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標(biāo)題: Titlebook: Beyond ΛCDM; Exploring Alternativ Sownak Bose Book 2018 Springer Nature Switzerland AG 2018 Dark Matter.Dark Energy.Modified Gravity.Steril [打印本頁]

作者: VER    時間: 2025-3-21 19:52
書目名稱Beyond ΛCDM影響因子(影響力)




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書目名稱Beyond ΛCDM網(wǎng)絡(luò)公開度




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書目名稱Beyond ΛCDM被引頻次




書目名稱Beyond ΛCDM被引頻次學(xué)科排名




書目名稱Beyond ΛCDM年度引用




書目名稱Beyond ΛCDM年度引用學(xué)科排名




書目名稱Beyond ΛCDM讀者反饋




書目名稱Beyond ΛCDM讀者反饋學(xué)科排名





作者: agnostic    時間: 2025-3-21 23:24

作者: defibrillator    時間: 2025-3-22 01:12
Substructure and Galaxy Formation in Warm Dark Matter Simulationset al. 2000, Bode et al. 2001, Viel et al. 2005, Knebe et al. 2008, Schneider et al. 2012, Lovell et al. 2012, Macció et al. 2013, Lovell et al. 2014, Reed et al. 2015, Colín et al. 2015, Yang et al. 2015, Bose et al. 2016, Horiuchi et al. 2016). In this chapter we use the . (.) high resolution .-bo
作者: Exclude    時間: 2025-3-22 04:38
Reionisation in Sterile Neutrino Cosmologiesicles are kinematically energetic at early times and thus free stream out of small-scale primordial perturbations, inducing a cut-off in the power spectrum of density fluctuations. On large scales unaffected by the free streaming cut-off, structure formation is very similar in CDM and sterile neutri
作者: 總    時間: 2025-3-22 11:40
Testing the Quasi-static Approximation in f(R) Gravity Simulations of the Universe. Einstein’s theory of General Relat6ivity (GR)has been the underlying gravity theory in the standard cosmological model of .CDM, the dark energy (.) and (cold) dark matter (CDM) components of which remain unresolved challenges to cosmologists.
作者: 有權(quán)    時間: 2025-3-22 16:27

作者: 創(chuàng)造性    時間: 2025-3-22 17:05
Conclusions and Future Workl is able to successfully fit and predict a vast range of phenomena in the Universe, such as the temperature fluctuations observed in the CMB, and the large-scale distribution of galaxies. The continuous development of sophisticated numerical and semi-analytic techniques have facilitated tests of th
作者: charisma    時間: 2025-3-22 22:05
2190-5053 ns.Confronts the predictions of theoretical models with obseThis book employs computer simulations of ‘a(chǎn)rtificial’ Universes to investigate the properties of two popular alternatives to the standard candidates for dark matter (DM) and dark energy (DE). It confronts the predictions of theoretical mod
作者: BLINK    時間: 2025-3-23 02:34
False-Name-Proofness in Social Networks Reed et al. 2015, Colín et al. 2015, Yang et al. 2015, Bose et al. 2016, Horiuchi et al. 2016). In this chapter we use the . (.) high resolution .-body simulation to investigate the properties of subhaloes in a WDM model.
作者: ANTH    時間: 2025-3-23 06:19
Substructure and Galaxy Formation in Warm Dark Matter Simulations Reed et al. 2015, Colín et al. 2015, Yang et al. 2015, Bose et al. 2016, Horiuchi et al. 2016). In this chapter we use the . (.) high resolution .-body simulation to investigate the properties of subhaloes in a WDM model.
作者: impale    時間: 2025-3-23 11:11

作者: Intercept    時間: 2025-3-23 14:55
Conclusions and Future Workis model on non-linear scales where, recently, hydrodynamical simulations within a .CDM context have managed to successfully reproduce a large set of observed galaxy properties at low redshift (e.g. Vogelsberger et al. 2014, Schaye et al. 2015).
作者: GRIN    時間: 2025-3-23 18:56
Future Internet — The Business Webamics of the cosmos, these theories suggest that the Universe contains only normal and dark matter (which is often assumed as cold dark matter, or CDM), but the law of gravitation deviates from that prescribed by Einstein’s General Relativity (GR) on large scales, resulting in an acceleration of the expansion rate.
作者: insolence    時間: 2025-3-23 23:06

