rd Planck 2014 - Ferrara, 3 December 2014 ⌦ e 1+z e ⌘ 1/a e Using Pettorino etal 2013 Planck constraints on holographic dark energy. Observations have long shown that only a small fraction of The largest fluctuations are the result of the total energy content of the Universe—dark energy, dark matter, ordinary matter, light, and anything else. The Planck scale was invented as a set of universal units, so it was a shock when those limits also turned out to be the limits where the known laws of physics applied. “As our data keeps getting better and better, we will subject this standard model to increasingly stringent tests,” says Ariel Sanchez. Xaq Rzetelny - Feb 11, 2015 2:35 pm UTC no informa tion los s as compared to a full analysis, while. We study the impact of Early Dark Energy (EDE) cosmologies, where the Dark Energy contribution is non-vanishing at early times, on the SZ cluster sample expected by the upcoming Planck mission. Planck results: First stars were born later than we thought Also constrains inflation, dark energy in the early Universe, and more. This is because Planck data appear to favor a higher matter density and lower Hubble constant, in tension with most of the other current cosmological data sets. "The dark energy hypothesis is holding up very well, but this is not the end of the story." On the Law of Distribution of Energy in the Normal Spectrum. the Planck data as well as dark energy and SUSY breaking. Planck, who was a colleague of Wien's when he was carrying out this work, later, in 1900, based quantum theory on the fact that Wien's law, while valid at high frequencies, broke down completely at low frequencies. News. If you want to check the reckoning Planck density is c^7/hbar G^2 A day is 1603E45 planck time. So Hubble time 14E9 years is 8.19 E60 planck time We constrain plausible dark energy models using the recently published cosmic microwave background (CMB) temperature anisotropy data from Planck together with WMAP9 low-ℓ polarization data and the data from low redshift surveys. Abstract. Conversely, dark energy, a mysterious force thought to be responsible for accelerating the expansion of the Universe, accounts for less than previously thought. Although the observational evidence for dark energy implies a component which is unclustered in space as well as slowly-varying in … Since structures grow slower in the presence of EDE, one expects an enhancement of the number of galaxy clusters compared to CDM at intermediate and high redshifts, which could explain the reported excess Toggle navigation emion.io. OSTI.GOV Journal Article: Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data Recent preprints; astro-ph; cond-mat; cs; econ; eess; gr-qc; hep-ex; hep-lat; hep-ph; hep-th In this paper we use the 2015 data release from Planck1 (Planck Collaboration I 2016) to perform a system-atic analysis of a large set of dark energy and modiﬁed gravity theories. Therefore, it will be very hard to produce it in accelerators. We develop four-parameter supergravity models of inflation and dark energy, constrained so that δ ρ ρ $$\\frac{\\delta \\rho }{\\rho }$$ , n s and the cosmological constant Λ take their known observable values, but where the mass of gravitino m 3/2 and the tensor-to-scalar ratio r are free parameters. Jun-Qing Xia (Beijing, Inst. However, adding Planck distance priors does not lead to significantly improved dark energy constraints using current data, compared to adding WMAP9 distance priors. Dynamical dark energy. As it is not found in galaxies or clusters of galaxies, the The bounds from Planck + WP (from last year Planck parameter paper) were: Omega_ede < 0.010 at 95% CL. Or thereabouts---allowing for some variation in the percentages people cite. What's more, the new Planck catalog of images now has more than 1,500 clusters of galaxies observed throughout the universe, the largest catalog of this type ever made. ⌦ e(z e ⇠ 50) . For this research, we study the implications of Planck data for models of dark energy (DE) and modified gravity (MG) beyond the standard cosmological constant scenario. being muc h faster. The Planck consortium has made their final data release, including new processing of the cosmic microwave background temperature and polarisation data. And (dark energy + dark matter + usual matter) is (1.17 + 0.53 + 0.07)E-123 planck. graphic dark energy (HDE) model by using the Planck data. Moreover, these models have nice properties with regard to initial conditions for inﬂation, analogous to the ones studied in [27] for models without SUSY breaking and dark energy. For example, a distance smaller than the Planck length just doesn’t make sense—the physics breaks down. arXiv:1305.5302v3 [astro-ph.CO] 1 Oct 2013 Planck Constraints on Holographic Dark Energy Miao Li,1,2,3, ∗ Xiao-Dong Li,4, † Yin-Zhe Ma,5,6, ‡ Xin Zhang,7,8, § and Zhenhui Zhang1,2,3, ¶ 1Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China 2Kavli Institute for Theoretical Physics China, Chinese Academy of Sciences, Beijing 100190, China Max Planck. Dark energy is the dominant component in the Universe, yet there are currently no compelling explanations for its existence or its distribution. the derivation of the Planck spectrum. Finally, the Planck data also set a new value for the rate at which the Universe is expanding today, known as the Hubble constant. Planck Collaboration Peacock & Dodds, 1994 . Much like dark matter which explained the “missing mass,” it then became necessary to find this elusive energy, or at least provide a coherent theoretical framework for it. However, KIPAC scientists, along with many others in the astrophysics and cosmology community, are generating a suite of techniques and observational tools that will greatly enhance our understanding of this enigmatic phenomenon. We perform a detailed investigation on the cosmologicalconstraints on the holographic dark energy (HDE) model by usingthe Plank data. We make a comparison for ten typical, popular dark energy models according to their capabilities of fitting the current observational data. (a) The present dark energy fraction Ω Λ vs. Ω m, assuming a "CMB" is Planck+WP, "BAO" is the combination of SDSS-II, BOSS, and 6dFGS, and "SN" is Union2. Dark matter and dark energy may be weird and (as of now) inexplicable, but they do seem to exist, the final data release from Europe's Planck satellite mission suggests. Dark energy is a diffuse, very weakly interacting with matter and very low energy phenomenon. energy is quantized. Dark Energy Constraints after Planck. 2.2. Planck Collaboration: Planck 2015 results. Published 18 September 2013 • Journal of Cosmology and Astroparticle Physics, Volume 2013, September 2013 We find that HDE can provide a good fit tothe Plank high-ℓ (ℓ 40) temperature powerspectrum, while the discrepancy at ℓ 20-40 found in theΛCDM model remains unsolved in the HDE model. Dark energy is even more mysterious, and its discovery in the 1990s was a complete shock to scientists. We nd that HDE can provide a good t to the Planck high-‘(‘& 40) temperature power spectrum, while the discrep-ancy at ‘’20 40 found in the CDM model remains unsolved in the HDE model. 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