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Watanabe Naoki

Institute of Low Temperature Science Frontier Ice and Snow ScienceProfessor

Researcher basic information

■ Degree
  • (BLANK)
■ URL
researchmap URLホームページURL■ Various IDs
ORCID IDResearcher ID
  • A-7451-2012
J-Global ID■ Research Keywords and Fields
Research Keyword
  • 原子・分子
  • 星間物質
  • 低温表面反応
  • atoms & molecules
  • ice surface
  • Astrochemistry
Research Field
  • Natural Science, Space and planetary sciences
  • Natural Science, Semiconductors, optical properties of condensed matter and atomic physics
■ Educational Organization

Career

■ Career
Career
  • Oct. 2009 - Present
    Hokkaido University, 低温科学研究所, 教授
  • Apr. 2022 - Mar. 2026
    北海道大学低温科学研究所 所長
  • Apr. 2018 - Mar. 2024
    北海道大学ディスティングイッシュトプロフェッサー
  • Oct. 2020 - Mar. 2022
    北海道大学総長補佐
  • 2006 - Sep. 2009
    Hokkaido University, Institute of Low Temperature Science, 准教授
  • Jul. 1996 - 2006
    Hokkaido University, Institute of Low Temperature Science, 助手
  • Aug. 2000 - Aug. 2001
    University College London, Department of Physics and Astronomy, 客員研究員
  • Apr. 1994 - Jun. 1996
    理化学研究所, 原子物理研究室, 基礎科学特別研究員
  • Oct. 1993 - Mar. 1994
    理化学研究所, 奨励研究員
Educational Background
  • Apr. 1990 - Mar. 1993, Tokyo Metropolitan University, Graduate School, Division of Natural Science
  • Apr. 1988 - Mar. 1990, Tokyo Metropolitan University, Graduate School of Science, 物理学専攻(修士課程), Japan
Position History
  • 教育研究評議会評議員, 2022年4月1日 - 2024年3月31日
  • 研究戦略室室員, 2020年10月12日 - 2022年3月31日
  • 総長補佐, 2020年10月12日 - 2022年3月31日
  • 低温科学研究所長, 2022年4月1日 - 2024年3月31日
  • 低温科学研究所長, 2024年4月1日 - 2026年3月31日
  • 低温科学研究所副所長, 2018年4月1日 - 2020年3月31日
  • 低温科学研究所副所長, 2020年4月1日 - 2022年3月31日

Research activity information

■ Awards
  • Apr. 2020, 令和2年度 科学技術分野の文部科学大臣表彰 科学技術賞 研究部門
■ Papers
■ Other Activities and Achievements
■ Lectures, oral presentations, etc.
  • Experimental approach to fast ortho to para nuclear spin conversion of hydrogen molecule on dust grain analogues
    Naoki Watanabe
    COSPAR 2021, Chemical Evolution and Origin of Life, English, Invited oral presentation
    29 Jan. 2021 - 01 Feb. 2021, [Invited]
  • Clarifying a proton-hole transfer in ice by the new method of OH detection
    Naoki Watanabe
    Frontier of structures and dynamics of water by advanced spectroscopic techniques, 27 Oct. 2020, English, Invited oral presentation
    [Invited]
  • Behavior of OH radical on ice
    Naoki Watanabe
    Water in the Universe in the ACS National Meeting, English, Invited oral presentation
    25 Aug. 2019 - 29 Aug. 2019, [Invited]
  • Ortho-to-Para Ratios in water and H2 desorbed from ice --Experimental view--
    Naoki Watanabe
    Astrochemistry: From nanometers to megaparsecs - A symposium in honour of John H. Black, English, Invited oral presentation
    24 Jun. 2019 - 28 Jun. 2019, [Invited]
  • Behavior of OH Radical on an Ice Surface at Low Temperatures
    Naoki Watanabe
    35th Symposium on Chemical Kinetics and Dynamics, English, Invited oral presentation
    05 Jun. 2019 - 07 Jun. 2019, [Invited]
  • Detection of OH radicals on amorphous solid water
    Naoki Watanabe
    IAU Symposium 350 Laboratory Astrophysics: From Observations to Interpretation, English, Invited oral presentation
    14 Apr. 2019 - 29 Apr. 2019, [Invited]
  • Infrared measurements on efficient chemical desorption of hydrogen sulfide from amorphous solid water
    Naoki Watanabe
    Oxygen in Space, English, Invited oral presentation
    16 Oct. 2018 - 17 Oct. 2018, [Invited]
  • 星間塵表面の化学:重水素濃集に果たす役割
    渡部 直樹
    日本地球化学会年会, 11 Sep. 2018, Japanese, Invited oral presentation
    [Invited], [Domestic Conference]
  • Measurements of activation energies for diffusion of hydrogen atom on pure CO solid
    N. Watanabe
    European Conference On Surface Science (ECOSS34), 26 Aug. 2018, English, Invited oral presentation
    [Invited], [International presentation]
  • Infrared Measurements of Efficient Chemical Desorption of Hydrogen Sulfide from Amorphous Solid Water
    N. Watanabe
    COSPAR 2018, The Evolving Chemical Universe: from proto-stars to the Origin of Life, 26 Jul. 2018, English, Invited oral presentation
    [Invited], [International presentation]
  • Surface Chemistry of the ISM: Experimental Approach to grain surface processes
    N. Watanabe
    The Olympian Symposium 2018 Gas and stars from milli- to mega- parsecs, 01 May 2018, English, Invited oral presentation
    [Invited], [International presentation]
  • Strong temperature dependence of H2 nuclear spin conversion on ice: what controls the rate?
