Relevant bibliographies by topics / High energy astrophysics and galactic cosmic rays

Academic literature on the topic 'High energy astrophysics and galactic cosmic rays'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Contents

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'High energy astrophysics and galactic cosmic rays.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "High energy astrophysics and galactic cosmic rays"

1

BIERMANN, P. L., J. K. BECKER, L. CARAMETE, L. GERGELY, I. C. MARIŞ, A. MELI, V. DE SOUZA, and T. STANEV. "ACTIVE GALACTIC NUCLEI: SOURCES FOR ULTRA HIGH ENERGY COSMIC RAYS." International Journal of Modern Physics D 18, no. 10 (October 2009): 1577–81. http://dx.doi.org/10.1142/s0218271809015369.

Full text
Abstract:
Ultra high energy cosmic ray events presently show a spectrum, which we interpret here as galactic cosmic rays due to a starburst, in the radio galaxy Cen A which is pushed up in energy by the shock of a relativistic jet. The knee feature and the particles with energy immediately higher in galactic cosmic rays then turn into the bulk of ultra high energy cosmic rays. This entails that all ultra high energy cosmic rays are heavy nuclei. This picture is viable if the majority of the observed ultra high energy events come from the radio galaxy Cen A, and are scattered by intergalactic magnetic fields across much of the sky.
APA, Harvard, Vancouver, ISO, and other styles
2

Blandford, R. D. "The Phenomena of High Energy Astrophysics." Symposium - International Astronomical Union 214 (2003): 3–20. http://dx.doi.org/10.1017/s0074180900194124.

Full text
Abstract:
A brief summary of some highlights in the study of high energy astrophysical sources over the past decade is presented. It is argued that the great progress that has been made derives largely from the application of new technology to observation throughout all of the electromagnetic and other spectra and that, on this basis, the next decade should be even more exciting. However, it is imperative to observe cosmic sources throughout these spectra in order to obtain a full understanding of their properties. In addition, it is necessary to learn the universal laws that govern the macroscopic and the microscopic behavior of cosmic plasma over a great range of physical conditions by combining observations of different classes of source. These two injunctions are illustrated by discussions of cosmology, hot gas, supernova remnants and explosions, neutron stars, black holes and ultrarelativistic outflows. New interpreations of the acceleration of Galactic cosmic rays, the cooling of hot gas in rich clusters and the nature of ultrarelativistic outflows are outlined. The new frontiers of VHE γ-ray astronomy, low frequency radio astronomy, neutrino astronomy, UHE cosmic ray physics and gravitational wave astronomy are especially promising.
APA, Harvard, Vancouver, ISO, and other styles
3

BLASI, PASQUALE. "ON THE ORIGIN OF VERY HIGH ENERGY COSMIC RAYS." Modern Physics Letters A 20, no. 40 (December 28, 2005): 3055–76. http://dx.doi.org/10.1142/s0217732305019213.

Full text
Abstract:
We discuss the most recent developments in our understanding of the acceleration and propagation of cosmic rays up to the highest energies. In particular we specialize our discussion to three issues: (a) developments in the theory of particle acceleration at shock waves; (b) the transition from galactic to extragalactic cosmic rays; (c) implications of up-to-date observations for the origin of ultra high energy cosmic rays (UHECRs).
APA, Harvard, Vancouver, ISO, and other styles
4

Fukushima, Masaki. "The Highest Energy Cosmic Rays, A Review and Prospects." Symposium - International Astronomical Union 214 (2003): 399–408. http://dx.doi.org/10.1017/s007418090019480x.

Full text
Abstract:
The existence of extremely high energy cosmic rays (EHECRs) with energy above 1020eV have been reported by several air shower experiments. The sources of these cosmic rays were considered to be extra-galactic. Relevant high energy astrophysical sources were searched in the arrival direction of these cosmic rays but no appropriate candidates were found. The origin of EHECRs stays unexplained. We review the present status of EHECR studies and introduce several new experiments aiming to unveil its mysterious origin.
APA, Harvard, Vancouver, ISO, and other styles
5

Palladino, Andrea, Arjen van Vliet, Walter Winter, and Anna Franckowiak. "Can astrophysical neutrinos trace the origin of the detected ultra-high energy cosmic rays?" Monthly Notices of the Royal Astronomical Society 494, no. 3 (April 15, 2020): 4255–65. http://dx.doi.org/10.1093/mnras/staa1003.