作者: infarct    時間: 2025-3-24 02:20

作者: 調(diào)整    時間: 2025-3-24 08:30

作者: 異常    時間: 2025-3-24 12:21
Empirical Findings and Analysis Results,rent way in the two cases. No haloes form below a certain mass scale determined by the cut-off and the formation of small haloes above the cut-off is delayed (see Colín et al. 2000, Bode et al. 2001, Avila-Reese et al. 2001, Viel et al. 2005, Lovell et al. 2012, Schneider et al. 2012, Bose et al. 2016a, 2017).
作者: 極端的正確性    時間: 2025-3-24 16:31
Reionisation in Sterile Neutrino Cosmologiesrent way in the two cases. No haloes form below a certain mass scale determined by the cut-off and the formation of small haloes above the cut-off is delayed (see Colín et al. 2000, Bode et al. 2001, Avila-Reese et al. 2001, Viel et al. 2005, Lovell et al. 2012, Schneider et al. 2012, Bose et al. 2016a, 2017).
作者: Flawless    時間: 2025-3-24 19:04
Book 2018for dark matter (DM) and dark energy (DE). It confronts the predictions of theoretical models with observations using a sophisticated semi-analytic model of galaxy formation. Understanding the nature of dark matter (DM) and dark energy (DE) are two of the most central problems in modern cosmology. W
作者: dialect    時間: 2025-3-25 00:02
2190-5053 can placestrong constraints on the sterile neutrino scenario. In the second half, the authors propose and test novel numerical algorithms for simulating Universes with a ‘modified’ theory of gravity, as an alte978-3-030-07245-2978-3-319-96761-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
作者: 確定的事    時間: 2025-3-25 03:38
Book 2018re observations of the high redshift Universe and faint dwarf galaxies in the Local Group can placestrong constraints on the sterile neutrino scenario. In the second half, the authors propose and test novel numerical algorithms for simulating Universes with a ‘modified’ theory of gravity, as an alte
作者: overhaul    時間: 2025-3-25 09:09
Statistical Properties of Warm Dark Matter Haloesdecades, the model of non-relativistic dark matter consisting of heavy weakly-interacting particles with negligible thermal velocities at early times, the Cold Dark Matter (CDM) model, has become the cornerstone of the standard cosmological paradigm.
作者: Isolate    時間: 2025-3-25 15:06
Testing the Quasi-static Approximation in f(R) Gravity Simulations of the Universe. Einstein’s theory of General Relat6ivity (GR)has been the underlying gravity theory in the standard cosmological model of .CDM, the dark energy (.) and (cold) dark matter (CDM) components of which remain unresolved challenges to cosmologists.
作者: 密碼    時間: 2025-3-25 19:52
Beyond ΛCDM978-3-319-96761-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
作者: investigate    時間: 2025-3-25 23:59
Truthful Mechanisms for Exhibitionsdecades, the model of non-relativistic dark matter consisting of heavy weakly-interacting particles with negligible thermal velocities at early times, the Cold Dark Matter (CDM) model, has become the cornerstone of the standard cosmological paradigm.
作者: nerve-sparing    時間: 2025-3-26 01:12
https://doi.org/10.1007/978-3-642-21507-0 of the Universe. Einstein’s theory of General Relat6ivity (GR)has been the underlying gravity theory in the standard cosmological model of .CDM, the dark energy (.) and (cold) dark matter (CDM) components of which remain unresolved challenges to cosmologists.
作者: 條約    時間: 2025-3-26 06:27
https://doi.org/10.1007/978-3-319-96761-5Dark Matter; Dark Energy; Modified Gravity; Sterile Neutrinos; Cosmological Simulations; Structure Format
作者: Charitable    時間: 2025-3-26 09:06
978-3-030-07245-2Springer Nature Switzerland AG 2018
作者: Panacea    時間: 2025-3-26 15:15
https://doi.org/10.1007/978-3-540-92185-1ced back to the earliest annals of human history. Oft-repeated fundamental questions of cosmology such as “Why are we here?” or “How does the Universe work?” put an almost metaphysical spin on what has, over time, become a precision science. It is perhaps due to its dual nature – treading a fine lin
作者: 模仿    時間: 2025-3-26 17:10
Truthful Mechanisms for Exhibitionsdecades, the model of non-relativistic dark matter consisting of heavy weakly-interacting particles with negligible thermal velocities at early times, the Cold Dark Matter (CDM) model, has become the cornerstone of the standard cosmological paradigm.
作者: follicle    時間: 2025-3-26 23:25
False-Name-Proofness in Social Networkset al. 2000, Bode et al. 2001, Viel et al. 2005, Knebe et al. 2008, Schneider et al. 2012, Lovell et al. 2012, Macció et al. 2013, Lovell et al. 2014, Reed et al. 2015, Colín et al. 2015, Yang et al. 2015, Bose et al. 2016, Horiuchi et al. 2016). In this chapter we use the . (.) high resolution .-bo
作者: 王得到    時間: 2025-3-27 04:58
Empirical Findings and Analysis Results,icles are kinematically energetic at early times and thus free stream out of small-scale primordial perturbations, inducing a cut-off in the power spectrum of density fluctuations. On large scales unaffected by the free streaming cut-off, structure formation is very similar in CDM and sterile neutri
作者: chapel    時間: 2025-3-27 07:12
https://doi.org/10.1007/978-3-642-21507-0 of the Universe. Einstein’s theory of General Relat6ivity (GR)has been the underlying gravity theory in the standard cosmological model of .CDM, the dark energy (.) and (cold) dark matter (CDM) components of which remain unresolved challenges to cosmologists.
作者: 描繪    時間: 2025-3-27 12:51

作者: 揉雜    時間: 2025-3-27 17:06

作者: 錢財    時間: 2025-3-27 19:32
Sownak BoseNominated as an outstanding PhD thesis by the University of Durham, England.Employs state-of-the-art, high-resolution cosmological simulations.Confronts the predictions of theoretical models with obse
作者: 注意力集中    時間: 2025-3-27 22:06
Springer Theseshttp://image.papertrans.cn/b/image/185370.jpg




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