    Naoki Watanabe
    Dust and Ice Particles Spectroscopy and Scattering, English, Invited oral presentation
    25 Sep. 2017 - 28 Sep. 2017, [Invited]
  • H 2ortho-para conversion on amorphous solid water
    N. Watanabe
    International Conference on Photonic Electronic and Atomic Collisions(ICPEAC2017), 26 Jul. 2017, English, Invited oral presentation
    [Invited], [International presentation]
  • 低温氷表面における水素の化学物理過程:宇宙の分子進化の鍵
    渡部 直樹
    日本真空学会関西支部&日本表面科学会関西支部合同セミナー2017水素の挙動と物質科学 -最近の展開-, 06 Jul. 2017, Japanese, Invited oral presentation
    [Invited], [Domestic Conference]
  • Ortho-to-para nuclear spin conversion of H2 on ice: a key to chemical evolution in space
    Naoki Watanabe
    XXXVI BIENNAIAL MEETING OF THE SPANISh ROYAL SOCIETY OF CHEMISTRY, 25 Jun. 2017, English, Invited oral presentation
    [Invited], [International presentation]
  • Physicochemical processes on Ice Dust towards Deuterium Enrichment
    N. Watanabe
    International Symposium on Molecular Spectroscopy, 19 Jun. 2017, English, Invited oral presentation
    [Invited], [International presentation]
  • Physicohemical Processes on ice dust towards deuterium enrichment
    N.Watanabe
    International Symposium on Molecular Spectroscopy 72ND MEETING, 19 Jun. 2017, English, Invited oral presentation
    [Invited], [International presentation]
  • Ortho-to-para ratios of hydrogen molecules desorbed from ice at around 10 K: What happens on cosmic ice dust?
    N. Watanabe; H. Ueta; T. Hama; A. Kouchi
    The 253thAmerican Chemical Society National Meeting, 02 Apr. 2017, English, Invited oral presentation
    [Invited], [International presentation]
  • Strong temperature dependence of ortho-to-para conversion of H2 on amorphous solid water at around 10 K
    N. Watanabe
    EUROPEAN CONFERNCE ON LABORATORY ASTROPHYSICS (ECLA2016) GAS ON THE ROCKS, 21 Nov. 2016, English, Oral presentation
    Madrid, Spain, [Invited], [International presentation]
  • Experimental approach to hydrogen chemistry on grain surfaces: molecular formation
    N. Watanabe
    Center for Astrochemical Studies Seminar, 12 Oct. 2016, English, Invited oral presentation
    Max-Planck-Institut für extraterrestrische Physik, Germany, [Invited], [International presentation]
  • Experimental approach to ortho-to-para ratio of hydrogen and water molecules desorbed from ice at around 10 K
    Naoki Watanabe
    Workshop on Astrochemistry in Star and Planet Formation, 16 Feb. 2016, English, Invited oral presentation
    Riken, Saitama, Japan, [Invited], [International presentation]
  • Deuterium chemistry and nuclear spin conversion on grain surfaces: implication to deuterium enrichment
    N. Watanabe
    From clouds to protoplanetary disk: the astrochemical link, 05 Oct. 2015, English, Invited oral presentation
    Hans Harnack Haus, Berlin, Germany, [Invited], [International presentation]
  • Grain Surface Chemistry: What Happens Without Photons and Ions
    N. Watanabe
    A symposium to honor Lou Allamandola’s Contributions to the Molecular Universe, 13 Sep. 2015, English, Invited oral presentation
    Annapolis, MD, USA, [Invited], [International presentation]
  • Role of Tunneling in the Formation and Deuterium Enrichment of Molecules on Dust Grains
    Naoki Watanabe
    Astrobiology Science Conference 2015, English, Invited oral presentation
    15 Jun. 2015 - 19 Jun. 2015, [Invited]
  • Experimental Approach to Chemistry of Cosmic Dust
    N. Watanabe
    COST Action Our Astrochemical History CM1401, 25 May 2015, English, Invited oral presentation
    The Czech Republic, [Invited], [International presentation]
  • Experimental approach to nonenergetic physicochemical processes on icy grains
    Naoki Watanabe
    Icy Grain Chemistry for Formation of Complex Organic Molecules: From Molecular Clouds to Protoplanetary Disks, Comets and Meteorites, 05 Mar. 2015, Japanese, Invited oral presentation
    Tokyo Institute of Technology, Japan, [Invited], [International presentation]
  • What controls the diffusion mechanism of hydrogen atom on ice?
    Naoki Watanabe
    Second Workshop on Experimental Laboratory Astrophysics, English, Invited oral presentation
    23 Feb. 2015 - 26 Feb. 2015, [Invited]
  • Nuclear spin temperatures of hydrogen and water molecules formed and trapped on ice
    Naoki Watanabe
    Nuclear Spin Effects in Astrochemistry 2014, English, Invited oral presentation
    09 Jun. 2014 - 11 Jun. 2014, [Invited]
  • Diffusion of hydrogen atom on amorphous solid water: Thermal or tunneling?
    N. Watanabe
    247th ACS Chemistry & Materials for Energy, 16 Mar. 2014, English, Invited oral presentation
    Dallas, USA, [Invited], [International presentation]
  • Physics and chemistry of hydrogen on cosmic dust: diffusion, spin temperatures, and water formation
    N. Watanabe; T. Hama; H. Hidaka; Y. Kimura; A. Kouchi; Y. Oba; V. Pirronello
    First Workshop on Experimental Laboratory Astrophysics, Feb. 2013, English, Invited oral presentation
    Kauai, Hawaii, [Invited], [International presentation]
  • Physicochemical Processes of Hydrogen on Ice: A Key for Chemical Evolution in Space
    N. Watanabe
    2nd International Symposium on Hierarchy and Holism, Feb. 2013, English, Invited oral presentation
    Tokyo, Japan, [Invited], [International presentation]
  • Surface diffusion mechanism of atomic hydrogen and the ortho/para ratio of nascent H2 molecule on amorphous solid water at around 10 K
    N. Watanabe
    International Lorentz Center Workshop: Dynamical Phenomena at Surfaces: The Role of Complexity, Nov. 2012, English
    Leiden, The Netherlands, [Invited]