Full text
Abstract:
ABSTRACT Since astrophysical neutrinos are produced in the interactions of cosmic rays, identifying the origin of cosmic rays using directional correlations with neutrinos is one of the most interesting possibilities of the field. For that purpose, especially the Ultra-High Energy Cosmic Rays (UHECRs) are promising, as they are deflected less by extragalactic and Galactic magnetic fields than cosmic rays at lower energies. However, photo-hadronic interactions of the UHECRs limit their horizon, while neutrinos do not interact over cosmological distances. We study the possibility to search for anisotropies by investigating neutrino-UHECR correlations from the theoretical perspective, taking into account the UHECR horizon, magnetic-field deflections, and the cosmological source evolution. Under the assumption that the neutrinos and UHECRs all come from the same source class, we demonstrate that the non-observation of neutrino multiplets strongly constrains the possibility to find neutrino-UHECR correlations.
APA, Harvard, Vancouver, ISO, and other styles
6

Armillotta, Lucia, Eve C. Ostriker, and Yan-Fei Jiang. "Cosmic-Ray Transport in Simulations of Star-forming Galactic Disks." Astrophysical Journal 922, no. 1 (November 1, 2021): 11. http://dx.doi.org/10.3847/1538-4357/ac1db2.

Full text
Abstract:
Abstract Cosmic-ray transport on galactic scales depends on the detailed properties of the magnetized, multiphase interstellar medium (ISM). In this work, we postprocess a high-resolution TIGRESS magnetohydrodynamic simulation modeling a local galactic disk patch with a two-moment fluid algorithm for cosmic-ray transport. We consider a variety of prescriptions for the cosmic rays, from a simple, purely diffusive formalism with constant scattering coefficient, to a physically motivated model in which the scattering coefficient is set by the critical balance between streaming-driven Alfvén wave excitation and damping mediated by local gas properties. We separately focus on cosmic rays with kinetic energies of ∼1 GeV (high-energy) and ∼30 MeV (low energy), respectively important for ISM dynamics and chemistry. We find that simultaneously accounting for advection, streaming, and diffusion of cosmic rays is crucial for properly modeling their transport. Advection dominates in the high-velocity, low-density hot phase, while diffusion and streaming are more important in higher-density, cooler phases. Our physically motivated model shows that there is no single diffusivity for cosmic-ray transport: the scattering coefficient varies by four or more orders of magnitude, maximal at density n H ∼ 0.01 cm−3. The ion-neutral damping of Alfvén waves results in strong diffusion and nearly uniform cosmic-ray pressure within most of the mass of the ISM. However, cosmic rays are trapped near the disk midplane by the higher scattering rate in the surrounding lower-density, higher-ionization gas. The transport of high-energy cosmic rays differs from that of low-energy cosmic rays, with less effective diffusion and greater energy losses for the latter.
APA, Harvard, Vancouver, ISO, and other styles
7

TOMOZAWA, YUKIO. "HIGH ENERGY COSMIC RAYS, GAMMA RAYS AND NEUTRINOS FROM AGN." Modern Physics Letters A 23, no. 24 (August 10, 2008): 1991–97. http://dx.doi.org/10.1142/s0217732308027278.

Full text
Abstract:
The author reviews a model for the emission of high energy cosmic rays, gamma-rays and neutrinos from AGN (Active Galactic Nuclei) that he has proposed since 1985. Further discussion of the knee energy phenomenon of the cosmic ray energy spectrum requires the existence of a heavy particle with mass in the knee energy range. A possible method of detecting such a particle in the Pierre Auger Project is suggested. Also presented is a relation between the spectra of neutrinos and gamma-rays emitted from AGN. This relation can be tested by high energy neutrino detectors such as ICECUBE, the Mediterranean Sea Detector and possibly by the Pierre Auger Project.
APA, Harvard, Vancouver, ISO, and other styles
8

del Valle, Maria V. "Gamma-rays from reaccelerated cosmic rays in high-velocity clouds colliding with the Galactic disc." Monthly Notices of the Royal Astronomical Society 509, no. 3 (November 11, 2021): 4448–56. http://dx.doi.org/10.1093/mnras/stab3206.

