静-动加载相结合的材料状态方程实验平台的研制

舒桦; 涂昱淳; 王寯越; 贾果; 叶君建; 邓文; 束海云; 杨艳平; 杜雪艳; 谢志勇; 贺芝宇; 方智恒; 华能; 黄秀光; 裴文兵; 傅思祖

doi:10.7498/aps.67.20172502

摘要

根据神光-Ⅱ第九路高功率激光加载的特点，对传统静高压金刚石压砧装置进行了改进和优化设计，研制出了适合高功率激光加载条件下材料宽域状态方程研究的新型静高压靶.在神光-Ⅱ高功率激光装置上建立了基于静高压金刚石压砧和动高压激光相结合的材料宽域状态方程研究平台.利用这一平台开展了超纯水的宽域状态方程实验探索，获得了较好的实验结果.

关键词:

Materials can be experimentally characterized up to terapascal pressures by sending a laser-induced shock wave through a sample that is pre-compressed inside a diamond-anvil cell. Pre-compression expands the ability to control the initial condition, allowing access to thermodynamic states from the principal Hugoniot and enter into the 10 TPa to 100 TPa (0.1-1 Gbar) pressure range that is relevant to planetary science. We demonstrate here a laser-driven shock wave in a water sample that is pre-compressed in a diamond anvil cell. The compression factors of the dynamic and static techniques are multiplied. This approach allows access to a family of Hugoniot curves which span the P-T phase diagram of fluid water to high density. According to the loading characteristics of the SG-Ⅱ high-power laser, the traditional diamond anvil cell is improved and optimized, and a new diamond anvil cell target adapting to high power laser loading is developed. In order to adapt to laser shock, the diamond window should be thin (100 μm) enough so that the shock can propagate to the sample before the side rarefaction erodes too much the shock planarity. With a thickness of 100 mm over an aperture of 600 μm diameter, a pre-compressed water sample at 0.5 GPa can be obtained. The water is pre-compressed to 0.5 GPa by using the diamond anvil cell. Hugoniot curve is partially followed starting from pre-compression at a pressure of 0.5 GPa. Pressure, density, and temperature data for pre-compressed water are obtained in a pressure range from 150 GPa to 350 GPa by using the laser-driven shock compression technique. Our P-ρ-T data totally agree with the results from the model based on quantum molecular dynamics calculations. These facts indicate that this water model can be used as the standard for modeling interior structures of Neptune, Uranus, and exoplanets in the liquid phase in the multi-Mbar range and should improve our understanding of these types of planets.

Keywords:

作者及机构信息

1.
上海激光等离子体研究所, 上海 201800;

2.
北京高压科学研究中心, 北京 100094;

3.
中国科学院上海光学精密机械研究所, 上海 201800

通信作者: 舒桦, shuhua1979@163.com

基金项目: 科学挑战专题（批准号：TZ2016001）和国家重点研发计划（批准号：2017YFA0403200）资助的课题.

Authors and contacts

1.
Shanghai Institute of Laser Plasmas, Shanghai 201800, China;

2.
Center for High Pressure Science and Technology Advance Research, Beijing 100094, China;

3.
Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai 201800, China

Corresponding author: Shu Hua, shuhua1979@163.com

Funds: Project supported by the Science Challenge Project, China (Grant No. TZ2016001) and the National Key R&D Program of China (Grant No. 2017YFA0403200).