  • Grain surface processes at very low temperatures: hydrogen diffusion and tunneling reactions
    N. Watanabe
    Gordon Research Conference, Radiation Driven Processes in Physics, Chemistry, Biology, and Industry, Jul. 2012, English
    New Hampshire, USA, [Invited]
  • Spin temperatures of hydrogen and water molecules on amorphous solid water
    N.Watanabe
    ASTROCHEM 2012, Jul. 2012, English
    Kolkata, India, [Invited]
  • Hydrogen processes on dust grains: H atom diffusion and water formation
    N.Watanabe
    30th COSPAR Scientific Assembly, Jul. 2012, English
    Mysore, India, [Invited]
  • Hydrogen chemistry on cold grain surfaces
    N.Watanabe
    XVIIIth Symposium on Atomic, Cluster, and Surface Physics, Jan. 2012, English
    Alpe d'Huez, France, [Invited]
  • Hydrogen tunneling reaction and its isotope effect at a low temperature ice surface: Origin of deuterium enrichments in interstellar formaldehyde and methanol
    N. Watanabe; H. Hidaka; A. Kouchi; N. Watanabe; H. Hidaka; A. Kouchi
    International Conference on the Research of Chemistry and Physics of Matrix Isolated Species(MATRIX2011), Jul. 2011, English
    Vancouver, Canada, [Invited]
  • Ice surface chemistry of hydrogen atom in space
    N. Watanabe; H. Hidaka; T. Hama; A. Kouchi; T. Chigai; Y. Kimura
    27th European Conference on Surface Science, ECOSS 27, Aug. 2010, English
    Groningen, the Netherlands, [Invited]
  • Surface processes of atomic hydrogen at very low temperatures relevant to astrochemistry
    N. Watanabe
    24th International Conference on Atomic Collisions in Solids ICACS- 24, Jul. 2010, English
    Krak?w, Poland, [Invited]
  • Chemistry of atomic hydrogen on interstellar ice grains at very low temperatures
    N. Watanabe; H. Hidaka; A. Kouchi; T. Hama; Y. Kimura
    Western Pacific Geophysics Meeting, Jun. 2010, English
    Taipei, Taiwan, [Invited]
  • Physicochemical processes of atomic hydrogen on amorphous solid water at very low temperatures
    N. Watanabe; A. Kouchi; H. Hidaka; Y. Kimura; T. Hama
    239th American Chemical Society National Meeting & Exposition, Mar. 2010, English
    San Francisco, USA, [Invited]
  • Ice surface reactions: its role in chemical evolution in space
    N.Watanabe
    ILTS International Symposium "Frontier of Low Temperature Science", Sapporo, Nov. 2009, English
    Sapporo, [Invited]
  • Tunneling reactions of atomic hydrogen and molecules on amorphous solid water at very low temperatures
    N. Watanabe
    Horiba-ISSP International Symposium on “Hydrogen and water in condensed matter physics”, Oct. 2009, English
    Chiba, [Invited]
  • Nonenergetic reactions between hydrogen and molecules On Interstellar Grain Surfaces
    N. Watanabe
    XXVI International Conference on Photonic, Electronic, and Atomic Collisions, Jul. 2009, English
    Michigan, USA, [Invited]
  • Reactions of hydrogen atoms and molecules on amorphous solid water at very low temperatures
    N. Watanabe
    Gordon Research Conferences, Physics & Chemistry of Matrix-Isolated Species, Jul. 2009, English
    Oxford, UK, [Invited]
  • Experimental approach to grain surface reactions of hydrogen and deuterium atoms
    N.Watanabe
    International Lorentz Center Workshop: Interstellar Surfaces: From Laboratory to Models, Oct. 2008, English
    Leiden, Holland, [Invited]
  • Grain surface chemistry: fractionation routes
    N. Watanabe
    The Molecular Univers: an International Meeting on Physics and Chemistry of the Intersteller Medium, May 2008, English
    Arcachon, France, [Invited]
  • Simultaneous irradiation experiments of H2O-CO binary ice with UV photons and cold H atoms
    N. Watanabe; A. Nagaoka; O. MouriI; A. Kouchi; V. Pirronello
    Asia-Oceania Geosciences Society Annual Meeting, Aug. 2007, English
    Bangkok, Thailand, [Invited]
  • Laboratory study of chemical processes on interstellar ice grains
    N. Watanabe; A. Nagaoka; H. Hidaka; A. Kouchi
    XXIV International Union of Feodesy and Geophysics (IUGG) General Assembly, Jul. 2007, English
    Perguia, Italy, [Invited]
  • Reactions of hydrogen and deuterium atoms with CO, formaldehyde, and methanol on ice grains
    N.Watanabe
    International Astrophysics and Astrochemistry Meeting: Molecules in Space & Laboratory, May 2007, English
    Paris, France, [Invited]
  • Formation of simple organic molecules by Hydrogenation on grain surfaces
    N. Watanabe
    International Astronomical Union Symposium: Astrochemistry,, Aug. 2005, English
    California,USA, [Invited]
  • Formation of deuterated methanol by surface reactions at 10 K
    N. Watanabe; A. Nagaoka; A. Kouchi
    Asia-Oceania Geosciences Society Annual Meeting, Jun. 2005, English
    Singapore, [Invited]
  • Evolution of CO molecule on dusts in dense core: formation of H2CO and CH3OH
    N. Watanabe
    The 4th International Symposium on New Trends of Physics, Recent Advances in Astrophysics and Planetary Science -from the early universe to the Solar system-, Mar. 2005, English
    Sapporo, [Invited]
■ Syllabus
  • 環境と人間, 2024年, 学士課程, 全学教育
■ Affiliated academic society
  • JAPAN GEOSCIENCE UNION
  • 原子衝突学会
  • THE JAPANESE SOCIETY FOR PLANETARY SCIENCES
  • 日本物理学会
■ Research Themes
  • Exploration of the possibility of hydrated silicate formation in early stage of molecular clouds
    Grants-in-Aid for Scientific Research
    01 Apr. 2024 - 31 Mar. 2027
    中井 陽一; 渡部 直樹
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Institute of Physical and Chemical Research, 24K00699
  • ラジカルの拡散が活性化させる星間塵表面での分子進化:複雑有機分子生成の鍵
    科学研究費助成事業 基盤研究(A)
    01 Apr. 2022 - 31 Mar. 2027
    渡部 直樹; 柘植 雅士; Sameera W.M.C.
