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Low cycle fatigue behavior of zirconium−titanium−steel composite plate 被引量:1
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作者 Bin-bin ZHOU Peng YU +3 位作者 Le CHANG Chang-yu ZHOU Cheng YE bo-jun zhang 《Transactions of Nonferrous Metals Society of China》 SCIE EI CAS CSCD 2022年第5期1530-1547,共18页
The low cycle fatigue behavior of zirconium−titanium−steel composite plate under symmetrical and asymmetric stress control was studied.The effects of mean stress and stress amplitude on cyclic deformation,ratcheting e... The low cycle fatigue behavior of zirconium−titanium−steel composite plate under symmetrical and asymmetric stress control was studied.The effects of mean stress and stress amplitude on cyclic deformation,ratcheting effect and damage mechanism were discussed in detail.The results show that under symmetric stress control,the forward ratcheting deformation is observed.Under asymmetric stress control,the ratcheting strain increases rapidly with mean stress and stress amplitude increasing.Under high stress amplitude,the influence of mean stress is more significant.In addition,by studying the variation of strain energy density,it is found that the stress amplitude mainly promotes the fatigue damage,while the mean stress leads to the ratcheting damage.In addition,fractographic observation shows that the crack initiates in the brittle metal compound at the interface,and the steel has higher resistance to crack propagation.Finally,the accuracy of life prediction model considering ratcheting effect is discussed in detail,and a high-precision life prediction model directly based on mean stress and stress amplitude is proposed. 展开更多
关键词 zirconium−titanium−steel composite plate low cycle fatigue behavior fatigue damage mean stress ratcheting effect life prediction model
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Neutron star mass-radius relation with gravitational field shielding by a scalar field
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作者 bo-jun zhang Tian-Xi zhang +1 位作者 Padmaja Guggilla Mostafa Dokhanian 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2013年第5期571-578,共8页
The currently well-developed models for equations of state (EoSs) have been severely impacted by recent measurements of neutron stars with a small radius and/or large mass. To explain these measurements, the theory ... The currently well-developed models for equations of state (EoSs) have been severely impacted by recent measurements of neutron stars with a small radius and/or large mass. To explain these measurements, the theory of gravitational field shielding by a scalar field is applied. This theory was recently developed in accor- dance with the five-dimensional (5D) fully covariant Kaluza-Klein (KK) theory that has successfully unified Einstein's general relativity and Maxwell's electromagnetic theory. It is shown that a massive, compact neutron star can generate a strong scalar field, which can significantly shield or reduce its gravitational field, thus making it more massive and more compact. The mass-radius relation developed under this type of modified gravity can be consistent with these recent measurements of neutron stars. In addition, the effect of gravitational field shielding helps explain why the supernova explosions of some very massive stars (e.g.9 40 MQ as measured recently) actually formed neutron stars rather than black holes as expected. The EoS models, ruled out by measurements of small radius and/or large mass neutron stars according to the the- ory of general relativity, can still work well in terms of the 5D fully covariant KK theory with a scalar field. 展开更多
关键词 stars: neutron -- gravitation -- black hole physics -- equation of state
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