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Intrabeam scattering refers to the effects of the Coulomb interaction acting between pairs of charged particles within a bunch in an accelerator. One of the main consequences of intrabeam scattering is a change in the emittances of a bunch:…

加速器物理 · 物理学 2026-02-13 Andrzej Wolski

Molecular clouds act as primary targets for cosmic-ray interactions and are expected to shine in gamma-rays as a by-product of these interactions. Indeed several detected gamma-ray sources both in HE and VHE gamma-rays (HE: 100 MeV < E <…

高能天体物理现象 · 物理学 2015-06-12 G. Pedaletti , D. F. Torres , S. Gabici , E. de Oña Wilhelmi , D. Mazin , V. Stamatescu

The formation of beam halos has customarily been described in terms of a particle-core model in which the space-charge field of the oscillating core drives particles to large amplitudes. This model involves parametric resonance and predicts…

加速器物理 · 物理学 2009-11-10 Courtlandt L. Bohn , Ioannis V. Sideris

We present a dynamical model describing how halo particles can receive a significant energy kick from the merger between their own host halo and a target halo. This is highly relevant for understanding the growth of cosmological halos, and…

星系天体物理 · 物理学 2015-06-22 Johan Samsing

We present neutron scattering measurements of the atomic momentum distribution, n(k), in solid helium under a pressure p = 41 bars and at temperatures between 80 mK and 500 mK. The aim is to determine whether there is Bose-Einstein…

统计力学 · 物理学 2009-11-13 S. O. Diallo , J. V. Pearce , R. T. Azuah , O. Kirichek , J. W. Taylor , H. R. Glyde

The question is investigated whether the anomalous Hall effect (AHE) in Fe films is due to skew scattering or side jump. For this purpose sandwiches of FeIn are investigated in which the conduction electrons carry their drift velocity…

介观与纳米尺度物理 · 物理学 2007-05-23 Gerd Bergmann , Manjiang Zhang

The LHAASO Collaboration has recently reported a measurement of the diffuse gamma-ray emission from the Galactic Plane at energies between 10 TeV and 1 PeV. While this emission is brighter than that expected from cosmic-ray interactions in…

高能天体物理现象 · 物理学 2024-10-18 Ariane Dekker , Ian Holst , Dan Hooper , Giovani Leone , Emily Simon , Huangyu Xiao

Collimation systems in particle accelerators are designed to dispose of unavoidable losses safely and efficiently during beam operation. Different roles are required for different types of accelerator. The present state of the art in beam…

加速器物理 · 物理学 2016-08-11 S. Redaelli

Formation of halos in the Dark Ages from initial spherical perturbations is analyzed in a four component Universe (dark matter, dark energy, baryonic matter and radiation) in the approximation of relativistic hydrodynamics. Evolution of…

宇宙学与河外天体物理 · 物理学 2019-10-29 Bohdan Novosyadlyj , Valerii Shulga , Wei Han , Yurij Kulinich , Maxym Tsizh

Pulsar halos are extended gamma-ray structures generated by electrons and positrons escaping from pulsar wind nebulae (PWNe), considered a new class of gamma-ray sources. They are ideal indicators for cosmic-ray propagation in localized…

高能天体物理现象 · 物理学 2022-09-28 Kun Fang

Relativistically-intense laser beam with large field gradient ("laser gate") enables strong inelastic scattering of electrons crossing the beam. This process allows for multi-MeV electron net acceleration per pass within the wavelength…

原子物理 · 物理学 2009-06-04 A. E. Kaplan , A. L. Pokrovsky

Context. The recent discovery of so-called mega radio halos as a new class of diffuse, steep-spectrum radio sources in clusters of galaxies has raised questions about the origin and the evolution of cluster-wide radio emission. Aims. We…

高能天体物理现象 · 物理学 2024-10-02 Luca Beduzzi , Franco Vazza , Virginia Cuciti , Gianfranco Brunetti , Marcus Brüggen , Denis Wittor

Collisionless dark matter galactic halos are expected to exhibit damped oscillations as a result of ongoing late time accretion. An n-body model of the cosmological assembly of a Milky Way-like halo is used to quantify the time dependence…

星系天体物理 · 物理学 2020-01-08 Raymond G. Carlberg

Dark matter haloes have long been recognized as one of the fundamental building blocks of large scale structure formation models. Despite their importance -- or perhaps because of it! -- halo definitions continue to evolve towards more…

宇宙学与河外天体物理 · 物理学 2023-03-15 Rafael Garcia , Edgar Salazar , Eduardo Rozo , Susmita Adhikari , Han Aung , Benedikt Diemer , Daisuke Nagai , Brandon Wolfe

We present a theoretical analysis of a coupled, two-state Bose-Einstein condensate with non-equal scattering lengths, and show that dynamical instabilities can be excited. We demonstrate that these instabilities are exponentially amplified…

量子物理 · 物理学 2013-05-29 Graham R. Dennis , Mattias T. Johnsson

The study of extended $\gamma$-ray sources usually assumes symmetric diffusion of cosmic rays. However, recent observations of multiple sources near single pulsars and significant offsets between TeV halo centroids and their parent pulsars…

高能天体物理现象 · 物理学 2025-09-09 Yiwei Bao , Gwenael Giacinti , Ruo-Yu Liu , Hai-Ming Zhang , Yang Chen

A novel two-stage helium buffer gas cooled beam source is introduced. The properties of the molecular beams produced from this source are investigated theoretically using the CaF as a test molecule. The gas-phase molecules are first…

原子物理 · 物理学 2020-04-14 Vijay Singh

We consider a quantum theory of elastic light scattering from macroscopic atomic sample existing in the Bose-Einstein condensate (BEC) phase. Following to the second quantized formalism we introduce a set of coupled and closed diagram…

量子物理 · 物理学 2017-01-17 Victoria Ezhova , Leonid Gerasimov , Dmitriy Kupriyanov

We consider the nonlinear scattering and transmission of an atom laser, or Bose-Einstein condensate (BEC) on a finite rectangular potential barrier. The nonlinearity inherent in this problem leads to several new physical features beyond the…

量子气体 · 物理学 2015-05-05 Lincoln D. Carr , Rachel R. Miller , Daniel R. Bolton , Scott A. Strong

We observed the bright unidentified TeV gamma-ray source HESS J1616-508 with the X-ray Imaging Spectrometers onboard the Suzaku satellite. No X-ray counterpart was found to a limiting flux of 3.1e-13 erg/s/cm^2 in the 2--10 keV band, which…