査読論文
[1] Kawanaka, N., Mineshige, S. & Iwasawa, K. 2005, Astrophysical Journal, 635, 167-172 “Iron Fluorescent Line Emissions from Black Hole Accretion Disks with Magnetic Reconnection-Heated Corona”
[2] Kawanaka, N. & Mineshige, S. 2007, Astrophysical Journal, 662, 1156-1166, “Neutrino Cooled Accretion Disk and Its Stability”
[3] Masada, Y., Kawanaka, N., Sano, T. & Shibata, K. 2007, Astrophysical Journal, 663, 437-444, “Dead Zone Formation and Nonsteady Hyperaccretion in Collapsar Disks: A Possible Origin of Short-Term Variability in the Prompt Emission of Gamma-Ray Bursts”
[4] Kawabata, R., Mineshige, S. & Kawanaka, N. 2008, Astrophysical Journal, 675, 596, “Coronal Neutrino Emission in Hypercritical Accretion Flows”
[5] Kawanaka, N., Kato, Y. & Mineshige, S. 2008, Publications of the Astronomical Society of Japan, 60, 399, “X-ray Emissions from Three-Dimensional Magnetohydrodynamic Coronal Accretion Flows”
[6] Kawanaka, N., Ioka, K. & Nojiri, M. M. 2010, Astrophysical Journal, 710, 958 “Is Cosmic-Ray Electron Excess from Pulsars Spiky or Smooth?: Continuous and Multiple Electron/Positron Injections”
[7] Kashiyama, K., Ioka, K. & Kawanaka, N. 2011, Physical Review D, 83, 023002, “White Dwarf Pulsars as Possible Cosmic Ray Electron-Positron Factories”
[8] Kawanaka, N., Ioka, K., Ohira, Y. & Kashiyama, K. 2011, Astrophysical Journal, 729, 93, “TeV Electron Spectrum for Probing Cosmic-ray Escape from a Supernova Remnant”
[9] Ioka, K., Ohira, Y., Kawanaka, N. & Mizuta, A. 2011, Progress of Theoretical Physics, 126, 555, “Gamma-Ray Burst without Baryonic and Magnetic Load?”
[10] Actis, M. et al. (and 671 more) 2011, Experimental Astronomy, 32, 193, “Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy”
[11] Kawanaka, N. & Kohri, K. 2012, Monthly Notices of the Royal Astronomical Society, 419, 713, “A possible origin of the rapid variability of gamma-ray bursts due to convective energy transfer in hyperaccretion discs”
[12] Ohira, Y., Kohri, K. & Kawanaka, N. 2012, Monthly Notices of the Royal Astronomical Society, 421, L102, “Positron annihilation as a cosmic ray probe”
[13] Kisaka, S. & Kawanaka, N. 2012, Monthly Notices of the Royal Astronomical Society, 421, 3543, “TeV cosmic-ray electrons from millisecond pulsars”
[14] Ohira, Y., Yamazaki, R., Kawanaka, N. & Ioka, K. 2012, Monthly Notices of the Royal Astronomical Society, 427, 91 “Escape of cosmic-ray electrons from supernova remnants”
[15] Acharya, B. S. et al. (and 976 more) 2013, Astroparticle Physics, 43, 3 “Introducing the CTA concept”
[16] Kawanaka, N., Piran, T. & Krolik, J. H., 2013, Astrophysical Journal, 766, 31 “Jet Luminosity from Neutrino-Dominated Accretion Flows in Gamma-Ray Bursts”
[17] Kawanaka, N., Mineshige, S. & Piran, T., 2013, Astrophysical Journal Letter, 777, L15 “The Discovery of a New Instability in a Hyperaccretion Flow and its Implication for Gamma-Ray Bursts”
[18] Liu, T., Gu, W.-M., Kawanaka, N. & Li, A. 2015, Astrophysical Journal, 805, 37 “Vertical Convection in Neutrino-dominated Accretion Flows”
[19] Kimura, M., Mineshige, S. & Kawanaka, N. 2015, Publications of the Astronomical Society of Japan, 67, 101 “How does a secular instability grow in a hyperaccretion flow?”
