A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies,”M. L. Allen, P. L. Biermann, A. Chieffi, R. Chini, D. Frekers, L. Gergely, B. Harms, I. Jaroschewski, P.S. Joshi, P.P. Kronberg, E. Kun, A. Meli, E. S. Seo, and T. Stanev, Front. Astron. Space Sci., Sec. High-Energy and Astroparticle Physics, 11, in press, 2024.doi: 10.3389/fspas.2024.1394741
Loaded layer-cake model for cosmic ray interaction around exploding super-giant stars making black holes, M. L. Allen, P. L. Biermann, A. Chieffi, D. Frekers, L. Gergely, B. Harms, I. Jaroschewski, P.S. Joshi, P.P. Kronberg, E. Kun, A. Meli, E. S. Seo, and T. Stanev, Astroparticle Phys. 161,102976, 2024.
A Numerical Study of Cosmic-Ray Nuclei and Isotope Propagation, Z.M. Dorris,* Y. Chen,* V. S. Ptuskin, and E. S. Seo, PoS(ICRC2023)070, 2023.
Studies of Cosmic-Ray Propagation Using GALPROP," Y. Chen, Z.M. Dorris,* V. S. Ptuskin, E. S. Seo, and H, Wu,* PoS(ICRC2023)069, 2023.
Preface "Astrophysics of Cosmic Rays,” Moskalenko and E. S. Seo, Advances in Space Research, 70(9), 2583-2584, 2022.
The origin of the most energetic galactic cosmic rays: Supernova explosions into massive star plasma winds, P. L. Biermann, P. Kronberg, M. Allen, A. Meli, and E. S. Seo, Galaxies, 7/2, 48, 2019.doi:10.3390/galaxies7020048
Preface "Origins of Cosmic Rays," I. Moskalenko and E. S. Seo, Advances in Space Research, 62/10, 2729-230, 2018.
The Nature and Origin of Ultra-High Energy Cosmic Ray Particles, Biermann PL, Caramete LI, Fraschetti F, Gergely LA,Harms BC, Kun E, Lundquist JP, Meli A, Nath BB, Seo E-S, Stanev T and Tjus JB, Frascati Phys Ser 64, 103–121 2017.
Interpreting the Voyager 1 Data on the Interstellar Spectrum of Low-Energy Cosmic Rays in a Model with the Galactic Wind, V. S. Ptuskin, V. Zirakashvili, and E. S. Seo, Bulletin of the Russian Academy of Sciences: Physics 79, 345-347, 2015
Cosmic Ray Transport and Anisotropies to High Energies, P. L. Biermann, J. K. Becker, E. S. Seo, and M. Mandelartz, Astra Proc. 2, 39-44, 2015., doi:10.5194/ap-2-39-2015
Interpretation of Voyager 1 data on low energy cosmic rays in galactic wind model, V. S. Ptuskin, V. Zirakashvili, and E. S. Seo, Journal of Physics: Conf. Ser. 632 (1), 012022, 2015
Cosmic ray transport and anisotropy, P. L. Biermann, J. K. Becker, E. S. Seo, and M. Mandelartz, Astrophys. J.,768, 124, 2013, doi:10.1088/0004-637X/768/2/124
Spectra of Cosmic Ray Protons and Helium Produced in SupernovaRemnants,V. S. Ptuskin, V. Zirakashvili, and E. S. Seo, Astrophys. J.,763, 47, 2013, DOI: 10.1088/0004-637X/763/1/47
The origin of cosmic rays: Explosions of massive stars with magnetic winds and their supernova mechanism, P. L. Biermann, J. K. Becker, J. Dreyer, A. Meli, E. S. Seo, T. Stanev, Astrophys. J., 725, 184-187, 2010, doi: 10.1088/0004-637X/725/1/184
Spectrum of Galactic Cosmic Rays Accelerated in Supernova remnants, V. S. Ptuskin, V. Zirakashvili, and E. S. Seo, Astrophys. J., 718, 1, 31-36, July 20, 2010, arXiv:1006.0034v1
The WMAP haze from the Galactic Center region due to massive star explosions and a reduced cosmic ray scale height, P. L. Biermann, J. K. Becker, G. Caceres, A. Meli, E. S. Seo, T. Stanev, Astrophys. J. Lett., 710, L53-L57, 2010, doi: 10.1088/2041-8205/710/1/L53
Cosmic Ray Positrons and Electrons Supernova Explosions of Massive Stars, P. L. Biermann et al., Phys. Rev. Lett., 103, 061101, 2009
Origin of Cosmic Rays, E. S. Seo, Proceedings of UKC 2002(US-Korea Conference on Science, Technology, and Entrepreneurship), Technology for A Safe World, 1316-1321, 2002
Measurements of Cesium Radioisotopes in Cesium Compounds, Y. D. Kim et al. J.Kor. Phys. Soc., 40 (3), 520, 2002
Cosmic Ray H and He Isotopes in the Outer Heliosphere in 1994, E. S. Seo and F. B. McDonald, Proc. 24th Int. Cosmic Ray Conf.(Rome), 2, 626-629, 1995.
