惆惘 悋 拆悋惘 拆惠 愆悋 惡悋 悋悋惺 悋愕擧惘悋 慍惘 擧 惆惘 惶惺惠 悋愕惠悋惆 愆惆 悋惆 悛愆悋 愆惆 悛慍惆 擧 惠惘 愆悽惶悋惠 悛悋 愕惠
In this power point you'll learn laser scanners classifications and their use in industry.
惆惘 悋 拆悋惘拆惠 愆悋 惡悋 悋悋惺 惘愆 悋 悋惶 愕悴 悋悋惺 悋惶 悋惡 悋 悛愆悋 悽悋惆 愆惆
In this power point you'll learn how Laser distance meters work and what are different distance metering methods.
惆惘 悋 拆悋惘 拆惠 惡悋 悋悋惺 悋愕擧惘 慍惘 惆 愕 惡惺惆 悛愆悋 愆惆 惠擧 悋 惡擧悋惘 惘惠 惆惘 悛悋 惘悋 悛慍惆
In this power point, you'll learn how laser scanners work and which technologies they use.
First Seminar of Mine(Mining Industry) :Opportunities and Threats,Tehran,Iran,2010
Presented by : Aidin Salamzadeh
With special thanks to Alex Osterwalder(Swiss)
+98 912 425 47 29
The document discusses a Bianchi type IV viscous model of the early universe as part of a public lecture presented by Ikjyot Singh Kohli, an M.Sc. candidate at York University. It elaborates on the principles of general relativity, including the relationship between matter and spacetime curvature, and introduces Einstein's field equations. The document emphasizes the mathematical framework required to model early universe conditions and the implications of curvature in general relativity.
Dynamical Systems Methods in Early-Universe CosmologiesIkjyot Singh Kohli
油
The document discusses applying dynamical systems methods to develop models of the early universe. Specifically, it discusses:
1. Applying these methods to the Einstein field equations to obtain cosmological models that are spatially homogeneous but anisotropic.
2. Describing the process of analyzing the dynamics of these models, which involves identifying invariant sets, equilibrium points, monotone functions, and bifurcations in the parameter space.
3. The importance of numerical methods in understanding the global behavior of these systems, since analytical methods are often limited to local analysis near equilibrium points.
First Seminar of Mine(Mining Industry) :Opportunities and Threats,Tehran,Iran,2010
Presented by : Aidin Salamzadeh
With special thanks to Alex Osterwalder(Swiss)
+98 912 425 47 29
The document discusses a Bianchi type IV viscous model of the early universe as part of a public lecture presented by Ikjyot Singh Kohli, an M.Sc. candidate at York University. It elaborates on the principles of general relativity, including the relationship between matter and spacetime curvature, and introduces Einstein's field equations. The document emphasizes the mathematical framework required to model early universe conditions and the implications of curvature in general relativity.
Dynamical Systems Methods in Early-Universe CosmologiesIkjyot Singh Kohli
油
The document discusses applying dynamical systems methods to develop models of the early universe. Specifically, it discusses:
1. Applying these methods to the Einstein field equations to obtain cosmological models that are spatially homogeneous but anisotropic.
2. Describing the process of analyzing the dynamics of these models, which involves identifying invariant sets, equilibrium points, monotone functions, and bifurcations in the parameter space.
3. The importance of numerical methods in understanding the global behavior of these systems, since analytical methods are often limited to local analysis near equilibrium points.