標(biāo)題: Titlebook: Elements ofCosmological Thermodynamics; Subhajit Saha Book 2018 The Author(s), under exclusive licence to Switzerland AG, part of Springer [打印本頁(yè)] 作者: BRISK 時(shí)間: 2025-3-21 18:12
書目名稱Elements ofCosmological Thermodynamics影響因子(影響力)
作者: 進(jìn)入 時(shí)間: 2025-3-21 21:21 作者: 消瘦 時(shí)間: 2025-3-22 00:55 作者: 小爭(zhēng)吵 時(shí)間: 2025-3-22 08:08 作者: Diastole 時(shí)間: 2025-3-22 09:08
2191-5423 y suggestions for further readingBased on the author’s own work and results obtained by renowned cosmologists, this short book provides a concise introduction to the relatively new research field of cosmological thermodynamics. Starting with a brief overview of basic cosmology and thermodynamics, th作者: 碳水化合物 時(shí)間: 2025-3-22 16:08 作者: 碳水化合物 時(shí)間: 2025-3-22 19:01
Experiencing the (Anomalous) Moment,d) constant equation of state, the validity of the first law, the generalized second law, and thermodynamic equilibrium have been tested. It is evident that our analysis may help to constrain various parameters of phenomenological particle creation models that have been considered in recent literature.作者: HAIRY 時(shí)間: 2025-3-22 22:53
Sensory Connections and Emotional Knowledgezon and obtained three equivalent expressions for it. Consequently, the Hawking temperature has been obtained. Finally, by employing the Bekenstein entropy and the generalized Hawking temperature at the horizon, we have undertaken a thermodynamic study of the model.作者: botany 時(shí)間: 2025-3-23 05:01 作者: Malaise 時(shí)間: 2025-3-23 07:08
Cosmological Thermodynamics in FLRW Model, horizon to determine its entropy variation. Moreover, we have assumed the modified Hawking temperature on the event horizon. Three types of dark energy cosmic fluids have been considered—a perfect fluid with a constant equation of state, an interacting holographic dark energy, and a Chaplygin gas.作者: 吸引力 時(shí)間: 2025-3-23 10:26 作者: 發(fā)酵劑 時(shí)間: 2025-3-23 15:04 作者: 掙扎 時(shí)間: 2025-3-23 19:08
https://doi.org/10.1007/978-1-4302-6593-1e Einstein’s equations, this chapter goes on to explain the relevant concepts of Cosmology required to gain the necessary insights into the subject of cosmological thermodynamics. It gives a brief, yet an effective description of the Friedmann–Lemaitre–Robertson–Walker metric, the observational para作者: 全能 時(shí)間: 2025-3-24 00:26
https://doi.org/10.1007/978-3-030-89446-7lization to Cosmology. The concepts of the generalized second law of thermodynamics, surface gravity and its connection with Hawking temperature, and Bekenstein entropy are carefully explained. Finally, the implications of the modified and the generalized Hawking temperatures are discussed with refe作者: patriot 時(shí)間: 2025-3-24 03:17 作者: 臭名昭著 時(shí)間: 2025-3-24 06:35 作者: 領(lǐng)帶 時(shí)間: 2025-3-24 12:47
Sensory Connections and Emotional Knowledgeinhomogeneous) perfect fluid for the purpose. Starting from the basic equations of the model, we have defined the surface gravity at an arbitrary horizon and obtained three equivalent expressions for it. Consequently, the Hawking temperature has been obtained. Finally, by employing the Bekenstein en作者: agglomerate 時(shí)間: 2025-3-24 16:30 作者: Coordinate 時(shí)間: 2025-3-24 19:35 作者: endarterectomy 時(shí)間: 2025-3-25 02:45 作者: Gastric 時(shí)間: 2025-3-25 06:05
https://doi.org/10.1057/9780230107915thermodynamics. These problems are quite intriguing and are far from being settled. Among them, the problem due to dynamic cosmological horizons is quite serious and as a result, many Cosmologists still remain sceptical about the thermodynamic formulation of our Universe based on cosmic horizons.作者: 易彎曲 時(shí)間: 2025-3-25 07:55
Cosmological Thermodynamics,lization to Cosmology. The concepts of the generalized second law of thermodynamics, surface gravity and its connection with Hawking temperature, and Bekenstein entropy are carefully explained. Finally, the implications of the modified and the generalized Hawking temperatures are discussed with reference to the cosmological event horizon.作者: 壓倒 時(shí)間: 2025-3-25 13:52 作者: chassis 時(shí)間: 2025-3-25 18:47
Michael Preston-Shoot,Dick AgassIn this chapter, the fundamentals of equilibrium thermodynamics are briefly examined. The basic terminology is followed by the discussion of the thermodynamic concepts of temperature, internal energy, entropy, absolute entropy, and enthalpy. Finally, the four laws of thermodynamics are explained in detail.作者: 木質(zhì) 時(shí)間: 2025-3-25 19:59 作者: 解脫 時(shí)間: 2025-3-26 02:01
Subhajit SahaProvides the first introductory text on this topic.Offers a lucid presentation with a minimum of jargon.Contains a rich bibliography and many suggestions for further reading作者: 和藹 時(shí)間: 2025-3-26 06:37
SpringerBriefs in Physicshttp://image.papertrans.cn/e/image/307580.jpg作者: 賞錢 時(shí)間: 2025-3-26 10:29
978-3-319-74705-7The Author(s), under exclusive licence to Switzerland AG, part of Springer Nature 2018作者: ureter 時(shí)間: 2025-3-26 14:48
Elements ofCosmological Thermodynamics978-3-319-74706-4Series ISSN 2191-5423 Series E-ISSN 2191-5431 作者: Melodrama 時(shí)間: 2025-3-26 20:20
Fundamentals of Relativistic Cosmology,e Einstein’s equations, this chapter goes on to explain the relevant concepts of Cosmology required to gain the necessary insights into the subject of cosmological thermodynamics. It gives a brief, yet an effective description of the Friedmann–Lemaitre–Robertson–Walker metric, the observational para作者: 表主動(dòng) 時(shí)間: 2025-3-26 23:46 作者: Incise 時(shí)間: 2025-3-27 02:45 作者: 結(jié)果 時(shí)間: 2025-3-27 09:11 作者: aphasia 時(shí)間: 2025-3-27 13:03 作者: Introvert 時(shí)間: 2025-3-27 15:06
Controversies and Open Issues in Cosmological Thermodynamics,thermodynamics. These problems are quite intriguing and are far from being settled. Among them, the problem due to dynamic cosmological horizons is quite serious and as a result, many Cosmologists still remain sceptical about the thermodynamic formulation of our Universe based on cosmic horizons.作者: MONY 時(shí)間: 2025-3-27 19:42
Bewertung umweltpolitischer Instrumente,s of the equations (differential and algebraic) and of the initial and/or boundary conditions. The automatic computations are performed under a present error-limit, which is controlled by maintaining the integration stepsize to be well within the radius of convergence. The automatic solution is show作者: 流出 時(shí)間: 2025-3-27 22:42
Bital Savir-Baruch,Bruce J. Barronin the School of Engineering and Applied Science, and several und- graduate mathematics or physics majors. After a ?rst draft of the manuscript was completed, it was also used for an independent re978-1-4419-2753-8978-0-387-85529-5Series ISSN 0072-5285 Series E-ISSN 2197-5612 作者: 水槽 時(shí)間: 2025-3-28 05:53
