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相关论文: Galactic cosmic rays & gamma rays: a synthesis

200 篇论文

We are constructing a model which aims to reproduce observational data of many kinds related to cosmic-ray origin and propagation: direct measurements of nuclei, antiprotons, electrons and positrons, gamma-rays, and synchrotron radiation.…

天体物理学 · 物理学 2007-05-23 A. W. Strong , I. V. Moskalenko

We have developed a model which aims to reproduce observational data of many kinds related to cosmic-ray (CR) origin and propagation: direct measurements of nuclei, antiprotons, electrons and positrons, gamma-rays, and synchrotron…

天体物理学 · 物理学 2009-10-31 I. V. Moskalenko , A. W. Strong

An extensive program for the calculation of galactic cosmic-ray propagation has been developed. Primary and secondary nucleons, primary and secondary electrons, and secondary positrons are included. The basic spatial propagation mechanisms…

天体物理学 · 物理学 2008-02-03 A. W. Strong , I. V. Moskalenko , V. Schoenfelder

An extensive program for the calculation of galactic cosmic-ray propagation has been developed. Primary and secondary nucleons, primary and secondary electrons, secondary positrons and antiprotons are included. Fragmentation and energy…

天体物理学 · 物理学 2007-05-23 A. W. Strong , I. V. Moskalenko

A new numerical model of particle propagation in the Galaxy has been developed, which allows the study of cosmic-ray and gamma-ray production and propagation in 2D or 3D, including a full reaction network. This is a further development of…

天体物理学 · 物理学 2009-11-06 A. W. Strong , I. V. Moskalenko

Galactic diffuse continuum gamma-ray emission is intricately related to cosmic-ray physics and radio astronomy. We describe recent results from an approach which endeavours to take advantage of this. Information from cosmic-ray composition…

天体物理学 · 物理学 2010-12-13 A. W. Strong , I. V. Moskalenko , O. Reimer

A new study of the diffuse Galactic gamma-ray continuum radiation is presented, using a cosmic-ray propagation model which includes nucleons, antiprotons, electrons, positrons, and synchrotron radiation. Our treatment of the inverse Compton…

天体物理学 · 物理学 2009-10-31 A. W. Strong , I. V. Moskalenko , O. Reimer

An extensive program for the calculation of galactic cosmic-ray propagation has been developed. This is a continuation of the work described in Strong & Youssefi (1995). The main motivation for developing this code is the prediction of…

天体物理学 · 物理学 2009-10-30 A. W. Strong , I. V. Moskalenko

It is well established that phenomenological two-zone diffusion models of the galactic halo can very well reproduce cosmic-ray nuclear data and the observed antiproton flux. Here, we consider lepton propagation in such models and compute…

星系天体物理 · 物理学 2015-05-28 Torsten Bringmann , Fiorenza Donato , Roberto A. Lineros

We survey the theory and experimental tests for the propagation of cosmic rays in the Galaxy up to energies of 10^15 eV. A guide to the previous reviews and essential literature is given, followed by an exposition of basic principles. The…

天体物理学 · 物理学 2010-04-06 Andrew W. Strong , Igor V. Moskalenko , Vladimir S. Ptuskin

This paper presents an introduction to the astrophysics of cosmic rays and diffuse gamma rays and discusses some of the puzzles that have emerged recently due to more precise data and improved propagation models: the excesses in Galactic…

天体物理学 · 物理学 2008-11-26 I. V. Moskalenko

Continuum gamma-ray emission produced by interactions of cosmic rays with interstellar matter and radiation fields is a probe of non-thermal particle populations in galaxies. After decades of continuous improvements in experimental…

高能天体物理现象 · 物理学 2021-05-12 Luigi Tibaldo , Daniele Gaggero , Pierrick Martin

Cosmic-ray interactions with interstellar gas and photons produce diffuse gamma-ray emission. In this talk we will review the current understanding of this diffuse emission and its relationship to the problem of the origin of cosmic rays.…

天体物理学 · 物理学 2009-11-07 S. W. Digel , S. D. Hunter , I. V. Moskalenko , J. F. Ormes , M. Pohl

Various studies have implied the existence of a gaseous halo around the Galaxy extending out to 100 kpc. Galactic cosmic rays (CRs) that propagate to the halo, either by diffusion or by convection with the possibly existing large-scale…

高能天体物理现象 · 物理学 2019-01-30 Ruo-Yu Liu , Huirong Yan , Xiang-Yu Wang , Shi Shao , Hui Li

The excess of continuum gamma-ray emission from the Galaxy above 1 GeV is an unsolved puzzle. It may indicate that the interstellar nucleon or electron spectra are harder than local direct measurements, as could be the case if a local…

天体物理学 · 物理学 2011-05-23 I. V. Moskalenko , A. W. Strong , O. Reimer

We model the transport of cosmic ray nuclei in the Galaxy by means of a new numerical code. Differently from previous numerical models we account for a generic spatial distribution of the diffusion coefficient. We found that in the case of…

天体物理学 · 物理学 2016-05-19 C. Evoli , D. Gaggero , D. Grasso , L. Maccione

The last decade has been dense with new developments in the search for the sources of Galactic cosmic rays. Some of these developments have confirmed the tight connection between cosmic rays and supernovae in our Galaxy, through the…

高能天体物理现象 · 物理学 2015-06-18 Pasquale Blasi

This work presents preliminary results for the time-dependent cosmic-ray propagation in the Galaxy by a fully 3-dimensional Monte Carlo simulation. The distribution of cosmic-rays (both protons and helium nuclei) in the Galaxy is studied on…

天体物理学 · 物理学 2007-06-05 C. -Y. Huang , M. Pohl

A very interesting puzzle about the origin of electron and positron cosmic rays is deduced from the latests experimental results. We model the propagation of such cosmic rays in terms of a successfully tested two--zone propagation model.…

星系天体物理 · 物理学 2014-11-20 Roberto Lineros

Various studies firmly establish the fact that gamma-ray observations can act as a unique probe to detect the possible cosmic ray (CR) sources, study the CR density distribution and explore the average properties of interstellar medium…

高能天体物理现象 · 物理学 2020-01-08 Sayan Biswas , Nayantara Gupta
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