Full text
Abstract:
ABSTRACT High-velocity clouds moving towards the disc will reach the Galactic plane and will inevitably collide with the disc. In these collisions, a system of two shocks is produced, one propagating through the disc and the other develops within the cloud. The shocks produced within the clouds in these interactions have velocities of hundreds of kilometres per second. When these shocks are radiative they may be inefficient in accelerating fresh particles; however, they can reaccelerate and compress Galactic cosmic rays from the background. In this work, we investigate the interactions of Galactic cosmic rays within a shocked high-velocity cloud, when the shock is induced by the collision with the disc. This study is focused in the case of radiative shocks. We aim to establish under which conditions these interactions lead to significant non-thermal emission, especially gamma-rays. We model the interaction of cosmic ray protons and electrons reaccelerated and further energized by compression in shocks within the clouds, under very general assumptions. We also consider secondary electron–positron pairs produced by the cosmic ray protons when colliding with the material of the cloud. We conclude that nearby clouds reaccelerating Galactic cosmic rays in local shocks can produce high-energy radiation that might be detectable with existing and future gamma-ray detectors. The emission produced by electrons and secondary pairs is important at radio wavelengths, and in some cases it may be relevant at hard X-rays. Concerning higher energies, the leptonic contribution to the spectral energy distribution is significant at soft gamma-rays.
APA, Harvard, Vancouver, ISO, and other styles
9

Gorchakov, E., I. Kharchenko, Anvar Shukurov, and Dmitry Sokoloff. "Ultra-high energy cosmic rays in the galactic corona." Astrophysics and Space Science 179, no. 1 (1991): 141–45. http://dx.doi.org/10.1007/bf00642358.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Learned, John G., and Karl Mannheim. "High-Energy Neutrino Astrophysics." Annual Review of Nuclear and Particle Science 50, no. 1 (December 2000): 679–749. http://dx.doi.org/10.1146/annurev.nucl.50.1.679.

Full text
Abstract:
▪ Abstract High-energy (>100 MeV) neutrino astrophysics enters an era of opportunity and discovery as the sensitivity of detectors approaches astrophysically relevant flux levels. We review the major challenges for this emerging field, among which the nature of dark matter, the origin of cosmic rays, and the physics of extreme objects such as active galactic nuclei, gamma-ray bursts, pulsars, and supernova remnants are of prime importance. Variable sources at cosmological distances allow the probing of neutrino propagation properties over baselines up to about 20 orders of magnitude larger than those probed by terrestrial long-baseline experiments. We review the possible astrophysical sources of high-energy neutrinos, which also act as an irreducible background to searches for phenomena at the electroweak and grand-unified-theory symmetry-breaking scales related to possible supersymmetric dark matter and topological defects. Neutrino astronomy also has the potential to discover previously unimagined high-energy sources invisible in other channels and provides the only means for direct observations of the early universe prior to the era of decoupling of photons and matter. We conclude with a discussion of experimental approaches and a short report on present projects and prospects. We look forward to the day when it will be possible to see the universe through a new window in the light of what may be its most numerous particle, the elusive neutrino.
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "High energy astrophysics and galactic cosmic rays"

1

Gabici, Stefano. "Gamma ray astronomy and the origin of galactic cosmic rays." Habilitation à diriger des recherches, Université Paris-Diderot - Paris VII, 2011. http://tel.archives-ouvertes.fr/tel-00719791.