    日本学術振興会, 基盤研究(A), 北海道大学, 22H00159
  • Theoretical astrochemistry based on microscopic processes in the gas and solid phases
    Grants-in-Aid for Scientific Research
    19 Nov. 2020 - 31 Mar. 2025
    相川 祐理; 古家 健次; 高柳 敏幸; 山崎 祥平; 花輪 知幸; 吉田 直紀; 渡部 直樹
    Japan Society for the Promotion of Science, Grant-in-Aid for Transformative Research Areas (A), The University of Tokyo, 20H05847
  • Next Generation Astrochemistry: Transformative Action Based on Understandings of Microscopic Chemical Processes
    Grants-in-Aid for Scientific Research
    19 Nov. 2020 - 31 Mar. 2025
    坂井 南美; 橘 省吾; 中野 祐司; 相川 祐理; 今田 裕; 渡部 直樹
    低温低密度の単純な環境を前提としてきた星間化学を刷新し、惑星系形成領域のように、ガスや固体物質の組成が劇的に変化する広範な物理環境に対応できる強固な学術基盤を構築するための領域全体の連携を支援した。大きく異なる分野の融合研究を推進する計画であるため、分野間の相互研究理解が極めて重要である。そのために、下記3つの手法で相互理解を深めた。
    ①話題提供:総括班会議での運営議論の後、各班代表から新たな課題となりつつあるテーマや、重要なテーマの紹介を行ってもらい、議論を行った。各班の研究計画への他班からのフィードバックとしての役割を担った。
    ②セミナー:各班の研究テーマの背景にある基本的知見を、学生などを含めた他班の若手までもが理解しなければ、真の意味での融合・共同研究は難しい。このため、修士学生でもわかりやすいように日本語での基礎セミナーを1-2ヶ月に1度のペースで開催し始めた。また、参加できなかったメンバーのために、期間を定めて動画の公開も行った。
    ③ミクロ班会合:素過程理解に基づく学理の再構築のためには、どのような分子や化学反応素過程に着目すべきかを、逐次議論していくことが重要となる。そのために、より踏み込んだ詳細議論を行う場として、1-2ヶ月に1度のペースで開始した。
    これらに加え、協力研究者である渡部直樹教授を連携コーディネータとし、班間での議論促進に取り組んだ。例として、2021年11月(コロナにより約1年延期)にInternational workshop on interstellar matterを開催した。150名もの異分野研究者が集い、非常に活発に分野をまたぐテーマについての議論が行われた。 なお、コロナ禍であったため、国外からの招聘や出張旅費の計画は臨機応変に組替えを行った。具体的には、オンライン議論促進アプリ・ソフトの活用や動画記録でのセミナー開催などが挙げられる。
    Japan Society for the Promotion of Science, Grant-in-Aid for Transformative Research Areas (A), Institute of Physical and Chemical Research, 20H05844
  • 極低温星間塵表面における有機硫黄分子の化学反応
    科学研究費助成事業
    08 Mar. 2023 - 31 Mar. 2024
    渡部 直樹; NGUYEN THANH
    本研究の目的は,星や惑星誕生の場である星間分子雲に存在する固体微粒子,氷星間塵上での硫黄を含む分子の化学反応を実験的に検証し,宇宙における硫黄の化学進化をより詳細に理解することである。研究対象として,これまでに星間分子雲で観測されている硫黄を含む化学種,硫化カルボニル(OCS),メチルメルカプタン(CH3SH),二酸化硫黄(SO2)を選択した。超高真空(10-8Pa程度)チャンバー内で作製し,10ケルビン(K)に冷却されたアモルファス氷上にそれらの分子を蒸着し,水素原子との反応を検証した。反応はフーリエ変換型赤外吸収分光高度計でその場観測され,さらに氷から脱離する成分は四重極型質量分析計で分析された。
    いずれの分子も水素原子との反応には活性化エネルギー障壁が存在するため,通常10K程度の極低温では熱的に反応しえないが,量子トンネル効果による水素原子付加反応が進行した。OCSからはチオギ酸(HCOSH),SO2からはスルフィン酸(HSOOH)など,これまでの天文観測ではなじみのなかった硫黄を含む分子が生成し,CH3SHを含むいずれの分子も水素原子との反応で最終的に硫化水素(H2S)を生成した。硫化水素は水素原子との反応で容易にガス化するため,これらの硫黄を含む分子はいずれも氷星間塵上には固体として残りにくい化学種だと考えられる。これは,これまでの天文観測結果と極めて調和的である。
    上記の研究成果の大半は既に学術論文として公表され(Nguyen et al. 2021, 2023; The Astrophysical Journal),現時点でもう1報の論文投稿の準備がほぼ整っている。さらに,関連する化学反応を対象とした量子化学計算論文に実験データを提供し,実験と理論の両面で星間化学の発展に大きく貢献した。
    日本学術振興会, 特別研究員奨励費, 北海道大学, 22KF0001
  • 極低温星間塵表面における有機硫黄分子の化学反応
    科学研究費助成事業
    18 Nov. 2021 - 31 Mar. 2024
    渡部 直樹; NGUYEN THANH
    本研究は,極低温の星間塵表面における有機硫黄分子の化学反応を実験的に調べることを目的としている。本年は,硫黄を含む化合物の中で唯一固体として検出されている星間分子:硫化カルボニル(OCS)に着目し,星間塵表面でのH原子との反応性を調べた。真空中で10ケルビンに冷却したアモルファスH2O氷上に固体OCSを作製し,水素原子と反応させたところ,生成物としてCO, H2S, H2CO, およびCH3OHが検出された。量子化学計算により,氷とOCS分子の結合エネルギーや各種表面反応の活性化エネルギーを求めたところ,これらを生成する過程として,OCS + H → OCSHが始めに生じ,その後,さらに水素原子付加反応 OCSH + H → H2S + COが生じる連続反応であることがわかった。H2CO, CH3OHは左記の反応で生成したCOにH原子がさらに逐次付加して生成したものである。また,最近の天文観測で星間空間に見つかっているHC(O)SHが,氷星間塵表面でHCOとSHラジカルとの反応により生成しうることが初めて示唆された。この反応経路はこれまで知られていなかった新たな生成機構を示すものである。また,本研究により,比較的な簡単なOCS分子から,外部からのエネルギーを必要としないH原子付加反応により,多様な分子が生成されることが分かった。また,S含有物として,もっとも存在度が高いと思われるH2Sが最終生成物として残ることが明らかになった。
    日本学術振興会, 特別研究員奨励費, 北海道大学, 21F21319
  • Chemical evolution on cosmic dust: approach from elementary processes
    Grants-in-Aid for Scientific Research Grant-in-Aid for Specially Promoted Research
    25 Apr. 2017 - 31 Mar. 2022
    Watanabe Naoki
    Using novel experimental methods and quantum chemical calculations, we demonstrated various physicochemical processes on the surfaces of cosmic dust analogues, which play an important role in evolution of molecules in space. Notable findings were mode on (1) formation and desorption process of some organic molecules and sulfer- and phosphorous-containing molecules; (2) deuterium fractionation of molecules; (3) nuclear-spin conversion of hydrogen molecules on dust. Furthermore, direct observation of amorphous ice at around 10 K was first successful with cryogenic transmission electron microscope and atomic force microscope.