[20] Kawanaka, N. & Ioka, K. 2015, Physical Review D, 92, 085047 “Neutrino flavor ratios modified by cosmic-ray secondary acceleration”
[21] Ohira, Y., Kawanaka, N. & Ioka, K. 2016, Physical Review D, 93, 083001 “Cosmic-ray hardenings in light of AMS-02 data”
[22] Yamasaki, S., Totani, T. & Kawanaka, N. 2016, Monthly Notices of the Royal Astronomical Society, 460, 2875 “A blind search for prompt gamma-ray counterparts of fast radio bursts with Fermi-LAT data”
[23] Adriani, O. et al. (and 91 more) 2016, Astrophysical Journal Letters, 829, L20 “CALET Upper Limits on X-ray and Gamma-Ray Counterparts of GW151226”
[24] Asaoka, Y. et al. (and 93 more) 2017, Astroparticle Physics, 91, 1 “Energy calibration of CALET onboard the International Space Station”
[25] Adriani, O. et al. (and 91 more) 2017, Physical Review Letters, 119, 181101 “Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station”
[26] Kawanaka, N. & Yanagita, S. 2018, Physical Review Letters, 120, 041103 “Cosmic-Ray Lithium Production at the Nova Eruptions Followed by a Type Ia Supernova”
[27] Tsuna, D., Kawanaka, N. & Totani, T. 2018, Monthly Notices of the Royal Astronomical Society, 477, 791 “X-ray detectability of accreting isolated black holes in our Galaxy”
[28] Lee, S.-H., Maeda, K. & Kawanaka, N. 2018, Astrophysical Journal, 858, 53 “Shock acceleration of electrons and synchrotron emission from the dynamical ejecta of neutron star mergers”
[29] Mizumoto, M., Moriyama, K., Ebisawa, K., Mineshige, S., Kawanaka, N. & Tsujimoto, M. 2018, Publications of the Astronomical Society of Japan, 70, 42 “Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?”
[30] Sudoh, T., Totani, T. & Kawanaka, N. 2018, Publications of the Astronomical Society of Japan, 70, 49 “High-energy gamma-ray and neutrino production in star-forming galaxies across cosmic time: Difficulties in explaining the IceCube data”
[31] Adriani, O. et al. (and 91 more) 2018, Physical Review Letters, 120, 261102 “Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station”
[32] Asaoka, Y. et al. (and 90 more) 2018, Astroparticle Physics, 100, 29 “On-orbit operations and offline data processing of CALET onboard the ISS”
[33] Yamaguchi, M. S., Kawanaka, N., Bulik, T. & Piran, T. 2018, Astrophysical Journal, 861, 21 “Detecting Black Hole Binaries by Gaia”
[34] Adriani, O. et al. (and 91 more) 2018, Astrophysical Journal, 863, 160 “Search for GeV Gamma-Ray Counterparts of Gravitational Wave Events by CALET”
[35] Cannady, N. et al. (and 93 more) 2018, Astrophysical Journal Supplement Series, 238, 5 “Characteristics and Performance of the CALorimetric Electron Telescope (CALET) Calorimeter for Gamma-Ray Observations”
[36] Adriani et al. (and 90 more) 2019, Physical Review Letters, 122, 181102 “Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station”
[37] Kawanaka, N. & Masada, Y. 2019, Astrophysical Journal, 881, 138, “Neutrino-Dominated Accretion Flows with Magnetic Prandtl Number-Dependent MRI-driven Turbulence”
[38] Tsuna, D. & Kawanaka, N. 2019, Monthly Notices of the Royal Astronomical Society, 488, 2099, “Radio Emission from Accreting Isolated Black Holes in Our Galaxy”
[39] Zhu, S., Baryakhtar, M., Alessandra Papa, M., Tsuna, D., Kawanaka, N. & Eggenstein, H.-B. 2020, Physical Review D, 102, 063020 “Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes”