Full text
Abstract:
Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popular model for the origin of galactic cosmic rays. Despite the general consensus received by the model, an unambiguous and conclusive proof of the supernova remnant hypothesis is still missing. In this context, the recent developments in gamma ray astronomy provide us with precious insights into the problem of the origin of galactic cosmic rays, since production of gamma rays is expected both during the acceleration of cosmic rays at supernova remnant shocks and during their subsequent propagation in the interstellar medium. In particular, the recent detection of a number of supernova remnants at TeV energies nicely fits with the model, but it still does not constitute a conclusive proof of it, mainly due to the difficulty of disentangling the hadronic and leptonic contributions to the observed gamma ray emission. The main goal of my research is to search for an unambiguous and conclusive observational test for proving (or disproving) the idea that supernova remnants are the sources of galactic cosmic rays with energies up to (at least) the cosmic ray knee. Our present comprehension of the mechanisms of particle acceleration at shocks and of the propagation of cosmic rays in turbulent magnetic fields encourages beliefs that such a conclusive test might come from future observations of supernova remnants and of the Galaxy in the almost unexplored domain of multi-TeV gamma rays.
APA, Harvard, Vancouver, ISO, and other styles
2

Szabo, Anthony Paul. "High energy emissions for astrophysical objects." Title page, contents and abstract only, 1992. http://web4.library.adelaide.edu.au/theses/09PH/09phs996.pdf.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Brandt, Theresa J. "On High Energy Cosmic Rays from the CREAM Instrument." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1259540765.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Sutherland, Michael. "A Method for Establishing Constraints on Galactic Magnetic Field Models Using Ultra High Energy Cosmic Rays and Results from the Data of the Pierre Auger Observatory." The Ohio State University, 2010. http://rave.ohiolink.edu/etdc/view?acc_num=osu1274798328.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Grégoire, Timothée. "Search for high energy neutrinos from the Galactic plane with the ANTARES neutrino telescope." Thesis, Sorbonne Paris Cité, 2018. http://www.theses.fr/2018USPCC129/document.

Full text
Abstract:
Deux analyses sont présentées dans cette thèse. Une première analyse exploite les données du télescope à neutrino ANTARES pour sonder la présence d'un flux de neutrino diffus galactique. Cette analyse se base sur un modèle récent de propagation des rayons cosmiques dans la galaxie, le modèle KRAγ. Ce modèle prédit un flux de neutrinos particulièrement élevé et proche de la sensibilité des télescopes à neutrinos actuels. Il existe deux versions de ce modèle correspondant à différentes coupures sur l'énergie des rayons cosmiques, à 5 et 50 PeV/nucléon. Une méthode de maximisation d'une fonction de vraisemblance est utilisée pour prendre en compte les caractéristiques du modèle, autant spatiales qu'en énergie. Cette analyse a également été combinée avec les données de l'expérience IceCube dans le but d'exploiter au mieux les données actuelles. Des limites ont été mises sur ce modèle rejetant la version avec une coupure à 50 PeV et limitant la version avec une coupure à 5 PeV à moins de 1,2 fois le flux prédit par le modèle. Une deuxième analyse de suivi du signal d'ondes gravitationnelles GW170817 par le télescope à neutrino ANTARES est également présentée. Le signal d'onde gravitationnelles GW170817 résulte de la coalescence d'une binaire d'étoiles à neutrons. Cette deuxième analyse a pour objectif de sonder la présence d'un flux de neutrinos provenant de cet événement en cherchant des neutrinos corrélés spatialement et temporellement. J'ai pris part à cette analyse en y ajoutant les événement de type cascade. Aucun événement n'a été détecté en corrélation, des limites ont été mises sur le flux de neutrino attendu
Two analyses are detailed in this thesis. A first analysis exploit the data of the ANTARES neutrino telescope to probe the presence of a Galactic diffuse neutrino flux. This analysis is based on a recent model of cosmic ray propagation in the Galaxy, the KRAγ model. This model predict a neutrino flux particularly high and close to the sensitivity of the current neutrino telescopes. Two versions of this model exist corresponding to different cuts in the cosmic ray energy, one at 5 PeV/nucleon and an other one at 50 PeV/nucleon. A method of maximization of a likelihood function is used in order to account for the model characteristics in energy and space. The analysis has also been combined with the data of the IceCube experiment in order to exploit all the available data. Limits have been put on this model rejecting the version of the model with the 50 PeV cut and limiting the version with the 5 PeV cut to less than 1.2 times the predicted flux.A second analysis of gravitational wave signal follow-up by the ANTARES neutrino telescope is also presented in this work. The GW170817 gravitational wave signal results from the coalescence of a binary neutron star system. This second analysis aims at probing the presence of a neutrino flux coming from this event looking for neutrino events correlated in space and time. I took part to this analysis by adding the shower-like event sample. No event has been detected in correlation, limits have been put on the expected neutrino flux
APA, Harvard, Vancouver, ISO, and other styles
6

Taylor, Andrew Martin. "The propagation of ultra high energy cosmic rays." Thesis, University of Oxford, 2007. http://ora.ox.ac.uk/objects/uuid:63572ebe-fb32-41b6-8b91-a7294db135a6.

