日本地球惑星科学連合2015年大会

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口頭発表

セッション記号 S (固体地球科学) » S-VC 火山学

[S-VC46] 火山噴火のダイナミクスと素過程

2015年5月25日(月) 09:00 〜 10:45 304 (3F)

コンビーナ:*小園 誠史(東北大学大学院理学研究科地球物理学専攻)、鈴木 雄治郎(東京大学地震研究所)、奥村 聡(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、座長:奥村 聡(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)

10:36 〜 10:39

[SVC46-P06] 気泡核生成の大規模分子動力学計算と古典的核生成論の改良

ポスター講演3分口頭発表枠

*田中 今日子1田中 秀和1ディアマンド ユルグ2アンジェリル レイモンド2 (1.北海道大学低温科学研究所、2.チューリッヒ大学)

キーワード:気泡の核生成, 液相ー気相, 相変化, 分子動力学計算

Bubble nucleation in liquid is a liquid-to-vapor transition phenomenon and plays an important role in vulcanism. Studies of homogeneous liquid-vapour nucleation typically use the classical formula (CNT) for the bubble nucleation rate. However, the applicability of the CNT is not well understood.

Numerical techniques such as molecular dynamics and Monte-Carlo simulations are powerful methods to resolve details of the nucleation process and provide useful test cases for nucleation models. Typically, these simulations show large deviations from the CNT predictions. Most of the simulations for bubble nucleation in the literature use around 105 or fewer atoms, making it difficult to measure nucleation rates directly.

Recently, we presented large-scale, micro-canonical molecular dynamics simulations of homogeneous bubble nucleation with 5 * 108 Lennard-Jones atoms, and succeeded to directly measure nucleation rates in the range of 1021-25cm-3s-1 for argon by resolving bubble nucleation events in the steady state nucleation phase [1,2]. The unprecedented size of the simulated volumes allows us to resolve the nucleation and growth of many bubbles per run in simple direct micro-canonical (NVE) simulations while the ambient pressure and temperature remain almost perfectly constant.

We find bubble nucleation rates which are lower than in most of the previous, smaller simulations. It is widely believed that classical nucleation theory (CNT) generally underestimates bubble nucleation rates by very large factors. However, our measured rates are within two orders of magnitude of CNT predictions - only at very low temperatures the CNT underestimates the nucleation rate significantly.

We also derive an improved classical formula for the homogeneous bubble nucleation rate, where we revise the prefactor in the nucleation rate and compare it with the widely used classical nucleation theory (CNT) [3]. Our large-scale molecular dynamics simulations and laboratory experiments for argon bubble nucleation enable us to precisely test our theoretical models. The improved formula including the Tolman correction with a small positive Tolman length leads to good agreement with both MD simulations and laboratory experiments.

[1] J. Diemand, R. Angelil, K. K. Tanaka, and H. Tanaka, Pys. Rev E 90, 052407 (2014)
[2] R. Angelil, J. Diemand, K. K. Tanaka, and H. Tanaka, Pys. Rev E 90, 063301 (2014)
[3] K. K. Tanaka, H. Tanaka, R. Angelil, and J. Diemand, submitted