[40] Adriani, O. et al. (and 84 more) 2020, Physical Review Letters, 125, 251102 “Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/n to 2.2 TeV/n with the Calorimetric Electron Telescope on the International Space Station”
[41] Abdalla, H. et al. (and 498 more) 2021, Journal of Cosmology and Astroparticle Physics, 2, 048 “Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation”
[42] Kawanaka, N. & Mineshige, S., 2021, Publications of Astronomical Society of Japan, 73, 630 “What Determines Unique Spectra of Super-Eddington Accretors?: Origin of Optically Thick and Low Temperature Coronae in Super-Eddington Accretion Flows”
[43] Adriani, O. et al. (and 80 more) 2021, Physical Review Letters, 126, 241101, “Measurement of the Iron Spectrum in Cosmic Rays from 10 GeV/n to 2.0 TeV/n with the Calorimetric Electron Telescope on the International Space Station”
[44] Kimura, S. S., Sudoh, T., Kashiyama, K. & Kawanaka, N., 2021, Astrophysical Journal, 915, 31 “Magnetically Arrested Disks in Quiescent Black-Hole Binaries: Formation Scenario, Observational Signatures, and Potential PeVatrons”
[45] Kawanaka, N. & Lee, S.-H., 2021, Astrophysical Journal, 917, 61 “Origin of Spectral Hardening of Secondary Cosmic-Ray Nuclei”
[46] Asano, K., Asaoka, Y., Akaike, Y., Kawanaka, N., Kohri, K., Motz, H. M., & Terasawa, T., 2021, Astrophysical Journal, 926, 5 “Monte Carlo Study of Electron and Positron Cosmic-Ray Propagation with the CALET Spectrum”
[47] Shikauchi, M., Tanikawa, A. & Kawanaka, N., 2021, Astrophysical Journal, 928, 13 “Detectability of Black Hole Binaries with Gaia: Dependence on Binary Evolution Models”
[48] Adriani, O. et al. (and 81 more) 2022, Physical Review Letters, 128, 131103 “Direct Measurement of the Nickel Spectrum in Cosmic Rays in the Energy Range from 8.8 GeV/n to 240 GeV/n with CALET on the International Space Station”
[49] Adriani, O. et al. (and 80 more), 2022, Astrophysical Journal, 933, 85 “CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run”
[50] Adriani, O. et al. (and 80 more), 2022, Physical Review Letters, 129, 101102 “Observation of Spectral Structures in the Flux of Cosmic-Ray Protons from 50 GeV to 60 TeV with the Calorimetric Electron Telescope on the International Space Station”
[51] Adriani, O. et al. (and 80 more), 2022, Physical Review Letters, 129, 251103 “Cosmic-Ray Boron Flux Measured from 8.4 GeV /n to 3.8 TeV /n with the Calorimetric Electron Telescope on the International Space Station”
[52] Tanikawa, A., Hattori, K., Kawanaka, N., Kinugawa, T., Shikauchi, M. & Tsuna, D. 2023, Astrophysical Journal, 949, 79 “Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic data”
[53] Adriani, O. et al. (and 80 more), 2023, Physical Review Letters, 130, 171002 “Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station”
[54] Adriani, O. et al. (and 80 more), 2023, Physical Review Letters, 130, 211001 “Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space Station”
[55] Shikauchi, M., Tsuna, D., Tanikawa, A. & Kawanaka, N., 2023, Astrophysical Journal, 953, 52 “Spatial and Binary Parameter Distributions of Black Hole Binaries in the Milky Way Detectable by Gaia”
[56] Kawanaka, N. & Kohri, K., 2023, Astrophysical Journal, 955, 67 “Effects of Heat Conduction on Blocking off the Super-Eddington Growth of Black Holes at High Redshift”
