1 |
Giordano F, Naumann MG, Ballet J, Bechtol K , Funk S, et al., Fermi Large Area Telescope Detection of the Young Supernova Remnant Tycho, ApJ, 744, L2-L6 (2012). http://dx.doi.org/10.1088/2041-8205/744/1/L2
DOI
|
2 |
Guo F, Jokipii JR, Kota J, Particle Acceleration by Collisionless Shocks Containing Large-scale Magneticfield Variations, ApJ, 725, 128-133 (2010). http://dx.doi.org/10.1088/0004-637X/725/1/128
DOI
|
3 |
Hillas AM, TOPICAL REVIEW: Can diffusive shock acceleration in supernova remnants account for highenergy galactic cosmic rays?, J. Phys. G: Nucl. Part. Phys., 31, R95 (2005). http://dx.doi.org/10.1088/0954-3899/31/5/R02
DOI
ScienceOn
|
4 |
Jones TW, Alfven wave transport effects in the time evolution of parallel cosmic-ray-modified shocks, ApJ, 413, 619-632, (1993). http://dx.doi.org/10.1086/173031
DOI
|
5 |
Kang H, Cosmic Ray Spectrum in Supernova Remnant Shocks, JKAS, 43, 25-39 (2010).
과학기술학회마을
DOI
ScienceOn
|
6 |
Kang H, Diffusive Shock Acceleration with Magnetic Field Amplification and Alfvenic Drift, JKAS, 45, 127-138 (2012).
|
7 |
Kang H, Edmon PP, Jones JW, Nonthermal Radiation from Cosmic-Ray Modified Shocks, ApJ, 745, 146-159 (2012). http://dx.doi.org/10.1088/0004-637X/745/2/146
DOI
|
8 |
Acciari VA, Aliu E, Arlen T, Aune T, Beilicke M, et al., Discovery of TeV Gamma-ray Emission from Tycho's Supernova Remnant, ApJ, 730, L20-L25 (2011). http://dx.doi.org/10.1088/2041-8205/730/2/L20
DOI
|
9 |
Ave M, Boyle PJ, Hoeppner C, Marshall J, Mueller D, Propagation and source energy spectra of cosmic ray nuclei at high energies, ApJ, 697, 106-114 (2009). http://dx.doi.org/10.1088/0004-637X/697/1/106
DOI
|
10 |
Bamba A, Yamazaki R, Ueno M, Koyama K, Small-Scale Structure of the SN 1006 Shock with Chandra Observations, ApJ, 589, 827-837 (2003). http://dx.doi.org/10.1086/374687
DOI
ScienceOn
|
11 |
Bell AR, The Acceleration of Cosmic Rays in Shock Fronts. I, MNRAS, 182, 147-156 (1978).
DOI
|
12 |
Bell AR, Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays, MNRAS, 353, 550-558 (2004). http://dx.doi.org/10.1111/j.1365-2966.2004.08097.x
DOI
ScienceOn
|
13 |
Berezhko EG, Ksenofontov LT, Voelk, HJ., Cosmic ray acceleration parameters from multi-wavelength obser vat ions. The case of SN 1006, A&A, 505, 169-176 (2009). http://dx.doi.org/10.1051/0004-6361/200911948
DOI
ScienceOn
|
14 |
Blandford RD, Eichler D, Particle Acceleration at Astrophysical Shocks - a Theory of Cosmic-Ray Origin, Phys. Rept., 154, 1 (1987). http://dx.doi.org/10.1016/0370-1573(87)90134-7
DOI
ScienceOn
|
15 |
Bykov AM, Osipov SM, Ellison DC, Cosmic ray current driven turbulence in shocks with efficient particle acceleration: the oblique, long-wavelength mode instability, MNRAS, 410, 39-52 (2011). http://dx.doi.org/10.1111/j.1365-2966.2010.17421.x
DOI
ScienceOn
|
16 |
Caprioli D, Understanding hadronic gamma-ray emission from supernova remnants, JCAP, 5, 26 (2011). http://dx.doi.org/10.1088/1475-7516/2011/05/026
DOI
ScienceOn
|
17 |
Caprioli D, Cosmic-ray acceleration in supernova remnants: non-linear theory revised, JCAP, 7, 38 (2012). http://dx.doi.org/10.1088/1475-7516/2012/07/038
DOI
ScienceOn
|
18 |
Reynolds SP, Supernova Remnants at High Energy, ARAA, 46, 89-126 (2008). http://dx.doi.org/10.1146/annurev.astro.46.060407.145237
DOI
ScienceOn
|
19 |
Abdo AA, Ackermann M, Ajello M, Allafort A, Baldini L, et al., Fermi-Lat Discovery of GeV Gamma-Ray Emission from the Young Supernova Remnant Cassiopeia A, ApJ, 710, L92-L97 (2010). http://dx.doi.org/10.1088/2041-8205/710/1/L92
DOI
|
20 |
Riquelme MA, Spitkovsky A, Magnetic Amplification by Magnetized Cosmic Rays in Supernova Remnant Shocks, ApJ, 717, 1054-1066 (2010). http://dx.doi.org/10.1088/0004-637X/717/2/1054
DOI
|
21 |
Reynolds SP, Gaensler BM, Bocchino F, Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae, Space Science Reviews, 166, 231-261 (2012). http://dx.doi.org/10.1007/s11214-011-9775-y
DOI
|
22 |
Zirakashvili VN, Ptuskin VS, Diffusive Shock Acceleration with Magnetic Amplification by Nonresonant Streaming Instability in Supernova Remnants, ApJ, 678, 939-949 (2008). http://dx.doi.org/10.1086/529580
DOI
|
23 |
Rogachevskii I, Kleeorin N, Brandenburg A, Eichler D, Cosmic-Ray current-driven turbulence and mean-field dynamo effect, ApJ, 753, 6-22 (2012). http://dx.doi.org/10.1088/0004-637X/753/1/6
DOI
|
24 |
Schure KM, Bell AR, Drury LO'C, Bykov AM, Diffusive Shock Acceleration and Magnetic Field Amplification, Space Sci. Rev., 173, 491-519 (2012). http://dx.doi.org/10.1007/s11214-012-9871-7
DOI
|
25 |
Skilling J, Cosmic Ray Streaming. I - Effect of Alfven Waves on Particles, MNRAS, 172, 557-566 (1975).
