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書(shū)目名稱Gravity, a Geometrical Course影響因子(影響力)




書(shū)目名稱Gravity, a Geometrical Course影響因子(影響力)學(xué)科排名




書(shū)目名稱Gravity, a Geometrical Course網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Gravity, a Geometrical Course網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




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書(shū)目名稱Gravity, a Geometrical Course讀者反饋




書(shū)目名稱Gravity, a Geometrical Course讀者反饋學(xué)科排名

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的闡明

Nature in the Built Environmentnd Poincaré Lie algebras. The chapter ends with a conceptual criticism of Special Relativity, stressing its conflict with Newton’s Law. In this way the logical need to step forward to General Relativity is laid down.

周年紀(jì)念日

Modern Ideas of Nature and Environment,way gravitational waves should be produced by accelerated masses or lumps of energy. This chapter is devoted to discuss the emission of gravitational waves and the tests of General Relativity based on the slowing down of the period of double star systems.

窒息

https://doi.org/10.1007/978-1-349-27241-9s and emphasized the special status of Gravity within this general scheme. While recalling the historical development we have provided a, hopefully rigorous, exposition of all the mathematical foundations of gravity and gauge theories in a contemporary geometrical approach.

窒息

Gravitational Waves and the Binary Pulsars,way gravitational waves should be produced by accelerated masses or lumps of energy. This chapter is devoted to discuss the emission of gravitational waves and the tests of General Relativity based on the slowing down of the period of double star systems.

Predigest

forbid

https://doi.org/10.1007/978-81-322-2404-4This chapter addresses the issue of stellar equilibrium in General Relativity, derives the Tolman Oppenheimer Volkhoff equation and the corresponding mass limits. Next, considering the role of quantum mechanics the Chandrasekhar mass limits for white dwarfs and neutron stars are derived.

CANT

,Stellar Equilibrium: Newton’s Theory, General Relativity, Quantum Mechanics,This chapter addresses the issue of stellar equilibrium in General Relativity, derives the Tolman Oppenheimer Volkhoff equation and the corresponding mass limits. Next, considering the role of quantum mechanics the Chandrasekhar mass limits for white dwarfs and neutron stars are derived.