[57] Adriani, O. et al. (and 80 more), 2023, Physical Review Letters, 131, 191001 “Direct Measurement of the Spectral Structure of Cosmic-Ray Electrons+Positrons in the TeV Region with CALET on the International Space Station”
[58] Kawanaka, N. & Mineshige, S., 2024, Publications of the Astronomical Society of Japan, 76, 306 “Model of a `Warm Corona’ as the Origin of the Soft X-ray Excess of Active Galactic Nuclei”
[59] Fujita, Y., Izumi, T., Nagai, H., Kawakatu, N. & Kawanaka, N., 2024, Astrophysical Journal, 964, 29 “The Relationships between Active Galactic Nucleus Power and Molecular Gas Mass within 500 pc of the Center of Elliptical Galaxies”
[60] Takahashi, R., Umemura, M., Ohsuga, K., Asahina, Y., Takeda, R., Takahashi, M. M., Kawanaka, N., Konno, K. & Nagasawa, T., 2024, Astrophysical Journal Letters, 967, L10 “A Relativistic Formula for the Multiple Scattering of Photons”
[61] Kawata, D. et al. (and 88 more), 2024, Publications of the Astronomical Society of Japan, 76, 386 “JASMINE: Near-Infrared Astrometry and Time Series Photometry Science”
[62] Fujita, Y., Kawanaka, N. & Inoue, S., 2024, Publications of the Astronomical Society of Japan, 76, 765 “Broadband non-thermal emission of odd radio circles induced by galactic outflow remnants and their evolution”
[63] Koshimoto, N., Kawanaka, N. & Tsuna, D., 2024, Astrophysical Journal, 973, 5 “Influence of Black Hole Kick Velocity on Microlensing Distributions”
[64] Fujita, Y., Kawachi, A., Okazaki, A. T., Nagai, H., Kawanaka, N. & Akahori, T., 2024, Astrophysical Journal Letters, 977, L22 "ALMA Observations of the Gamma-ray Binary System PSR B1259-63/LS 2883 during the 2024 Periastron Passage"
[65] Kawanaka, N. & Takahashi, R., 2025, Physical Review D, 111, 123016 "Beyond diffusion: A causality-preserving model for cosmic-ray propagation"
[66] Adriani, O. et al. (and 80 more), 2025, Physical Review Letters, 135, 021102 "Precision Spectral Measurements of Chromium and Titanium from 10 to 250 GeV/n and Sub-Iron to Iron Ratio with the Calorimetric Electron Telescope on the International Space Station"
[67] Adriani, O. et al. (and 80 more), 2025, Astrophysical Journal, 988, 148 "Detected Abundances of Nuclei Relative to 26Fe for Elements 14Si through 44Ru with CALET on the International Space Station"
[68] Kawanaka, N., Nagai, H. & Fujita, Y. 2025, Astrophysical Journal, 990, 66 "Reexamination of the CO absorption line in the M87 nucleus"
国際会議集録（最近10年以内に限定）
[1] Kawanaka, N., Yamaguchi, M., Piran, T. and Bulik, T. 2017, New Frontiers in Black Hole Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, 324, 41-42 “Prospects for the Discovery of Black Hole Binaries without Mass Accretion with Gaia”
[2] Kawanaka, N. and Yanagita, S. 2017, Supernova 1987A:30 years later – Cosmic Rays and Nuclei from Supernovae and their aftermaths, Proceedings of the International Astronomical Union, IAU Symposium, 331, 254-257 “Cosmic-Ray Lithium Production in the Nova Ejecta”
[3] Ebisawa, K., Mineshige, S., Tsujimoto, M., Mizumoto, M., Moriyama, K. and Kawanaka, N. 2018, 42nd COSPAR Scientific Assembly. Held 14-22 July 2018, in Pasadena, California, USA, Abstract id. E1.4-61-18 “Can the relativistic light bending model explain X-ray spectral variations of Seyfert galaxies?”