DOI
|
26 |
Zirakashvili VN, Ptuskin VS, Numerical simulations of diffusive shock acceleration in SNRs, Astropart. Phys., 39, 12-21 (2012). http://dx.doi.org/10.1016/j.astropartphys.2011.09.003
DOI
ScienceOn
|
27 |
Kang H, Jones TW, Numerical studies of diffusive shock acceleration at spherical shocks, Astropart. Phys, 25, 246-258 (2006). http://dx.doi.org/10.1016/j.astropartphys.2006.02.006
DOI
ScienceOn
|
28 |
Kang H, Jones TW, Gieseler UDJ, Numerical Studies of Cosmic-Ray Injection and Acceleration, ApJ, 579, 337-358 (2002). http://dx.doi.org/10.1086/342724
DOI
ScienceOn
|
29 |
Lee S, Ellison DC, Nagataki S, A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant, ApJ, 750, 156-168 (2012). http://dx.doi.org/10.1088/0004-637X/750/2/156
DOI
|
30 |
Lucek SG, Bell AR, Non-linear amplification of a magnetic field driven by cosmic ray streaming, MNRAS, 314, 65-74 (2000). http://dx.doi.org/10.1046/j.1365-8711.2000.03363.x
DOI
ScienceOn
|
31 |
Malkov MA, Drury LO'C, Nonlinear Theory of Diffusive Acceleration of Particles by Shock Waves, Rep. Progr. Phys., 64, 429-481 (2001). http://dx.doi.org/10.1088/0034-4885/64/4/201
DOI
ScienceOn
|
32 |
Morlino G, Caprioli D, Strong evidence for hadron acceleration in Tycho's supernova remnant, Tycho, theoretical fit, Alfven drift, A&A, 538, 81-94 (2012). http://dx.doi.org/10.1051/0004-6361/201117855
DOI
|
33 |
Parizot E, Marcowith A, Ballet J, Gallant YA, Observational Constraints on Energetic Particle Diffusion in Young Supernovae Remnants: Amplified Magnetic Field and Maximum Energy, A&A, 453, 387-395 (2006). http://dx.doi.org/10.1051/0004-6361:20064985
DOI
ScienceOn
|
34 |
Ptuskin VS, Zirakashvili VN, On the spectrum of high-energy cosmic rays produced by supernova remnants in the presence of strong cosmic-ray streaming instability and wave dissipation, A&A, 429, 755-765 (2005). http://dx.doi.org/10.1051/0004-6361:20041517
DOI
ScienceOn
|
35 |
Riquelme MA, Spitkovsky A, Nonlinear Study of Bell's Cosmic Ray Current-Driven Instability, ApJ, 694, 626-642 (2009). http://dx.doi.org/10.1088/0004-637X/694/1/626
DOI
|
36 |
Drury LO'C, An Introduction to the Theory of Diffusive Shock Acceleration of Energetic Particles in Tenuous Plasmas, Rep. Prog. Phys., 46, 973-1027 (1983). http://dx.doi.org/10.1088/0034-4885/46/8/002
DOI
ScienceOn
|
37 |
Edmon PP, Kang H, Jones TW, Ma R, Non-thermal radiation from Type Ia supernova remnants, MNRAS, 414, 3521-3536 (2011). http://dx.doi.org/10.1111/j.1365-2966.2011.18652.x
DOI
ScienceOn
|
38 |
Gargate L, Spitkovsky A, Ion Acceleration in Non-relativistic Astrophysical Shocks, ApJ, 744, 67-81 (2012). http://dx.doi.org/10.1088/0004-637X/744/1/67
DOI
|