    Japan Society for the Promotion of Science, Grant-in-Aid for Specially Promoted Research, Hokkaido University, 17H06087
  • 星間分子雲初期に起こるケイ酸塩星間塵表面での分子進化
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A)
    01 Apr. 2017 - 31 Mar. 2018
    渡部 直樹; 大場 康弘
    本研究は,未解明になっている,星間塵表面に氷マントルが生成される以前の,ケイ酸塩星間塵表面での分子生成,重水素濃集に着目し,化学・物理素過程を系統的かつ定量的な実験で調べ,星間塵上での分子進化の解明を目指すものである。採択と同時に,研究の根幹をなす,新たなケイ酸塩試料作製装置開発に向け,真空ポンプ,真空部品などを購入した。また,表面を原子間力顕微鏡で評価するため,カンチレバーチップを購入した。同時に,プラズマ放電による鉱物サンプル試料の作製を業者に依頼した。ケイ酸塩試料作製装置の開発は引き続き行っているところだが,業者に作製を依頼したサンプル試料がかなり高品質であることが分かった。
    また,採択直後に東京理科大学にて,本研究課題についての研究討論を行い,本課題の独創性や重要性をアピールすることができた。
    その後,すぐに現在実施中の特別推進研究が採択されたため,本研究課題の実施は7月28日をもって終了した。しかし,上記の取り組みは特別推進研究に引き継がれるため,基盤研究Aで行った討論,整備した装置類は将来にわたって有効に活用される。
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (A), Hokkaido University, 17H01169
  • Mechanisms of formation and isotope fractionation of interstellar molecules on cosmic dust
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (S)
    31 May 2012 - 31 Mar. 2017
    WATANABE NAOKI; KOUCHI Akira
    Formation and isotope fractionation of molecules in molecular clouds are very important as the initial stage of chemical evolution toward planetary system. The aim of this project was to clarify the role of physicochemical processes on cosmic ice dust at very low temperatures which are keys in chemical evolution. We have experimentally demonstrated mechanisms of elementary processes for molecular formation and deuteration on ice at around 10 K. We determined diffusion-rates of hydrogen (deuterium) atoms on amorphous ice and formation (and deuteration) pathways and those reaction rates for water and some primordial organic molecules.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (S), Hokkaido University, 24224012
  • Experiments on io-induced nucleation to clarify a new mechanism of cosmic dust formation
    Grants-in-Aid for Scientific Research Grant-in-Aid for Challenging Exploratory Research
    01 Apr. 2014 - 31 Mar. 2016
    Watanabe Naoki; UETA Hirokazu
    Interstellar dust particles play an important role in chemical evolution of interstellar matter. Although the details of dust formation are still unknown, it is generally believed that they form in the gas phase via homogeneous nucleation. In contrast, the present study focuses on inhomogeneous ion-induced nucleation in the gas phase in which activation barriers for cluster formation decrease significantly by ion-ion induced dipole interaction. We have constructed an rf ion trap to study the cluster ion formation as the first stage of nucleation. We have been successful in storing several kinds of molecular ions and clusters and monitoring the successive reaction in the rf trap.
    Japan Society for the Promotion of Science, Grant-in-Aid for Challenging Exploratory Research, Hokkaido University, 26610137
  • Development of ultrahigh vacuum (UHV) transmission electron microscope for in-situ observation of ice
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A)
    21 Oct. 2013 - 31 Mar. 2016
    Kouchi Akira; HIDAKA Hiroshi; OBA Yasuhiro; HAMA Tetsuya; CHIGAI Takeshi; WATANABE Naoki; KIMURA Yuki; TOMARU Takayuki
    An ultrahigh vacuum (UHV) transmission electron microscope for in-situ observation of ice has been developed. We use a single tilt liquid He cooling holder for specimen cooling to 4 K. Two ports are directed to the specimen surface for in-situ studies: gas-inlet, and UV irradiation.
    Results of preliminary observation are as follows: (1) Macroscopic defect structure of vapor-deposited amorphous ice are observed at first time. (2) Formation of ice XI by UV irradiation onto ices Ih and Ic are observed at 75-100 K. On the other hand, no structural change has been observed by UV irradiation onto amorphous ice. (3) Formation of high-density amorphous ice by CO matrix sublimation method has been developed.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (A), Hokkaido University, 25247086
  • Quantitative investigation for ion-induced nucleation under non-equilibrium conditions of association/dissociation reactions: experimental approaches for elementary formation processes
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    01 Apr. 2013 - 31 Mar. 2016
    NAKAI Yoichi; WATANABE Naoki; KOJIMA Takao; HIDAKA Hiroshi
    We performed stable and precise measurements compared with previous studies for Gibbs free energy changes of stepwise association reactions of a water molecule to H3O+(H2O)n ions using a ion drift tube with a selected ion injection. Furthermore, an empirical effective temperature of the reaction equilibrium constants was obtained for association/dissociation reactions of a water molecule to/from H3O+(H2O)n ions in a pure water vapor. The effective temperature means a representative physical quantity of collision energy influenced by an electric field. It was found that a new parameter describing electric field dependence of the effective temperature presumably reflects structures of H3O+(H2O)n ions. We also performed R&D of ion handling methods in an RF ion trap, such as an ion mass selection, in order to make use of RF ion traps for cluster formation experiments.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Institute of Physical and Chemical Research, 25287148
  • Quantitative elucidation for ion induced nucleation in the atmosphere: Approach through the experiments for elementary processes
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C)
    01 Apr. 2010 - 31 Mar. 2013
    NAKAI Yoichi; WATANABE Naoki; KOJIMA Takao; HIDAKA Hiroshi
    Experimental study for cluster ion formation, early stages of ion induced nucleation, has been performed. We developed the experimental equipment, in which the region for production of initial ions is separated from that for generation of cluster ions, in order to define the reaction paths. Gibbs free energy changes for the stepwise association of an H2O molecule were measured for H3O+(H2O)n cluster ions and our method has provided more stable and precise results compared with previous measurements. In the use of initial NO+ ions, we have reduced influence of metastable NO+ ions in produced initial ions, using hydrogen buffer gas.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (C), The Institute of Physical and Chemical Research, 22540498
  • 星間塵表面反応:分子進化と同位体分別機構の新展開
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A)
    2012 - 2012
    渡部 直樹; 日高 宏; 羽馬 哲也
    本研究は,極低温下での星間塵表面反応素過程の詳細を実験的に調べ,星間分子雲での分子進化と同位体分別における星間塵の役割を明らかにすることを主たる目的としている.本研究課題が採択されると同時に,始原天体に関する国際会議(新潟),原始太陽系における鉱物・水・有機物に関する国際シンポジウム(東京)および日本地球惑星科学連合大会(千葉幕張)に出席し,星間塵表面における水分子および始原有機分子生成に関する研究の現状報告を行ない,同位体濃集プロセスに関する情報収集・議論を通して本研究の重要性や独創性を充分アピールすることができた.