参考文献

[1]	Benuzzi A, Löwer T, Koenig M, Faral B, Batani D, Beretta D, Danson C, Pepler D 1996 Phys. Rev. E 54 2162
[2]	Batani D, Morelli A, Tomasini M, et al. 2002 Phys. Rev. Lett. 88 235502
[3]	Batani D, Strati F, Stabile H, et al. 2004 Phys. Rev. Lett. 92 065503
[4]	Boehly T R, Vianello E, Miller J E, Craxton R S, Collins T J B, Goncharov V N, Igumenshchev I V, Meyerhofer D D, Hicks D G, Celliers P M, Collins G W 2006 Phys. Plasmas 13 056303
[5]	Barrios M A, Hicks D G, Boehly T R, Fratanduono D E, Eggert J H, Celliers P M, Collins G W, Meyerhofer D D 2010 Phys. Plasmas 17 056307
[6]	Sano T, Ozaki N, Sakaiya T, Shigemori K, Ikoma M, Kimura T, Miyanishi K, Endo T, Shiroshita A, Takahashi H, Jitsui T, Hori Y, Hironaka Y, Iwamoto A, Kadono T, Nakai M, Okuchi T, Ohtani K, Shimizu K, Kondo T, Kodama R, Mima K 2011 Phys. Rev. B 83 054117
[7]	Jeanloz R, Celliers P M, Collins G W, Eggert J H, Lee K K M, McWilliams R S, Brygoo S, Loubeyre P 2007 Proc. Natl. Acad. Sci. USA 104 9172
[8]	Loubeyre P, Celliers P M, Hicks D G, Henry E, Dawaele A, Pasley J, Eggert J, Koenig M, Occelli F, Lee K K M, et al. 2004 High-Pressure Res. 24 25
[9]	Lee K K M, Benedetti L R, Jeanloz R, Celliers P M, Eggert J H, Hicks D G, Moon S J, Mackinnon A, Da Silva L B, Bradley D K, et al. 2006 J. Chem. Phys. 125 014701
[10]	Eggert J, Brygoo S, Loubeyre P, McWilliams R S, Celliers P M, Hicks D G, Boehly T R, Jeanloz R, Collins G W 2008 Phys. Rev. Lett. 100 124503
[11]	Celliers P M, Loubeyre P, Eggert J H, Brygoo S, McWilliams R S, Hicks D G, Boehly T R, Jeanloz R, Collins G W 2010 Phys. Rev. Lett. 104 184503
[12]	Loubeyre P, Brygoo S, Eggert J, Celliers P M, Spaulding D K, Rygg J R, Boehly T R, Collins G W, Jeanloz R 2012 Phys. Rev. B 86 144115
[13]	Kimura T, Ozaki N, Sano T, Okuchi T, Sano T, Shimizu K, Miyanishi K, Terai T, Kakeshita T, Sakawa Y, Kodama R 2015 J. Chem. Phys. 142 164504
[14]	Seagle C T, Reinhart W D, Lopez A J, Hickman R J, Thornhill T F 2016 J. Appl. Phys. 120 125902
[15]	Knudson M D, Desjarlais M P 2009 Phys. Rev. Lett. 103 225501
[16]	Hicks D G, Boehly T R, Celliers P M, Eggert J H, Vianello E, Meyerhofer D D, Collins G W 2005 Phys. Plasmas 12 082702
[17]	Mao H K, Bell P M, Shaner J W, Steinberg D J 1978 J. Appl. Phys. 49 3276
[18]	Deng X M, Liang X C, Chen Z 1986 Appl. Opt. 25 377
[19]	Fu S Z, Gu, Y, Wu J, Wang S J 1995 Phys. Plasmas 2 3461
[20]	Shu H, Huang X G, Ye J J, Jia G, Wu J, Fu S Z 2017 Laser Part. Beams 35 145
[21]	Shu H, Fu S Z, Huang X G, Ye J J, Zhou H Z, Xie Z Y, Long T 2012 Acta Phys. Sin. 61 114102 (in Chinese) [舒桦, 傅思祖, 黄秀光, 叶君建, 周华珍, 谢志勇, 龙滔 2012 物理学报 61 114102]
[22]	Celliers P M, Bradley D K, Collins G W, Hicks D G, Boehly T R, Armstrong W J 2004 Rev. Sci. Instrum. 75 4916
[23]	Shu H, Fu S Z, Huang X G, Wu J, Zhou H Z, Ye J J 2012 Meas. Sci. Technol. 23 015203
[24]	Miller J E, Boehly T R, Melchior A, Meyerhofer D D, Celliers P M, Eggert J H, Hicks D G, Sorce C M, Oertel J A, Emmel P M 2007 Rev. Sci. Instrum. 78 034903
[25]	French M, Mattsson T R, Nettelmann N, Redmer R 2009 Phys. Rev. B 79 054107

施引文献

[1]	Benuzzi A, Löwer T, Koenig M, Faral B, Batani D, Beretta D, Danson C, Pepler D 1996 Phys. Rev. E 54 2162
[2]	Batani D, Morelli A, Tomasini M, et al. 2002 Phys. Rev. Lett. 88 235502
[3]	Batani D, Strati F, Stabile H, et al. 2004 Phys. Rev. Lett. 92 065503
[4]	Boehly T R, Vianello E, Miller J E, Craxton R S, Collins T J B, Goncharov V N, Igumenshchev I V, Meyerhofer D D, Hicks D G, Celliers P M, Collins G W 2006 Phys. Plasmas 13 056303
[5]	Barrios M A, Hicks D G, Boehly T R, Fratanduono D E, Eggert J H, Celliers P M, Collins G W, Meyerhofer D D 2010 Phys. Plasmas 17 056307
[6]	Sano T, Ozaki N, Sakaiya T, Shigemori K, Ikoma M, Kimura T, Miyanishi K, Endo T, Shiroshita A, Takahashi H, Jitsui T, Hori Y, Hironaka Y, Iwamoto A, Kadono T, Nakai M, Okuchi T, Ohtani K, Shimizu K, Kondo T, Kodama R, Mima K 2011 Phys. Rev. B 83 054117
[7]	Jeanloz R, Celliers P M, Collins G W, Eggert J H, Lee K K M, McWilliams R S, Brygoo S, Loubeyre P 2007 Proc. Natl. Acad. Sci. USA 104 9172
[8]	Loubeyre P, Celliers P M, Hicks D G, Henry E, Dawaele A, Pasley J, Eggert J, Koenig M, Occelli F, Lee K K M, et al. 2004 High-Pressure Res. 24 25
[9]	Lee K K M, Benedetti L R, Jeanloz R, Celliers P M, Eggert J H, Hicks D G, Moon S J, Mackinnon A, Da Silva L B, Bradley D K, et al. 2006 J. Chem. Phys. 125 014701
[10]	Eggert J, Brygoo S, Loubeyre P, McWilliams R S, Celliers P M, Hicks D G, Boehly T R, Jeanloz R, Collins G W 2008 Phys. Rev. Lett. 100 124503
[11]	Celliers P M, Loubeyre P, Eggert J H, Brygoo S, McWilliams R S, Hicks D G, Boehly T R, Jeanloz R, Collins G W 2010 Phys. Rev. Lett. 104 184503
[12]	Loubeyre P, Brygoo S, Eggert J, Celliers P M, Spaulding D K, Rygg J R, Boehly T R, Collins G W, Jeanloz R 2012 Phys. Rev. B 86 144115
[13]	Kimura T, Ozaki N, Sano T, Okuchi T, Sano T, Shimizu K, Miyanishi K, Terai T, Kakeshita T, Sakawa Y, Kodama R 2015 J. Chem. Phys. 142 164504
[14]	Seagle C T, Reinhart W D, Lopez A J, Hickman R J, Thornhill T F 2016 J. Appl. Phys. 120 125902
[15]	Knudson M D, Desjarlais M P 2009 Phys. Rev. Lett. 103 225501
[16]	Hicks D G, Boehly T R, Celliers P M, Eggert J H, Vianello E, Meyerhofer D D, Collins G W 2005 Phys. Plasmas 12 082702
[17]	Mao H K, Bell P M, Shaner J W, Steinberg D J 1978 J. Appl. Phys. 49 3276
[18]	Deng X M, Liang X C, Chen Z 1986 Appl. Opt. 25 377
[19]	Fu S Z, Gu, Y, Wu J, Wang S J 1995 Phys. Plasmas 2 3461
[20]	Shu H, Huang X G, Ye J J, Jia G, Wu J, Fu S Z 2017 Laser Part. Beams 35 145
[21]	Shu H, Fu S Z, Huang X G, Ye J J, Zhou H Z, Xie Z Y, Long T 2012 Acta Phys. Sin. 61 114102 (in Chinese) [舒桦, 傅思祖, 黄秀光, 叶君建, 周华珍, 谢志勇, 龙滔 2012 物理学报 61 114102]
[22]	Celliers P M, Bradley D K, Collins G W, Hicks D G, Boehly T R, Armstrong W J 2004 Rev. Sci. Instrum. 75 4916
[23]	Shu H, Fu S Z, Huang X G, Wu J, Zhou H Z, Ye J J 2012 Meas. Sci. Technol. 23 015203
[24]	Miller J E, Boehly T R, Melchior A, Meyerhofer D D, Celliers P M, Eggert J H, Hicks D G, Sorce C M, Oertel J A, Emmel P M 2007 Rev. Sci. Instrum. 78 034903
[25]	French M, Mattsson T R, Nettelmann N, Redmer R 2009 Phys. Rev. B 79 054107

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