Galactic Cosmic Rays Up to 10 TeV, J. F. Ormes et al., Proc. 1994 Snowmass Summer Study: Particle and Nuclear Astrophysics and Cosmology in the Next Millennium, Ed. E. W. Kolb and R. D. Peccei (Singapore: World Scientific) 312, 1995.
Absolute Spectrum and Charge Ratio of Cosmic Ray Muons in Energy Region From 0.2 GeV to 100 GeV at 600 m Above Sea Level, M. P. DePascale et al. J. Geophys. Res., 98, NO. A3, 3501-3507, 1993.
Ground Level Observation of Electrons, Positrons and Protons, G. Basini et al., Proc. 23rd Int. Cosmic Ray Conf.(Calgary), 3, 773-776, 1993.
Iterstellar Propagation of the Isotopes of H and He, E. S. Seo, F. B. McDonald, N. Lal, and W. R. Webber, Proc. 23rd Int. Cosmic Ray Conf.(Calgary), 1, 511-514, 1993.
Measurement of the Cosmic Ray H and He Isotopes at 23 AU, E. S. Seo, F. B. McDonald, N. Lal, and W. R. Webber, Proc. 23rd Int. Cosmic Ray Conf. (Calgary), 1, 507-510, 1993.
Measurement of the Cosmic Ray Proton and Helium Fluxes From 200 MeV/nucleon To 100 GeV/nucleon During the 1987 Solar Minimum, E. S. Seo et al. Nucl. Tracks Rad. Meas., 20, 431-444, 1992.
Performance of a Balloon-Borne Magnet Spectrometer for Cosmic Ray Studies, R. L. Golden et al. Nucl. Instrum. Methods A306, 366-377, 1991.
Measurement of Cosmic Ray Proton and Helium Spectra During the 1987 Solar Minimum, E. S. Seo, J. F. Ormes, R. E. Streitmatter, S. J. Stochaj, W. V. Jones, S. A. Stephens, T. Bowen, Astrophys. J., 378, 763-772, 1991.
Cosmic Ray Muon Spectrum and Charge Ratio Between 0.2 and 100 GeV at 600 meters above sea level, G. Basini et al, Proc. 22nd ICRC (Dublin) 4, 544-547, 1991.
Observation of Cosmic Ray Electrons and Positrons Using a Magnet Spectrometer with Imaging Calorimeter, G. Basini et al, Proc. 22nd ICRC (Dublin) 2, 137-140, 1991.
Cosmic Ray Proton and Helium Spectra During the 1987 Solar Minimum, E. S. Seo et al, Proc. 22nd ICRC (Dublin) 1, 627-630, 1991.
Study of 2H and 3He in the Outer Heliosphere, E. S. Seo et al, Proc. 22nd ICRC (Dublin) 1, 604-606, 1991.
Measurement of the Cosmic Ray Proton and Helium Fluxes Above 200 MeV/nucleon During the 1987 Solar Minimum, E. S. Seo et al, Proceedings of Workshop on Galactic Cosmic Radiation: Constraints on Space Exploration, ed. J. H. Adams Jr. (NRL publication 209-4154), 49-76, 1991.
Cosmic Ray Proton Spectra at Low Rigidities, E. S. Seo et al, Proc. 21st ICRC (Australia) 3, 7-10, 1990.
Experimental Limit on Low Energy Antiprotons in the Cosmic Radiation,, R. E. Streitmatter, et al, Proc. 21st ICRC (Australia) 3, 277-280, 1990.
Empirical Scaling Regularity Deduced from Angular Distribution of Shower Particles Produced in Collisions of 50-, 100-, and 200 GeV/c Hadrons with Various Nuclei, C. O. Kim and E. S. Seo, J. Korean Phys. Soc. (Seoul) 20, 292-302, 1987.
Empirical Scaling Regularity Deduced from Angular Distribution of Shower Particles Produced in Collisions of 50-, 100-, and 200- GeV/c Hadrons with Various Nuclei, C. O. Kim and E. S. Seo, Proceedings of the XXIII Int. Conf. on High Energy Physics (Berkeley), No. 2399, 1580, 1986.
Properties of Cosmic-Ray Sulfur and Determination of the Composition of Primary Cosmic-Ray Carbon, Neon, Magnesium, and Sulfur: Ten-Year Results from the Alpha Magnetic Spectrometer, M. Aguilar et al. AMS Collaboration, Phys. Rev. Lett. 130, 211002, 2023.
Temporal Structures in electron spectra and charge sign effects in galactic cosmic rays, M. Aguilar et al. AMS Collaboration, Phys. Rev. Lett. 130(6), 161001, 2023. (Highlighted as Editors’ Suggestion) Physics.Viewpoint.