    現有実験装置の改良も本研究課題の重要な目的である。まず気相の原子・分子を検出する装置を駆動するための電源ユニット(NIM標準ビン電源,クリアパス社製)を購入し,信号検出系の改善に取り組み始めた.改良は現時点でも引き続き行っているところだが,これにより,実験の際の信号/ノイズ比が向上し,さらに規則的に現れる電気的なノイズを除去することが可能になると予想され、実験値の精度向上等大きな効果が期待される.
    その後すぐに現在実施中の基盤研究Sが採択されたため,本研究課題の実施は5月31日をもって終了した.しかし,上記の取り組みは基盤研究Sに引き継がれるため,基盤研究Aで行った発表・研究議論,整備した物品は、将来にわたって有効に活用される.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (A), Hokkaido University, 24244083
  • Observation of surface structure of amorphous ice and role of amorphous ice in surface atomic reactions at low temperatures
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2010 - 2012
    KOUCHI Akira; WATANABE Naoki; HIDAKA Hiroshi
    An ultrahigh vacuum low temperature atomic force microscope for in-situ deposition of amorphous ice and for observation of ice surface has been developed. We have succeeded to observe the surface structure of amorphous ice and found that the surface of amorphous ice is very porous. This might cause the catalytic properties of amorphous ice in surface atomic reactions.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Hokkaido University, 22340157
  • Ice surface processes: tunneling reactions and isotope fractionation
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research on Innovative Areas (Research a proposed research project)
    2009 - 2011
    WATANABE Naoki; HIDAKA Hiroshi
    Ice surface reactions relevant to chemical evolution and deuterium fractionation were experimentally investigated. Activation energies for ice-surface diffusion of H and D atoms were determined. It was found that effective mass of reaction system is a control-factor of tunneling reactions. The reactivities of tunneling reactions related to deuterium fraction of formaldehyde can be well explained by the effective masses. A novel route of CO_2 formation on the ice surface was found.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research on Innovative Areas (Research a proposed research project), Hokkaido University, 21200048
  • Deuterium fractionation of water molecule via grain surface reactions at very low temperatures
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C)
    2009 - 2011
    WATANABE Naoki; HIDAKA Hiroshi
    Water molecule formation and its deuterium fractionation via surface tunneling reactions were investigated experimentally, relevant to chemical evolution in a molecular cloud. We found that H_2O molecule is produced by tunneling reaction, OH + H_2, at very low temperature surfaces and that, from the isotope effect on the above reaction, the formation of OD is essential for deuterium fractionation of water rather than HD or D_2 formation.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (C), Hokkaido University, 21540502
  • Evaluation of catalytic effect of amorphous ice on the surface atomic reactions
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (S)
    2005 - 2009
    KOUCHI Akira; WATANABE Naoki
    Surface atomic reactions on interstellar grains at low temperatures are investigated experimentally using newly developed experimental setup. Formation mechanisms of H_2, H_2O, CO_2, H_2CO, and CH_3OH are clarified. Measurement of sticking coefficient of H-atoms onto amorphous water ice enables us to deduce reaction rate constants. We also showed that amorphous water ice enhances reactivity at higher temperatures compared with pure solid reactants.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (S), Hokkaido University, 17104006
  • Role of cosmic-grain surface reactions in the deuterium fractionationof interstellar molecules
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2007 - 2008
    WATANABE Naoki; HIDAKA HIROSHI
    星間分子の重水素濃集プロセスとして研究代表者らが提唱している極低温星間塵表面反応を, 実験により定量的に評価した. 特に, 高度な重水素濃集が観測で確認されているホルムアルデヒド, メタノールの重水素化表面反応に焦点をあて, 重要な反応経路について実効的な反応速度定数を決定し, 上記分子種に関する重水素濃集の星間塵表面反応ネットワークを完成させた.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Hokkaido University, 19340167
  • Experimental and theoretical studies of the evolution from dust to exoplanets
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research on Priority Areas
    2004 - 2008
    YAMAMORO Tetsuo
    惑星系円盤におけるダストの衝突進化と熱進化の素過程,観測結果を読み解くうえで重要な光学に関する研究,ダスト生成とその後続解析実験,ダスト衝突実験,氷表面における分子反応等,物質進化の総合的研究を展開した.加えて,この分野の研究基盤形成にも貢献した.研究グループの交流を促進し,国内の関連研究グループの組織化を図り,研究コミュニティー形成を積極的に推進した
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research on Priority Areas, Hokkaido University, 16077203
  • 星間塵表面における重水素濃縮機構
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research on Priority Areas
    2004 - 2005
    渡部 直樹; 香内 晃
    本研究では,これまで全く情報の無かった星間塵表面における星間分子の重水素濃集過程を実験的に調べることを目的としている.本年度は以下のことを明らかにした.
    ホルムアルデヒド(H_2CO)における重水素濃集過程を調べるために,10KのH_2O氷(疑似星間塵表面)上でCO+DおよびH_2CO+D,D_2CO+Hの表面反応を定性的に調べた.その結果,すべての反応で重水素(D)原子を含む重水素体ホルムアルデヒドが生成された.実験条件から推測すると,これらの反応はすべて宇宙空間で起こりうることが解った.大雑把な見積もりでは重水素体を生成するのにもっとも速い反応はH_2CO+Dの系に見られるH-D置換反応である.しかし,一度重水素体が生成してもH原子との反応でD原子が再びH原子に入れ替わる反応(D_2CO+H→・・→H_2CO)も見られたことから,ホルムアルデヒドにおけるH-D置換反応が結果として重水素濃集過程になりうるかどうかを見極めるにはより定量的な実験が必要であることがわかった.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research on Priority Areas, Hokkaido University, 16036201
  • Surface reactions of atoms and the mechanism of deuterium fractionation on inter Stellar dusts at the very low temperature
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2004 - 2005
    WATANABE Naoki; KOUCHI Akira
    This project was carried out for the purpose of obtaining the reaction channels and rates of the formation of interstellar molecules via surface reactions of atoms and also revealing the origin of deuterium enrichment in methanol molecules observed. We summarize the results of our research as follows.