[4] Asaoka, Y., Adriani, O. et al. 2019, International Symposium on Very High Energy Cosmic Ray Interactions (ISCHECRI 2018); EPK Web of Conferences 208, id.13001 “The CALorimetric Electron Telescope (CALET) on the International Space Station: Results from the First Two Years of Operation”
[5] Asaoka, Y., Adriani, O. et al. 2020, Journal of Physics: Conference Series, 1468, id.012074 “CALET results after three years on the International Space Station”
[6] Kawanaka, N. and Masada, Y. 2020, Yamada Conference LXXI: Gamma-ray Bursts in the Gravitational Wave Era 2019, 81-83 “Instability in Neutrino-Dominated Accretion Flows and Its Application to Gamma-Ray Bursts”
[7] Brogi, P., Adriani, O. et al. 2020, Physics Scripta 95, id.074012 “CALET on the International Space Station: the first three years of observations”
[8] Yonetoku, D., Mihara, T., Doi, A., Sakamoto, T., Tsumura, K., Ioka, K., Amaya, Y. et al. 2020, Proceedings of the SPIE, 11444, id.114442Z “High-redshift gamma-ray burst for unrabeling the Dark Ages Mission: HiZ-GUNDAM”
[9] Motz, H., Adriani, O. et al. 2022, 37th International Cosmic Ray Conference id.100 “Investigating the Vela SNR’s Emission of Electron Cosmic Rays with CALET at the International Space Station”
[10] Asano, K., Asaoka, Y., Akaike, Y., Kawanaka, N., Kohri, K., Motz, H. and Terasawa, T. 2022, 44th COSPAR Scientific Assembly, Abstract E1.3-0024-22 “Interpretation of Electron and Positron Cosmic-Ray Spectrum Measured with CALET”
[11] Kawanaka, N. and Lee, S.-H. 2022, Acta Physica Polonica B Proceedings Supplement 15, 3-A4 “Origin of Spectral Hardening of Secondary Cosmic Ray Nuclei”
[12] Kawanaka, N. 2023, Proceedings of Science, International Cosmic Ray Conference 2023, 162 “Origin of Spectral Hardening and Softening of Secondary Cosmic-Ray Nuclei”
国際会議発表（最近10年以内に限定）
[1] N. Kawanaka, “Structure and Evolution of a Hyperaccretion Flow as a Central Engine of Gamma-ray Bursts”, HEAP2015 “Central Engines in the High Energy Universe”, 高エネルギー加速器研究機構, 口頭発表（招待講演）, 2015年10月
[2] N. Kawanaka, “Theoretical Models of X-ray Emission from Black Hole Accretion Flows”, Workshop on “Prospects, Challenges and Evolution of AGN Modeling in the ASTRO-H Era”, 立教大学, 口頭発表（招待講演）, 2015年10月
[3] N. Kawanaka & K. Ioka “Neutrino Flavor Ratios Modified by Cosmic Ray Secondary-acceleration”, TeV Particle Astrophysics 2015, 千葉県柏市, 口頭発表，2015年10月
[4] N. Kawanaka, “Astrophysical Electron-Positron Factories and their Spectral Features”, MACROS 2016, 口頭発表（招待講演）, Pennsylvania State University, 2016年6月