Full text
Abstract:
This thesis presents theoretical work on the propagation of ultra high energy cosmic rays, from their source to Earth. The different energy loss processes, resulting from cosmic ray interactions with the radiation fields, are addressed. The subsequent uncertainties in the energy loss rates and the effect produced on the arriving cosmic ray spectrum are highlighted. The question of the composition of ultra high energy cosmic rays remains unresolved, with the range of possibilities leading to quite different results in both the secondary fluxes of particles produced through cosmic ray energy loss interactions en route, and the arriving cosmic ray spectra at Earth. A large range of nuclear species are considered in this work, spanning the range of physically motivated nuclear types ejected from the cosmic ray source. The treatment of cosmic ray propagation is usually handled through Monte Carlo simulations due to the stochastic nature of some of the particle physics processes relevant. In this work, an analytic treatment for cosmic ray nuclei propagation is developed. The development of this method providing a deeper understanding of the main components relevant to cosmic ray nuclei propagation, and through its application, a clear insight into the contributing particle physics aspects of the Monte Carlo simulation. A flux of secondary neutrinos, produced as a consequence of cosmic ray energy loss through pion production during propagation, is also expected to be observed at Earth. This spectrum, however, is dependent on several loosely constrained factors such as the radiation field in the infrared region and cosmic ray composition. The range of possible neutrino fluxes obtainable with such uncertainties are discussed in this work. High energy cosmic ray interactions with the radiation fields present within the source may also occur, leading to cosmic ray energy loss before the cosmic ray has even managed to escape. The secondary spectra produced are investigated through the consideration of three candidate sources. A relationship between the degree of photo-disintegration in the source region and the neutrino flux produced through p γ interactions is found.
APA, Harvard, Vancouver, ISO, and other styles
7

Chadwick, Mary Paula. "Very high energy cosmic gamma rays from radio and X-ray pulsars." Thesis, Durham University, 1987. http://etheses.dur.ac.uk/6720/.

Full text
Abstract:
This thesis is concerned with the detection of very high energy cosmic gamma-rays from isolated pulsars and X-ray binary sources using the atmospheric Cerenkov technique. A general introduction to gamma ray detection techniques is followed by adscription of the properties of atmospheric Cerenkov radiation and a discussion of the principles of the atmospheric Cerenkov technique. The Mark I and Mark II gamma-ray telescopes operated in Dugway, Utah by the University of Durham between 1981 and 1984 are briefly described. There follows a discussion of the results from observations at many different wavelengths of Cygnus X-3. This object was observed by the Durham group between 1981 and 1983 in Dugway Utah and also in Durham during autumn 1985. The detection in the Dugway data of the 4.8 hr X-ray period and the possible detection of a19.2 day intensity variation are considered. The discovery of a 12.59 ms pulsar in data taken on Cygnus X-3 in 1983 is described. Evidence is presented which suggests this periodicity is also present at a weaker level in earlier data and also in the data taken in Durham in 1985.Results from observations of PSR1937+21 , PSR1953+29and six radio pulsars , are presented. The design and construction of the Mark III telescope, now operating in Narrabri , N.S.W. , is described in detail. Preliminary results from observations with the Mark III telescope of three objects, LMC X-4, the Vela pulsar and CentaurusX-3, are presented, with particular reference to periodicities inherent in the sources. An observation of the supernova in the Large Magellanic Cloud is discussed. A brief discussion of the mechanisms by which V.H.E. gamma-rays may be produced in isolated pulsars and X-ray binary pulsars is given, followed by a description of the future prospects for the Mark III and Mark IV telescopes.
APA, Harvard, Vancouver, ISO, and other styles
8

Lee, Anthony A. "Application of Monte Carlo methods to some problems in high energy astrophysics /." Title page, contents and abstract only, 1993. http://web4.library.adelaide.edu.au/theses/09PH/09phl4768.pdf.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

MacRae, John Hamish Kenneth. "The detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique." Thesis, Durham University, 1985. http://etheses.dur.ac.uk/7854/.