    1.The rate of addition of deuterium atoms to solid CO molecule is as slow as one-tenths of that of hydrogen addition, indicating that the deuterium addition is unlikely for the first step of the deuterium enrichment of methanol.
    2.We confirmed that H-D substitution reactions in CH_3OH-d_n(CH_3OH-d_n+D→CH_3OH-d_,n=0-2) proceed in solid phase at 〜10K. The reaction rates of the substitution decrease as number of D atoms in methanol, n, increases
    3.We demonstrated for the first time that deuterium enrichment observed can be achieved partly by the grain-surface reactions. Our quantitative data shows that H-D substitution is more efficient to produce deuterated methanol than the successive deuterium addition to CO in a molecular cloud.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), HOKKAIDO UNIVERSITY, 16340145
  • UV-induced diamond formation in interstellar clouds
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2003 - 2004
    KOUCHI Akira; ARAKAWA Masahiiko; WATANABE Naoki
    New formation routes of diamond in interstellar clouds and parent bodies of carbonaceous chondrites are found based on laboratory experiments. It is shown that diamond precursor nucleated as a result of UV photolysis of interstellar ice mixtures in molecular clouds, and grew with further UV irradiation in diffuse clouds. The present study supports the occurrence of diamonds in interstellar clouds, and suggests that diamond is ubiquitous in space. Furthermore, we performed experiments on the aqueous alteration and the subsequent thermal metamorphism of organic materials formed in molecular cloud, and found that diamonds formed by this process in the parent bodies of carbonaceous chondrites. The various characteristics of nano-diamonds in chondrites and interplanetary dusts are well explained by these new formation routes.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Hokkaido University, 15340180
  • Development of electrostatic accelerator for ice dust and the aggregates
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2001 - 2003
    ARAKAWA Masahiko; WATANABE Naoki; MAENO Norikazu
    We have developed an electrostatic accelerator to launch a ice dust and ice aggregates at a wide range of velocities from cm/s to km/s. The ice sample launched was prepared by a condensation, method : a cold copper plate cooled by liquid nitrogen was subjected to an air saturated with water vapor at -10℃. The condensed icy dust is an almost spherical shape with the size of 10 μm, Ice aggregates were grown by collecting each ice dust under high electric field more than 100 V/cm. The aggregate was charged under the electric field, so that it was launched by the electrostatic attraction. The relationship between the electric field and the velocity is derived as follows for the aggregates of 500μm.: V_i=0.25(V_/d)^<0.9> (m/s), V_i: velocity, V_o: Voltage, d: distance between electrodes (d=2.5mm). The launch velocity is strongly affected by the air drag for the small aggregates, so we have set a vacuum chamber to eliminate the gas drag to the aggregates in the acceleration. We also used a longer acceleration tube to avoid disruption of the aggregates by the strong attraction force. As a result we have achieved 20m/s for 500μm aggregate at the electric field of 1kV/mm and 1 bar. In the evacuated condition of 0.1 bar, the launched velocity increased about 3 to 4 times higher than that of 1 bar at the same electric field strength. This means that it could be possible to achieve more than 100 m/s for ice aggregate of 500 μm at 1kV/mm.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), HOKKAIDO UNIVERSITY, 13554015
  • Collisional sticking of organic grains in the solar nebula
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    2000 - 2001
    KOUCHI Akira; WATANABE Seiichiro; WATANABE Naoki; ARAKAWA Masahiko
    Heating and collision experiments were performed involving interstellar organic material analogue to determine the distribution of interstellar organic material in the proto solar nebula and to investigate the growth of organic grains. We found that there were interstellar organic grains in 2.1-3.0 AU, silicate grains <2.1 AU, and ice grains>3.0 AU. We also found that gas evaporated at around 2.2 AU is very reductive. The organic material in 2.1-3.0 AU is very sticky ; the sticking threshold velocity of the mm-size organic grains is 5 m/s. This shows a very rapid coagulation of organic grain aggregates, the formation of planetesimals even the early stage of the turbulent accretion disk. The planetesimals in this region become achondrites' parent bodies. In contrast, the formation of planetesimals in <2.1 AU and >3.0 AU occur when passive disk is formed, because silicate and ice grains are not sticky. The planetesimals in <2.1 AU and >3.0 AU become ordinary and carbonaceous chondrites' parent bodies, respectively. In these framework, we discuss a redox state of chondrites, an oxygen isotope composition of meteorites and planets, and the formation of chondrules. We have succeded to give an explanation for various sequences among meteorites and planets by the heliocentric distance only : the sequence from the sun is the Earth, Mars, LL, L, H, E, Aubrite, HED, Acapulcoite, Ureilite, CO, CV, CM, CI.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), HOKKAIDO UNIVERSITY, 12440142
  • The observation of the growth and ifrured absorption for dust particles ecclosed in a small scale space
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C)
    1999 - 2000
    ARAKAWA Masahiko; KOUCHI Akira; WATANABE Naoki
    The purpose of this study is to clarify the growth process of cosmic dusts in the interstellar space and to determine the optical property of the cosmic dusts in the laboratory. Our final goal of this experiment is that we observe the growth process of the dust particles in collision with time when various kinds of small dusts are enclosed in a small vacuum space for a long time. The chosen materials are ices, organic matters and silicates, and their sizes are from 0.1 to 1 mm. We also intend to analyze these dusts by using a infrared absorption method. In this term, we have finished to develop the instrument to enclose the dust particles, which is the most important part of this experiment, moreover we estimated the adhesion strength among the organic dust particles.
    We succeeded to enclose molecular ions for several hours by means of the developed instrument of dust enclosure, so called RF ion trap instrument in ultra-high vacuum chamber. This instrument has characteristics that there are 4 holes of the diameter of 5mm at the ion trap electrode necessary to observe the interior and that the electric gun is set as a lower electrode. We did a preliminary test with molecular ions, then we developed the impedance matching instrument for high frequency electric field in order to arrange the experimental conditions to enclose the dust particles. We improved our electrodes for the ion trap according to these preliminary tests.