[5] N. Kawanaka, M. S. Yamaguchi, T. Bulik & T. Piran, “Prospects for the Discovery of Black Hole Binaries without Mass Accretion with Gaia”, IAU Symposium 324 “New Frontiers in Black Hole Astrophysics”, Ljubljana, Slovenija, ポスター発表, 2016年9月
[6] N. Kawanaka & S. Yanagita, “Cosmic-Ray Lithium Production in the Nova Ejecta”, IAU Symposium 331 “SN1987A, 30 years later”, Reunion, France, ポスター発表, 2017年2月
[7] N. Kawanaka & S. Yanagita, “Cosmic-Ray Lithium Production at a Type Ia Supernova Following a Nova Eruption”, TeV Particle Astrophysics 2017, Berlin, Germany, 口頭発表, 2017年8月
[8] N. Kawanaka & S. Yanagita, “Cosmic-Ray Lithium Production in the Nova Ejecta”, JSI workshop “Cosmic Accelerators: Understanding Nature’s High Energy Particles and Radiations”, Annapolis, MD, USA, ポスター発表, 2017年11月
[9] N. Kawanaka, “Neutrino-Dominated Accretion Flows as the Central Engine of Gamma-Ray Bursts”, YITP workshop, “Jet and Shock Breakouts in Cosmic Transients”, 京都大学基礎物理学研究所, 口頭発表（招待講演）2018年5月
[10] N. Kawanaka & S. Mineshige “Origin of Optically Thick and Low Temperature Coronae in Supercritical Accretion Flows”, Breaking the Limits 2018, Castiadas, Italy, 口頭発表, 2018年10月
[11] N. Kawanaka & Y. Masada “Instability in Neutrino-Dominated Accretion Flows and Its Application to Gamma-Ray Bursts”, High Energy Astrophysics Japan-Israel Workshop, 理化学研究所, 口頭発表（招待講演）2019年7月
[12] N. Kawanaka, Y. Masada “Instability in Neutrino-Dominated Accretion Flows and Its Application to Gamma-Ray Bursts”, Multi-Messenger Astrophysics in the Gravitational Wave Era, 京都大学基礎物理学研究所, 口頭発表, 2019年10月
[13] N. Kawanaka, Y. Masada “Instability in Neutrino-Dominated Accretion Flows and Its Application to Gamma-Ray Bursts”, Yamada Conference LXXI: Gamma-Ray Bursts in the Gravitational Wave Era, Yokohama, 口頭発表, 2019年10月
[14] N. Kawanaka, S.-H. Lee “Origin of Spectral Hardening of Secondary Cosmic Ray Nuclei”, Connecting high-energy astroparticle physics for origins of cosmic rays and future perspectives, 京都大学基礎物理学研究所, 口頭発表, 2020年12月
[15] N. Kawanaka, S. Mineshige “Origin of optically thick and low temperature coronae in super-Eddington accretion flows”, Black Hole Astrophysics with VLBI: Multi-Wavelength and Multi-Messenger Era, オンライン, 口頭発表, 2021年1月
[16] N. Kawanaka, S.-H. Lee “Origin of Spectral Hardening of Secondary Cosmic-Ray Nuclei”, XXVIII Cracow Epiphany Conference on Recent Advances in Astroparticle Physics, オンライン, 口頭発表, 2022年1月
[17] N. Kawanaka “Origin of Spectral Hardening and Softening of Secondary Cosmic Ray Nuclei”, 38th International Cosmic Ray Conference, Nagoya University, 口頭発表, 2023年7月
国内会議口頭発表（最近10年以内に限定）
