Titlebook: Beyond ΛCDM; Exploring Alternativ Sownak Bose Book 2018 Springer Nature Switzerland AG 2018 Dark Matter.Dark Energy.Modified Gravity.Steril

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書目名稱Beyond ΛCDM影響因子(影響力)




書目名稱Beyond ΛCDM影響因子(影響力)學(xué)科排名




書目名稱Beyond ΛCDM網(wǎng)絡(luò)公開度




書目名稱Beyond ΛCDM網(wǎng)絡(luò)公開度學(xué)科排名




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

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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

Exclude

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

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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.

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創(chuàng)造性

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

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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

BLINK

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.

ANTH

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.