Full text
Abstract:
This thesis is concerned with the detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique. A general introduction to gamma ray detection techniques is followed by a detailed discussion of the principles of the atmospheric Cerenkov technique and the history of its use prior to this work. The design and operation of the University of Durham facility in Dugway, Utah is described in depth. Monte Carlo computer simulations have been developed to assist in both the understanding of the equipment and the analysis of the results for the Durham facility. The variation of the response of the array with zenith angle and detector threshold has been investigated and the aperture function of a single telescope calculated. The latter has been found to be a complicated function of both zenith angle and detector threshold. Computer simulations have also been developed to aid in the design of a camera to record two-dimensional Cerenkov light images from small extensive air showers, and to provide a means of testing analysis routines; these are discussed. The camera is located at the F.L. Whipple Observatory in Arizona. The techniques employed in the analysis of data recorded by the Dugway facility are discussed, and a computer package developed to aid in the routine aspects of the analysis is described. Results of observations from two sources, Cygnus X-3 and PSR0531, are presented, with particular reference to periodicities inherent in the sources and to bursts of gamma ray emission. The discussion of the results includes a review of the various models which have been proposed for Cygnus X-3.
APA, Harvard, Vancouver, ISO, and other styles
10

Morris, Chad Michael. "Detection Techniques of Radio Emission from Ultra High Energy Cosmic Rays." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1254506832.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "High energy astrophysics and galactic cosmic rays"

1

Clay, Roger. Cosmic bullets: High energy particles in astrophysics. Reading, Mass: Addison-Wesley, 1998.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
2

1959-, Dawson Bruce, ed. Cosmic bullets: High energy particles in astrophysics. St Leonards, NSW, Australia: Allen & Unwin, 1997.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
3

Clay, Roger. Cosmic bullets: High energy particles in astrophysics. Reading, Mass: Addison-Wesley, 1997.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
4

High energy astrophysics. 2nd ed. Cambridge [England]: Cambridge University Press, 1994.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
5

Lemoine, Martin, and Günter Sigl, eds. Physics and Astrophysics of Ultra-High-Energy Cosmic Rays. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/3-540-45615-5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. Hauppauge, N.Y: Nova Science Publishers, 2009.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
7

Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. New York: Nova Science Publishers, 2010.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
8

Schröder, Frank G. Instruments and Methods for the Radio Detection of High Energy Cosmic Rays. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
9

European Cosmic Ray Symposium (15th 1996 Perpignan, France). Cosmic rays 97: Solar, heliospheric, astrophysical, and high energy aspects : proceedings of the 15th European Cosmic Ray Symposium : Perpignan, France, 26-30 August 1996. [Amsterdam]: North-Holland, 1998.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
10

European Cosmic Ray Symposium (13th 1992 Geneva, Switzerland). Cosmic rays 92: Astrophysical, high energy and heliospheric processes : proceedings of the 13th European Cosmic Ray Symposium, Geneva, Switzerland, 27-31 July 1992. Amsterdam: North-Holland, 1993.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Book chapters on the topic "High energy astrophysics and galactic cosmic rays"

