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Nature, 2005 Scientific celebrity has a relativity all of its own. Some scientists are celebrated by their peers, some are treasured by their students, while others are lionized by the public at large. But very few are given the burden of being a celebrity to everyone, everywhere, all the time. Albert Einstein achieved that universality.
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Interdisciplinary Science Reviews, 1969
I have talked about Einstein many times before. That I speak once more on the same subject is due to the fact that in the leisure of my old age I have looked through the letters which Einstein wrote to me during his lifetime. There are more than fifty of them, short and long. I copied them all by hand to make doubly sure of their preservation, and this
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I have talked about Einstein many times before. That I speak once more on the same subject is due to the fact that in the leisure of my old age I have looked through the letters which Einstein wrote to me during his lifetime. There are more than fifty of them, short and long. I copied them all by hand to make doubly sure of their preservation, and this
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European Journal of Physics, 2005
Summary: This paper examines the challenges and rewards that can arise when the teaching of Einsteinian physics has to be accomplished by means of distance education. The discussion is mainly based on experiences gathered over the past 35 years at the UK Open University, where special and general relativity, relativistic cosmology and other aspects of ...
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Summary: This paper examines the challenges and rewards that can arise when the teaching of Einsteinian physics has to be accomplished by means of distance education. The discussion is mainly based on experiences gathered over the past 35 years at the UK Open University, where special and general relativity, relativistic cosmology and other aspects of ...
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Communication via one- and two-particle operators on Einstein-Podolsky-Rosen states.
Physical Review Letters, 1992Charles H. Bennett, S. Wiesner
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Quantum states with Einstein-Podolsky-Rosen correlations admitting a hidden-variable model.
Physical review. A, General physics, 1989R. Werner
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1996
In this chapter we discuss Einstein’s gravitational equations, which state that the presence of matter and energy creates curvature in spacetime, via $${G}_{jk} = 8\pi \kappa {T}_{jk},$$ (0.1) where Gjk = Ricjk − (1∕2)Sgjk is the Einstein tensor, Tjk is the stress-energy tensor due to the presence of matter, and κ is a positive constant. In 1
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In this chapter we discuss Einstein’s gravitational equations, which state that the presence of matter and energy creates curvature in spacetime, via $${G}_{jk} = 8\pi \kappa {T}_{jk},$$ (0.1) where Gjk = Ricjk − (1∕2)Sgjk is the Einstein tensor, Tjk is the stress-energy tensor due to the presence of matter, and κ is a positive constant. In 1
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Bose–Einstein condensation of exciton polaritons
Nature, 2006J. Kasprzak +13 more
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