Norman

We present a newly developed code that allows simulations of optical observations of galaxy fields with a variety of instruments. The code incorporates gravitational lensing effects and is targetted at simulating lensing by galaxy clusters.…

We present a detailed phenomenological analysis of single-inclusive hadron production at the CERN-LHC in both proton-proton and proton-lead collisions. First data from the LHC experiments on charged hadron spectra are compared to…

高能物理 - 唯象学 · 物理学 2014-11-21 M. Stratmann , R. Sassot , P. Zurita

Previous work on calculating energy spectra from Compton scattering events has either neglected considering the pulsed structure of the incident laser beam, or has calculated these effects in an approximate way subject to criticism. In this…

We present a computational framework for "painting" galaxies on top of the Dark Matter Halo/Sub-Halo hierarchy obtained from N-body simulations. The method we use is based on the sub-halo clustering and abundance matching (SCAM) scheme…

宇宙学与河外天体物理 · 物理学 2024-02-15 Tommaso Ronconi , Andrea Lapi , Matteo Viel , Alberto Sartori

This paper describes the concept of a primary electron beam facility at CERN, to be used for dark gauge force and light dark matter searches. The electron beam is produced in three stages: A Linac accelerates electrons from a photo-cathode…

加速器物理 · 物理学 2019-05-21 T. Åkesson , R. Corsini , Y. Dutheil , L. Evans , B. Goddard , A. Grudiev , A. Latina , Y. Papaphilippou , S. Stapnes

The gravitational lensing signal produced by a galaxy or a galaxy cluster is determined by its total matter distribution, providing us with a way to directly constrain their dark matter content. State-of-the-art numerical simulations…

宇宙学与河外天体物理 · 物理学 2023-11-27 Giulia Despali , Felix M. Heinze , Claudio Mastromarino

The study of hadronic showers, which are produced by cosmic rays penetrating the Earth's atmosphere, is essential for shedding light on the origins and characteristics of high-energy particles originating from space and reaching our planet.…

高能物理 - 实验 · 物理学 2024-02-22 Michael Pitt

The event generator Sibyll can be used for the simulation of hadronic multiparticle production up to the highest cosmic ray energies. It is optimized for providing an economic description of those aspects of the expected hadronic final…

高能物理 - 唯象学 · 物理学 2015-10-05 Felix Riehn , Ralph Engel , Anatoli Fedynitch , Thomas K. Gaisser , Todor Stanev

Lightcone observations are the natural data format of galaxy surveys, but their evolving geometry breaks the translational symmetry assumed by standard convolutional neural networks (CNNs). In particular, applying CNNs to 3D gridded…

宇宙学与河外天体物理 · 物理学 2026-03-30 Min Zhiwei , Xiao Xu , Jiang Zhujun , Xiao Liang , Yin Fenfen , Ding Jiacheng , Miao Haitao , Chen Shupei , Lin Qiufan , Wang yang , Zhang Le , Li XiaoDong

Details of various unknown physical processes during the cosmic dawn and the epoch of reionization can be extracted from observations of the redshifted 21-cm signal. These observations, however, will be affected by the evolution of the…

宇宙学与河外天体物理 · 物理学 2015-08-14 Raghunath Ghara , Kanan K. Datta , T. Roy Choudhury

Extended source effects can be seen in gravitational lensing events when sources cross critical lines. Those events probe the stellar intensity profile and could be used to measure limb darkening coefficients to test stellar model…

天体物理仪器与方法 · 物理学 2019-08-14 Hans J. Witt , F. Atrio-Barandela