[1] “質量降着を伴わない星質量ブラックホール連星のいち天文衛星による検出数予測と理論モデルへの示唆”, 2015年日本天文学会秋季年会, 甲南大学, 2015年9月
[2] “2次粒子の衝撃波加速による高エネルギーニュートリノのフレーバー比の変更”, 2016年日本天文学会春季年会, 首都大学東京, 2016年3月
[3] “電子陽電子対消滅放射から探る銀河系内宇宙線源”, MeVガンマ線天文学研究会, 京都大学, 招待講演, 2017年2月
[4] “銀河宇宙線Liの過剰と新星爆発放出物質”, 2017年日本天文学会春季年会, 九州大学, 2017年3月
[5] “銀河宇宙線Liの過剰と新星爆発放出物質”, 2017年日本物理学会春季大会, 大阪大学, 2017年3月
[6] “超臨界降着流における円盤コロナモデル”, 2017年日本天文学会秋季年会, 北海道大学, 2017年9月
[7] “銀河系内ブラックホール探査”, 研究会X, 広島大学, 招待講演, 2018年3月
[8] “ブラックホール超臨界降着流に付随するコロナからのX線放射スペクトル”, 2018年日本天文学会春季年会, 2018年3月
[9] “最新の宇宙線スペクトルとその宇宙物理学的解釈”, 第8回日大理工・益川塾連携シンポジウム, 京都産業大学むすびわざ館, 招待講演, 2018年11月
[10] “ニュートリノ優勢降着円盤における質量降着の不安定性とガンマ線バーストへの応用”, 2019年日本天文学会秋季年会, 熊本大学, 2019年9月
[11] “銀河系内ブラックホール探査”, 天の川銀河研究会2020, 鹿児島大学, 招待講演, 2020年2月
[12] “超新星残骸中で生成された二次宇宙線原子核の逃走とそのエネルギースペクトル”, 2020年日本天文学会春季年会, 筑波大学, 2020年3月
[13] “超臨界降着流におけるコロナモデルとスペクトルの特徴”, 2020年日本天文学会秋季年会, オンライン, 2020年9月
[14] “宇宙線軽元素のハードニングの起源”, 2021年日本天文学会春季年会, オンライン, 2021年3月
[15] “活動銀河核の軟Ｘ線超過の起源としての温かいコロナモデル”, 2022年日本天文学会秋季年会, 新潟大学 (オンライン参加), 2022年9月
[16] “銀河系内宇宙線の起源 ~理論的研究を中心に~”, 研究会「宇宙線で繋ぐ文明・地球環境・太陽系・銀河」, 京都大学理学研究科セミナーハウス, 招待講演, 2022年10月
[17] “大質量降着円盤の理論モデル〜ガンマ線バーストとコンパクト連星合体への応用〜”, 宇宙線研究所共同利用小研究会「高エネルギー現象で探る宇宙の多様性II」, 東京大学宇宙線研究所, 招待講演, 2022年11月
[18] “活動銀河核の軟Ｘ線超過の起源”, ブラックホールジェット・降着円盤・円盤風研究会2023, 東北大学, 2023年3月
[19] “活動銀河核の軟Ｘ線超過の起源：温かいコロナの加熱とその安定性”, 日本天文学会春季年会, 立教大学, 2023年3月
[20] “活動銀河核の軟Ｘ線超過の起源としての温かいコロナモデル”, 第11回山田研究会「宇宙における降着現象〜活動性・多様性の源〜」, 京都大学, 2023年6月
[21] “銀河宇宙線原子核スペクトルの理論的解釈とその検証法について”, CALET による銀河宇宙線・ガンマ線観測の現状と展望, 東京大学宇宙線研究所, 2024年2月
[22] “超巨大ブラックホールの超エディントン降着成長における熱伝導の影響”, ブラックホール大研究会〜星質量から超巨大ブラックホールまで〜, 静岡県御殿場市 (オンライン参加), 2024年3月
[23] “超巨大ブラックホールの超エディントン降着成長における熱伝導の影響”, 日本天文学会春季年会, オンライン開催, 2024年3月
[24] “因果律を保った高エネルギー宇宙線粒子の伝搬の定式化に向けて”, 日本天文学会秋季年会, 関西学院大学, 2024年9月
[25] "Detection of CO Absorption Line in the Nucleus of M87", ALMA Workshop 2024: AGN Feeding and Feedback in Massive Galaxies at the Center of Galaxy Clusters, 鹿児島大学, 2024年11月
[26] "孤立ブラックホールの電波観測の可能性", ブラックホール探査研究会2025, 東京都立大学, 2025年3月
[27] "Theoretical Models of Accretion Disk Coronae in Active Galactic Nuclei", ALMA Workshop 2024: Revealing the Nature of Supermassive Black Hole Coronae with Synergy of XRISM and ALMA, 大阪大学中之島センター, 招待講演, 2025年3月
[28] "ALMAによるM87中心領域からの分子ガス検出報告の真偽", 日本天文学会春季年会, 水戸市民会館, 2025年3月
総説・レビュー
[1]「ブラックホール降着円盤からのX線放射の理論モデル」川中 宣太, 日本天文学会月刊誌《天文月報》, 2008年12月号, 717-726
[2] 「天体起源の宇宙線電子・陽電子について」川中 宣太, 日本天文学会月刊誌《天文月報》, 2014年3月号, 154-162
[3] 書評「ガンマ線バースト」（河合誠之・浅野勝晃著、日本評論社）川中宣太, 日本天文学会月刊誌《天文月報》，2019年7月号, 507
著書
[1] 「宗教と科学の対話: -宇宙の摂理への想い その四」高野山大学・編, 企業開発センターKKCネクスト出版 （pp172-191「星の最期とその後」）