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Astrophysics at ultra-high energies [[electronic resource] ] : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel
| Astrophysics at ultra-high energies [[electronic resource] ] : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel |
| Pubbl/distr/stampa | Singapore ; ; Hackensack, NJ, : World Scientific, c2007 |
| Descrizione fisica | 1 online resource (239 p.) |
| Disciplina | 523.019722 |
| Altri autori (Persone) |
ShapiroMaurice M <1915-> (Maurice Mandel)
StanevTodor WefelJ. P |
| Collana | Science and culture series. Astrophysics |
| Soggetto topico |
Cosmic rays
Nuclear astrophysics Gamma rays |
| Soggetto genere / forma | Electronic books. |
| ISBN |
1-281-93828-9
9786611938284 981-279-015-2 |
| Formato | Materiale a stampa  |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
CONTENTS; Preface M. M. Shapiro, T. Stanev & J. P. Wefel; Powerful Astrophysical Sources; Gamma Ray Bursts: Discoveries with Swift A , Wells; 1. Introduction; 2. Observations with Swift; 3. Models, progenitors and jets; 4. Afterglows; 5 . Short-hard gamma-ray bursts; References; Gamma Ray Burst Phenomenology in the Swift Era P. Meza'ros; 1. Challenges posed by new Swift observations; 2. Prompt gamma-ray emission; 3. Models of early afterglows in the Swift Era; 3.1. Prompt optical emission; 3.2. Steep X-ray decay; 3.3. Shallow X-ray decay; 3.4. X-ray flares; 3.5. High redshift afterglows
3.6. GRB-SN3.7. Short bursts; 3.8. Long-short classification; References; Modeling of Multiwavelength Spectra and Variability of 3C 66A in 2003-2004 M. Joshi & M. Bottcher; 1. Introduction; 2. Model description and model parameters; 3. Results and discussion; 4. Summary; References; High Energy Signatures of Post-Adiabatic Supernova Remnants I. 0. Telezhinsky & B. I. Hnatyk; 1. Introduction; 2. Hydrodynamic model of the transition stage; 2.1. Origin and dynamics of the thing shell during transition phase; 2.2. Hot gas parameters inside the shell; 2.3. Cold shell gas parameters 3. High energy signatures of transition stage3.1. X-ray emission; 3.2. y-ray emission from SNRs; 4. Conclusion; Acknowledgments; References; The Nature of Dark Matter P. L. Biermann & F. Munyaneza; 1. Dark Matter: Introduction; 2. Proposal; 2.1. Our recent work; 3. The tests; 3.1. Primordial magnetic fields; 3.2. Galaxies; 3.3. Dwarf spheroidal galaxies; 3.4. Lyman alpha forest; 3.5. The X-ray test; 4. Outlook; 5. Acknowledgements; References; Cosmic Rays; Particle Acceleration and Propagation in the Galaxy V. S. Ptuskin; 1. Introduction.; 2. Diffusion; 3. Supernova remnants 4. Knee and aboveAcknowledgments; References; Cosmic Rays from the Knee to the Second Knee: 1014 TO 1018 eV J. R. Horandel; 1. Introduction; 2. Galactic cosmic rays and the knee; 2.1. Sources; 2.2. Propagation; 2.3. Structures in the energy spectrum; 3. Measurement techniques; 3.1. A Heitler model for air showers; 3.1.1. Electromagnetic cascades; 3.1.2. Hadronic showers; 3.1.3. Number of muons; 3.1.4. Number of electrons; 3.1.5. Depth of the shower maximum; 3.1.6. Energy and mass of the primary particle; 4. Experimental results; 5. Conclusion and Outlook; References Ultra High-energy Cosmic Rays: Origin and Propagation T. Stanev1. Introduction; 1.1. The highest energy cosmic ray event; 2. Origin of UHECR; 2.1. Possible astrophysical sources of UHECR; 2.2. Top-down scenarios; 2.3. Hybrid models; 3. Propagation of UHECR; 3.1. Energy loss processes; 3.2. Modification of the proton spectrum in propagation. Numerical derivation of the GZK effect; 4. Production of Secondary Particles in Propagation; References; GRB as Sources of Ultra-High Energy Particles P. M&za'ros; 1. Introduction; 2. Cosmic rays from GRB; 3. GeV and TeV y-ray emission from GRB 4. High energy neutrinos |
| Record Nr. | UNINA-9910458355703321 |