1

Protheroe, R. J., and A. P. Szabo. "High Energy Cosmic Rays from Cores of Active Galactic Nuclei." In Particle Astrophysics and Cosmology, 43–51. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1707-4_5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Dorman, L. I. "Cosmic Ray Nonlinear Effects in Space Plasma, 1. General Characteristics and Dynamic Galactic Halo." In Currents in High-Energy Astrophysics, 183–91. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0253-7_15.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Link, J. T. "The Astrophysics of Ultra-Heavy Galactic Cosmic Rays (and How we Can Detect Them)." In Astrophysical Sources of High Energy Particles and Radiation, 311–15. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0560-9_26.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Niebur, Susan M. "Reacceleration of Galactic Cosmic Rays: Secondary Electron Capture Isotopes Measured by the Cosmic Ray Isotope Spectrometer." In Astrophysical Sources of High Energy Particles and Radiation, 305–9. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0560-9_25.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Dorman, Lev I. "Variables Gamma Ray Sources, 2: Interactions of Galactic Cosmic Rays with Solar and Stellar Winds." In Astrophysical Sources of High Energy Particles and Radiation, 231–43. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0560-9_20.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Lake, George, and R. E. Pudritz. "Ultra-High Energy Cosmic Ray Production by Current Disruption in Active Galactic Nuclei." In Unstable Current Systems and Plasma Instabilities in Astrophysics, 471–73. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-6520-1_50.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Horvath, Jorge Ernesto. "Cosmic Rays." In High-Energy Astrophysics, 237–55. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-92159-0_12.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Spurio, Maurizio. "Ultra High Energy Cosmic Rays." In Astronomy and Astrophysics Library, 203–41. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-08051-2_7.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Cesarsky, Catherine J. "Galactic Cosmic Rays: Propagation and Origin." In High Energy Phenomena Around Collapsed Stars, 331–58. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3823-6_18.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Wdowczyk, J. "Anisotropies of High Energy Cosmic Rays." In Cosmic Radiation in Contemporary Astrophysics, 149–59. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-5488-5_10.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "High energy astrophysics and galactic cosmic rays"

1

Gaisser, T. K. "Origin of high energy galactic cosmic rays." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39149.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Hörandel, J. R. "Galactic cosmic rays and the knee — Results from the KASCADE experiment." In ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP, 2005. http://dx.doi.org/10.1063/1.2141835.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Bartko, H. "OBSERVATION OF GALACTIC SOURCES OF VERY HIGH ENERGY γ-RAYS WITH THE MAGIC TELESCOPE." In Proceedings of the 15th Course of the International School of Cosmic Ray Astrophysics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812790156_0017.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Amenomori, M., X. J. Bi, D. Chen, S. W. Cui, Danzengluobu, L. K. Ding, X. H. Ding, et al. "Heliospheric signatures seen in the sidereal anisotropy of high-energy galactic cosmic ray intensity." In PICKUP IONS THROUGHOUT THE HELIOSPHERE AND BEYOND: Proceedings of the 9th Annual International Astrophysics Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3529985.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Ptuskin, Vladimir. "Origin of Galactic Cosmic Rays." In HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP, 2005. http://dx.doi.org/10.1063/1.1878393.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Engel, Ralph, Mariana Orellana, Matías M. Reynoso, Gabriela S. Vila, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "High-energy cosmic ray interactions." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141378.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Meszaros, Peter. "High-energy astrophysics, (neutrinos, cosmic rays, GRBs)." In XIII Nuclei in the Cosmos. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.204.0188.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Kalli, Sihem, Martin Lemoine, Kumiko Kotera, N. Mebarki, and J. Mimouni. "Ultra High Energy Cosmic Rays Anisotropies Signatures." In THE THIRD ALGERIAN WORKSHOP ON ASTRONOMY AND ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3518323.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Ferrand, Gilles, and Samar Safi-Harb. "A Catalogue of High-Energy Observations of Galactic Supernova Remnants." In Cosmic Rays and the InterStellar Medium. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.221.0004.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Matthiae, Giorgio, Da-Shin Lee, Wolung Lee, and She-Sheng Xue. "Results from the Auger Observatory on high-energy cosmic rays." In RELATIVISTIC ASTROPHYSICS: 5th Sino-Italian Workshop on Relativistic Astrophysics. AIP, 2008. http://dx.doi.org/10.1063/1.3012270.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Reports on the topic "High energy astrophysics and galactic cosmic rays"

1

Tajima, T., and Y. Takahashi. Laboratory laser acceleration and high energy astrophysics: {gamma}-ray bursts and cosmic rays. Office of Scientific and Technical Information (OSTI), August 1998. http://dx.doi.org/10.2172/674811.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'High energy astrophysics and galactic cosmic rays' for particular source types:
Journal articles Dissertations / Theses Books
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography