期刊文献+
共找到3篇文章
< 1 >
每页显示 20 50 100
Prediction of low-cycle crack initiation life of powder superalloy FGH96 with inclusions based on damage mechanics 被引量:3
1
作者 Yuan-ming XU Shu-ming ZHANG +2 位作者 Tian-peng HE Xin-ling LIU Xia-yuan CHANG 《Transactions of Nonferrous Metals Society of China》 SCIE EI CAS CSCD 2022年第3期895-907,共13页
The effects of inclusions in powder superalloy FGH96 on low-cycle fatigue life were studied, and a low-cycle crack initiation life prediction model based on the theory of damage mechanics was proposed. The damage char... The effects of inclusions in powder superalloy FGH96 on low-cycle fatigue life were studied, and a low-cycle crack initiation life prediction model based on the theory of damage mechanics was proposed. The damage characterization parameter was proposed after the construction of damage evolution equations. Fatigue tests of the powder superalloy specimens with and without inclusion were conducted at 530 and 600 ℃, and the model verification was carried out for specimens with elliptical, semi-elliptical, polygon and strip-shaped surface/subsurface inclusion. The stress analysis was performed by finite element simulation and the predicted life was calculated. The results showed a satisfying agreement between predicted and experimental life. 展开更多
关键词 powder superalloy FGH96 low-cycle fatigue INCLUSION crack initiation life prediction damage mechanics
下载PDF
The naked planet Earth:Most essential pre-requisite for the origin and evolution of life 被引量:10
2
作者 S.Maruyama M.Ikoma +3 位作者 H.Genda K.Hirose T.Yokoyama M.Santosh 《Geoscience Frontiers》 SCIE CAS CSCD 2013年第2期141-165,共25页
Our blue planet Earth has long been regarded to carry full of nutrients for hosting life since the birth of the planet.Here we speculate the processes that led to the birth of early life on Earth and its aftermath, fi... Our blue planet Earth has long been regarded to carry full of nutrients for hosting life since the birth of the planet.Here we speculate the processes that led to the birth of early life on Earth and its aftermath, finally leading to the evolution of metazoans.We evaluate:(1) the source of nutrients,(2) the chemistry of primordial ocean,(3) the initial mass of ocean,and(4) the size of planet.Among the life-building nutrients,phosphorus and potassium play a key role.Only three types of rocks can serve as an adequate source of nutrients:(a) continent-forming TTG(granite),enabling the evolution of primitive life to metazoans;(b) primordial continents carrying anorthosite with KREEP(Potassium,Rare Earth Elements, and Phosphorus) basalts,which is a key to bear life;(c) carbonatite magma,enriched in radiogenic elements such as U and Th,which can cause mutation to speed up evolution and promote the birth of new species in continental rift settings.The second important factor is ocean chemistry.The primordial ocean was extremely acidic(pH = 1-2) and enriched in halogens(CI,F and others),S,N and metallic elements(Cd,Cu,Zn,and others),inhibiting the birth of life.Plate tectonics cleaned up these elements which interfered with RNA.Blue ocean finally appeared in the Phanerozoic with pH = 7 through extensive interaction with surface continental crust by weathering,erosion and transportation into ocean.The initial ocean mass was also important.The birth of life and aftermath of evolution was possible in the habitable zone with 3-5 km deep ocean which was able to supply sufficient nutrients. Without a huge landmass,nutrients cannot be supplied into the ocean only by ridge-hydrothermal circulation in the Hadean.Finally,the size of the planet plays a crucial role.Cooling of massive planets is less efficient than smaller ones,so that return-flow of seawater into mantle does not occur until central stars finish their main sequence.Due to the suitable size of Earth,the dawn of Phanerozoic witnessed the initiation of return-flow of seawater into the mantle,leading to the emergence of huge landmass above sea-level,and the distribution of nutrients on a global scale.Oxygen pump also played a critical role to keep high-PO_2 in atmosphere since then,leading to the emergence of ozone layer and enabling animals and plants to invade the land. To satisfy the tight conditions to make the Earth habitable,the formation mechanism of primordial Earth is an important factor.At first,a 'dry Earth' must be made through giant impact,followed by magma ocean to float nutrient-enriched primordial continents(anorthosite + KREEP).Late bombardment from asteroid belt supplied water to make 3-5 km thick ocean,and not from icy meteorites from Kuiper belt beyond cool Jupiter.It was essential to meet the above conditions that enabled the Earth as a habitable planet with evolved life forms.The tight constraints that we evaluate for birth and evolution of life on Earth would provide important guidelines for planetary scientists hunting for life in the exosolar planets. 展开更多
关键词 Earth life Habitable planet initial ocean mass Metazoan Nutrients
下载PDF
Method for Predicting Crack Initiation Life of Notched Specimen Based on Damage Mechanics 被引量:3
3
作者 LIU Jianhui WEI Yaobing +1 位作者 YAN Changfeng LANG Shanshan 《Journal of Shanghai Jiaotong university(Science)》 EI 2018年第2期286-290,共5页
Based on the theory of damage mechanics, a method for fatigue crack initiation life prediction of notched components is proposed in this paper. The damage evolution equation of notched specimen under tensioncompressio... Based on the theory of damage mechanics, a method for fatigue crack initiation life prediction of notched components is proposed in this paper. The damage evolution equation of notched specimen under tensioncompression loading is obtained in term of closed-form solution. The crack initiation life of notched specimen is estimated by the proposed method even when material and stress concentration factor are different. It has been verified that the result calculated by the proposed method agrees with the experimental result. The proposed method is concise, effective and feasible to practical application. 展开更多
关键词 crack initiation life notch specimen damage mechanics
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部