| Singapore ; ; Hackensack, NJ, : World Scientific, c2007 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Astrophysics at ultra-high energies [[electronic resource] ] : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel
| Astrophysics at ultra-high energies [[electronic resource] ] : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel |
| Pubbl/distr/stampa | Singapore ; ; Hackensack, NJ, : World Scientific, c2007 |
| Descrizione fisica | 1 online resource (239 p.) |
| Disciplina | 523.019722 |
| Altri autori (Persone) |
ShapiroMaurice M <1915-> (Maurice Mandel)
StanevTodor WefelJ. P |
| Collana | Science and culture series. Astrophysics |
| Soggetto topico |
Cosmic rays
Nuclear astrophysics Gamma rays |
| ISBN |
1-281-93828-9
9786611938284 981-279-015-2 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
CONTENTS; Preface M. M. Shapiro, T. Stanev & J. P. Wefel; Powerful Astrophysical Sources; Gamma Ray Bursts: Discoveries with Swift A , Wells; 1. Introduction; 2. Observations with Swift; 3. Models, progenitors and jets; 4. Afterglows; 5 . Short-hard gamma-ray bursts; References; Gamma Ray Burst Phenomenology in the Swift Era P. Meza'ros; 1. Challenges posed by new Swift observations; 2. Prompt gamma-ray emission; 3. Models of early afterglows in the Swift Era; 3.1. Prompt optical emission; 3.2. Steep X-ray decay; 3.3. Shallow X-ray decay; 3.4. X-ray flares; 3.5. High redshift afterglows
3.6. GRB-SN3.7. Short bursts; 3.8. Long-short classification; References; Modeling of Multiwavelength Spectra and Variability of 3C 66A in 2003-2004 M. Joshi & M. Bottcher; 1. Introduction; 2. Model description and model parameters; 3. Results and discussion; 4. Summary; References; High Energy Signatures of Post-Adiabatic Supernova Remnants I. 0. Telezhinsky & B. I. Hnatyk; 1. Introduction; 2. Hydrodynamic model of the transition stage; 2.1. Origin and dynamics of the thing shell during transition phase; 2.2. Hot gas parameters inside the shell; 2.3. Cold shell gas parameters 3. High energy signatures of transition stage3.1. X-ray emission; 3.2. y-ray emission from SNRs; 4. Conclusion; Acknowledgments; References; The Nature of Dark Matter P. L. Biermann & F. Munyaneza; 1. Dark Matter: Introduction; 2. Proposal; 2.1. Our recent work; 3. The tests; 3.1. Primordial magnetic fields; 3.2. Galaxies; 3.3. Dwarf spheroidal galaxies; 3.4. Lyman alpha forest; 3.5. The X-ray test; 4. Outlook; 5. Acknowledgements; References; Cosmic Rays; Particle Acceleration and Propagation in the Galaxy V. S. Ptuskin; 1. Introduction.; 2. Diffusion; 3. Supernova remnants 4. Knee and aboveAcknowledgments; References; Cosmic Rays from the Knee to the Second Knee: 1014 TO 1018 eV J. R. Horandel; 1. Introduction; 2. Galactic cosmic rays and the knee; 2.1. Sources; 2.2. Propagation; 2.3. Structures in the energy spectrum; 3. Measurement techniques; 3.1. A Heitler model for air showers; 3.1.1. Electromagnetic cascades; 3.1.2. Hadronic showers; 3.1.3. Number of muons; 3.1.4. Number of electrons; 3.1.5. Depth of the shower maximum; 3.1.6. Energy and mass of the primary particle; 4. Experimental results; 5. Conclusion and Outlook; References Ultra High-energy Cosmic Rays: Origin and Propagation T. Stanev1. Introduction; 1.1. The highest energy cosmic ray event; 2. Origin of UHECR; 2.1. Possible astrophysical sources of UHECR; 2.2. Top-down scenarios; 2.3. Hybrid models; 3. Propagation of UHECR; 3.1. Energy loss processes; 3.2. Modification of the proton spectrum in propagation. Numerical derivation of the GZK effect; 4. Production of Secondary Particles in Propagation; References; GRB as Sources of Ultra-High Energy Particles P. M&za'ros; 1. Introduction; 2. Cosmic rays from GRB; 3. GeV and TeV y-ray emission from GRB 4. High energy neutrinos |
| Record Nr. | UNINA-9910784787603321 |
| Singapore ; ; Hackensack, NJ, : World Scientific, c2007 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Astrophysics at ultra-high energies : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel
| Astrophysics at ultra-high energies : International School of Cosmic Ray Astrophysics, 15th course, Erice, Italy, 20-27 June 2006 / / edited by Maurice M. Shapiro, Todor Stanev, John P. Wefel |
| Edizione | [1st ed.] |
| Pubbl/distr/stampa | Singapore ; ; Hackensack, NJ, : World Scientific, c2007 |
| Descrizione fisica | 1 online resource (239 p.) |
| Disciplina | 523.019722 |
| Altri autori (Persone) |
ShapiroMaurice M <1915-> (Maurice Mandel)
StanevTodor WefelJ. P |
| Collana | Science and culture series. Astrophysics |
| Soggetto topico |
Cosmic rays
Nuclear astrophysics Gamma rays |
| ISBN |
1-281-93828-9
9786611938284 981-279-015-2 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
CONTENTS; Preface M. M. Shapiro, T. Stanev & J. P. Wefel; Powerful Astrophysical Sources; Gamma Ray Bursts: Discoveries with Swift A , Wells; 1. Introduction; 2. Observations with Swift; 3. Models, progenitors and jets; 4. Afterglows; 5 . Short-hard gamma-ray bursts; References; Gamma Ray Burst Phenomenology in the Swift Era P. Meza'ros; 1. Challenges posed by new Swift observations; 2. Prompt gamma-ray emission; 3. Models of early afterglows in the Swift Era; 3.1. Prompt optical emission; 3.2. Steep X-ray decay; 3.3. Shallow X-ray decay; 3.4. X-ray flares; 3.5. High redshift afterglows
3.6. GRB-SN3.7. Short bursts; 3.8. Long-short classification; References; Modeling of Multiwavelength Spectra and Variability of 3C 66A in 2003-2004 M. Joshi & M. Bottcher; 1. Introduction; 2. Model description and model parameters; 3. Results and discussion; 4. Summary; References; High Energy Signatures of Post-Adiabatic Supernova Remnants I. 0. Telezhinsky & B. I. Hnatyk; 1. Introduction; 2. Hydrodynamic model of the transition stage; 2.1. Origin and dynamics of the thing shell during transition phase; 2.2. Hot gas parameters inside the shell; 2.3. Cold shell gas parameters 3. High energy signatures of transition stage3.1. X-ray emission; 3.2. y-ray emission from SNRs; 4. Conclusion; Acknowledgments; References; The Nature of Dark Matter P. L. Biermann & F. Munyaneza; 1. Dark Matter: Introduction; 2. Proposal; 2.1. Our recent work; 3. The tests; 3.1. Primordial magnetic fields; 3.2. Galaxies; 3.3. Dwarf spheroidal galaxies; 3.4. Lyman alpha forest; 3.5. The X-ray test; 4. Outlook; 5. Acknowledgements; References; Cosmic Rays; Particle Acceleration and Propagation in the Galaxy V. S. Ptuskin; 1. Introduction.; 2. Diffusion; 3. Supernova remnants 4. Knee and aboveAcknowledgments; References; Cosmic Rays from the Knee to the Second Knee: 1014 TO 1018 eV J. R. Horandel; 1. Introduction; 2. Galactic cosmic rays and the knee; 2.1. Sources; 2.2. Propagation; 2.3. Structures in the energy spectrum; 3. Measurement techniques; 3.1. A Heitler model for air showers; 3.1.1. Electromagnetic cascades; 3.1.2. Hadronic showers; 3.1.3. Number of muons; 3.1.4. Number of electrons; 3.1.5. Depth of the shower maximum; 3.1.6. Energy and mass of the primary particle; 4. Experimental results; 5. Conclusion and Outlook; References Ultra High-energy Cosmic Rays: Origin and Propagation T. Stanev1. Introduction; 1.1. The highest energy cosmic ray event; 2. Origin of UHECR; 2.1. Possible astrophysical sources of UHECR; 2.2. Top-down scenarios; 2.3. Hybrid models; 3. Propagation of UHECR; 3.1. Energy loss processes; 3.2. Modification of the proton spectrum in propagation. Numerical derivation of the GZK effect; 4. Production of Secondary Particles in Propagation; References; GRB as Sources of Ultra-High Energy Particles P. M&za'ros; 1. Introduction; 2. Cosmic rays from GRB; 3. GeV and TeV y-ray emission from GRB 4. High energy neutrinos |
| Record Nr. | UNINA-9910808153903321 |
| Singapore ; ; Hackensack, NJ, : World Scientific, c2007 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||