• Title/Summary/Keyword: IGM's theory

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A Study on Skin Friction Estimation of Drilled Shaft Socketed in Weathered Granite by IGM's Theory (화강풍화암에 근입된 현장타설말뚝의 주면마찰력 산정에 대한 IGM 이론의 적용)

  • Hong, Soon Taek;Lee, Jong In;Shin, Young Wan;Lee, Seung Ho
    • KSCE Journal of Civil and Environmental Engineering Research
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    • v.31 no.6C
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    • pp.241-250
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    • 2011
  • The design method of IGM proposed by FHWA to predict bearing capacities of drilled shaft socketed in weathered granite has been used generally. In this study, site investigations were performed in a pilot test site, and disturbance and roughness were measured. Geotechnical properties were assorted as cohesive material and undisturbed and smooth surface. A simple relationship was proposed to predict unconfined strength ($q_u$) of weathered granite using static load test results, load transfer test results and N values. It was confirmed that the design method to estimate bearing capacities of drilled shaft could improve IGM's theory for weathered granite from this research.

The Analysis of Shaft Deformation for Evaluating the Bearing Capacity of IGM Sosketed Drilled Shaft (IGM에 근입된 말뚝의 지지력 해석을 위한 기준침하량 결정방법 제안)

  • Chun, Byung-Sik;Kim, Won-Cheul;Seo, Deok-Dong
    • Journal of the Korean GEO-environmental Society
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    • v.5 no.3
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    • pp.17-30
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    • 2004
  • In this study, a new formula of settlement at the head of IGM was suggested and the applicability of suggested formula was verified with field test results. This suggested formula was the function of the settlement at the shaft head and the elastic compression of shaft. The applicability of suggested formula was verified with the result of in-situ load test. Also, the bearing capacity of drilled shaft with the IGM's theory was compared with those of classical theories. The results showed that classical method showed smaller values of bearing capacity than those of field load test data. The results of analysis also showed that the suggested formula and IGM's theory were applicable for the estimation of bearing capacity with the increase of shaft settlement. Especially, settlement correction factor($k_m$), which reflects ground condition and load transfer characteristics, increases as the applying load and shaft deformation increase. This suggested formula was applicable for medium density or higher density of soil condition and $k_m=1$ means yielding load for firm soil condition.

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Applicability Evaluation of IGM시s Theory Using the Results of Load Transfer Tests of Drilled Shafts (현장타설말뚝의 하중전이시험 결과를 이용한 IGM 이론의 적용성 평가)

  • 천병식;김원철;서덕동;윤우현
    • Journal of the Korean Geotechnical Society
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    • v.20 no.6
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    • pp.29-40
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    • 2004
  • The bearing capacity of drilled shaft is affected by several factors, such as shaft length, shape, surface roughness, young's modulus of geomaterials and shaft, soil strength, confining stress and so on. However, there has been no design method of drilled shaft considering all factors mentioned above. Moreover, since geomaterials are simply classified as sand, clay and rock, there was no design criterion for IGM (Intermediate Geomaterials). Therefore, the rigorous design approach of drilled shaft was not possible by classical design method. However, since these characteristics were not considered in classical theories, bearing capacity was generally different ken practical value. In this study, the bearing capacity of drilled shaft with the IGM's theory was compared with those of classical theories. The results showed that classical method showed smaller values of bearing capacity than those of field load transfer data. Moreover, the evaluated value of bearing capacity with IGM theory corresponded fairly well with those of field data.

INTERGALACTIC MEDIUM IN THE ACDM UNIVERSE FROM COSMOLOGICAL SIMULATIONS

  • FENG LONG-LONG;HE PING;FANG LIZHI;SHU CHI-WANG;ZHANG MENG-PING
    • Journal of The Korean Astronomical Society
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    • v.38 no.2
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    • pp.129-133
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    • 2005
  • The temperature (T) and entropy (S) fields of baryonic gas, or intergalactic medium (IGM), in the ACDM cosmology are analyzed using simulation samples produced by a hybrid cosmological hydrodynamic/N-body code based on the weighted essentially non-oscillatory scheme. We demonstrate that, in the nonlinear regime, the dynamical similarity between the IGM and dark matter will be broken in the presence of strong shocks in the IGM. The heating and entropy production by the shocks breaks the IGM into multiple phases. The multiphase and non-Gaussianity of the IGM field would be helpful to account for the high-temperature and high-entropy gas observed in groups and clusters with low-temperature IGM observed by Ly$\alpha$ forest lines and the intermittency observed by the spikes of quasi-stellar object's absorption spectrum.