    Before we try to enclose the organic dusts, we studied the adhesion force of ethylene glycol particles, which particles were formed by a spray, at 200 K.The adhesion force was measured by a flowing method. As a result, the adhesion force of the organic matter was concluded to be several orders of magnitudes larger than that of silicate particles.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (C), HOKKAIDO UNIVERSITY, 11640470
  • Development of comet nucleus simulation experiments
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (B)
    1998 - 1999
    KOUCHI Akira; WATANABE Naoki
    We have developed new methods for making amorphous icy grains:
    1 ) CO sublimation-induced disruption method
    First, we deposited CO sample of 10 mm thickness. Second, thin film of amorphous water ice was deposited on the CO. After deposition, the substrate was heated by turning off the helium refrigerator. At temperatures around 30 K, corresponding to CO sublimation temperatures, the sublimation of CO occurred violently, and this caused the disruption of the thin film of amorphous water ice.
    2) Continuous production method by fast codeposition of HィイD22ィエD2O and COィイD22ィエD2.
    We found that continuous disruption of ice film occurred during the deposition , when deposition rate is larger than 3x10ィイD1-9ィエD1 m/s and when thickness of the film is larger than critical thickness.
    In both method, we collected amorphous icy grains falling from the substrate using grain collector. These methods enables us to perform better comet nucleus simulation experiments than hitherto performed.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (B), Institute of Low Temperature Science, HOKKAIDO UNIVERSITY, 10554027
  • Structure and physical properties of impure amorphous interstellar icy grains
    Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A)
    1997 - 1999
    AKIRA Kouichi; WATANABE Naoki
    The following research was carried out on the formation and metamorphism of amorphous icy grains and origin and evolution of comets using newly developed ultrahigh-vacuum very low temperature atomic force microscope and existing equipments :
    1) By irradiating the ultraviolet rays onto amorphous ice thin film, we analyze the formation of hydrogen molecule quantitatively. In addition, the reaction cross section was measured, and the reaction mechanism was decided.
    2) The measurements on physical properties of impure amorphous ices were carried out. The thermal conductivity of impure amorphous ice was found to be 2-3 orders of magnitude smaller than that of the amorphous ice without the defect. As a result of the differential thermal analysis, we found that the crystallization of amorphous ices including impurities were endothermic reaction.
    3) There results clearly shows that the some properties of impure amorphous ices strongly depends on their defect structure in amorphous ices.
    4) On the basis of the above results, we have calculated the thermal history of comet nucleus. We found that runaway crystallization considered until now could not be occurred in the actual comet nucleus.
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (A), HOKKAIDO UNIVERSITY, 09304050
  • アモルファス氷星間塵上での水素分子生成機構
    Grants-in-Aid for Scientific Research Grant-in-Aid for Encouragement of Young Scientists (A)
    1997 - 1998
    渡部 直樹
    本研究の目的は、アモルファス氷星間塵上での水素分子生成機構の解明である。そのうち、期間内にアモルファス氷への紫外線照射による水素分子生成を定性的、かつ定量的に調べ、その生成メカニズムを明らかにした。具体的には以下の通りである。
    1. 紫外線照射による水素分子生成の確認:10K基板に蒸着法により生成されたアモルファス重水氷に126nm、172nmの紫外線を照射し、昇温脱離法により光反応生成物を分析した。その結果、重水素分子の生成が確認された。
    2. 重水素分子の生成メカニズム:生成量の波長依存性、光量依存性を調べたところ、重水素分子は、重水分子の第一電子励起状態を経由した、1光子過程の光反応により生成されることが強く示唆された。
    3. 重水素分子生成量の定量化:氷厚、紫外線照射時間を変えて生成量の変化を調べた。生成量は50〜150Åの範囲で膜厚に比例し、照射時間40分付近で飽和を始め、120分(星間空間10^6yに相当)で生成量は重水分子の数%になった。この照射時間の範囲では逆反応は観測されなかったことから、生成反応は氷固体内部よりも、むしろ氷内部の裂け目や孔の表面で起きているものと考えられる。以上のことから、紫外線による水素分子生成は星間空間で支配的とは言えないまでも無視できない過程であり、星間空間で観測された「氷内水素分子」の生成過程として有力な生成反応であることが分かった。
    Japan Society for the Promotion of Science, Grant-in-Aid for Encouragement of Young Scientists (A), Hokkaido University, 09740371
  • The development of a simulation device for the nucleation in the primordial solar nebula.
    Grants-in-Aid for Scientific Research
    1996 - 1998
    YAMAMOTO Tetsuo; ABE Tsutomu; WATANABE Naoki
    In order to investigate the mechanism of the nucleation of solid particles and its role in the evolution of the solar system materials, we have developed an experimental apparatus that simulates the non-equilibrium homogeneous nucleation from simple molecules to polymerized clusters. Condensable gas species are collimated in molecular beams and introduced into a high-vacuum chamber. A pulsed beam of the controlled environmental gas supplied from another vacuum port crosses the previous molecular beams. This method makes the necessary conditions of the cluster formation fulfilled in a localized area of the chamber and suffices the quantitative analysis of the nucleation and condensation. We have obtained the following results during this three-year grant-in-aid project
    (1) We have built a system that enables the cluster formation in a clean environment A vibration-free ultra-high vacuum system have been installed.
    (2) We have modified a gas effusion device for high vacuum and high temperature to truncate a mili-second small pulses out of the high-temperature gas mixture. The test of the device was satisfactory.
    (3) We have developed a TOF mass spectrometer for an in-situ analysis of the polymerized cluster that formed by multiple collisions.
    (4) In order to improve the emittance from the excimer laser device purchased with a Heisei 8 grant-in-aid, we have obtained a necessary local energy flux with a use of focal lens of high transmission.
    (5) Following the above developments, we have performed a laboratory experiment of the non-equilibrium homogeneous nucleation. We were able to observe clusters of low mass range, but polymerized clusters of high mass range were too small in abundance to be detected. A higher laser energy flux and a much larger mass flux of the condensable gas from the effusion device will be necessary to accomplish this task..
    Japan Society for the Promotion of Science, Grant-in-Aid for Scientific Research (A), HOKKAIDO UNIVERSITY, 08554016
  • 原子・イオン・分子の光電離過程の研究
    Competitive research funding
  • アモルファス氷表面上における原子・分子素過程
    Competitive research funding
  • Study on Atomic,ionic,and Molecular Photoionization processes
    Competitive research funding
  • Atomic and Molecular Processes on Amorphous ice surface
    Competitive research funding