1,046 research outputs found

    Cosmology with x-matter

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    Motivated by the possibility of H0t0>1H_0t_0 > 1 where H0H_0 and t0t_0 are the Hubble parameter and the age of the universe, respectively, we investigate the cosmology including x-matter. x-matter is expressed by the equation of state px=w0ρx0+cs2(ρxρx0)p_x=w_0\rho_{x0} + c_s^2(\rho_x-\rho_{x0}), where pxp_x, ρx\rho_x and ρx0\rho_{x0} are the pressure, the density of x-matter and the density at present, respectively. w0w_0 and cs2c_s^2 are functions of ρx\rho_x in general. x-matter has the most general form of the equation of state which is characterized by 1)violation of strong energy condition at present for w0<1/3w_0 < -1/3 ; 2) locally stable (i.e. cs20c_s^2\geq 0); 3)causality is guaranteed (cs1c_s\leq 1). Considering the case that w0w_0 and cs2c_s^2 are constants, we find that there is a large parameter space of (w0,cs2,Ωx0)(w_0,c_s^2,\Omega_{x0}) in which the model universe is consistent with the age of the universe and the observations of distant Type I supernovae.Comment: minor changes, 4 pages, 6 figures, accepted for publication as a Letter in MNRA

    Observational tests of x-matter models

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    We study gravitational lensing statistics, matter power spectra and the angular power spectra of the cosmic microwave background (CMB) radiation in x-matter models. We adopt an equation-of-state of x-matter which can express a wide range of matter from the pressureless dust to the cosmological constant. A new ingredient in this model is the sound speed of the x-component in addition to the equation-of-state w0=px0/ρx0w_0=p_{x0}/\rho_{x0}. Except for the cosmological constant case, the perturbations of x-matter itself are considered. Our primary interest is in the effect of non-zero sound speed on the structure formation and the CMB spectra. It is found that there exist parameter ranges where x-matter models are consistent with all current observations. The x-matter generally leaves imprints in the CMB anisotropy and the matter power spectrum, which should be detectable in future observations.Comment: minor changes, 10 pages+14 figures, MNRAS in pres

    Microwave Background Anisotropies in Primeval Isocurvature Baryon Models: Constraints on the Cosmological Parameters

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    We have performed the most comprehensive predictions of the temperature fluctuations \dtt in the primeval isocurvature baryon models to see whether or not the models are consistent with the recent data on the cosmic microwave background anisotropies. More specifically, we computed the \dtt corresponding to the experimental set-up by the South-Pole and the Owens Valley experiments as well as the COBE satellite. The amplitudes of the predicted \dtt are normalized by means of the COBE 10^\circ data. The resulting constraints on the models are presented on nΩbn - \Omega_b plane in the case of λ0=1Ωb\lambda_0=1-\Omega_b (flat models) and λ0=0\lambda_0=0 (open models), where nn is the primordial spectral index of entropy fluctuations and Ωb\Omega_b is the present baryon density parameter. Our results imply that the PIB models cannot be reconciled with the current observations for any reasonable set of cosmological parameters.Comment: 10pages and 4figures compressed uuencoded postscript (with figures), UTAP-93-16

    Diffusion behavior of delta-doped Si in InAlAs/InP heterostructures

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    Diffusion behavior of delta-doped Si in InAlAs and InP was studied by using secondary ion mass spectroscopy. A significant broadening of the profile due to postgrowth annealing was observed in In0.52Al0.48As. In contrast, the depth profile of delta-doped Si in InP was scarcely changed by annealing. This indicates that the diffusion coefficient of delta-doped Si in InP is much smaller than that in In0.52Al0.48As. Suppression of Si diffusion by using a delta-doped InP layer as the carrier supply layer (CSL) improves the thermal stability of the InP-HEMT structures

    Development and Social Implementation of Smartphone App Nige-Tore for Improving Tsunami Evacuation Drills: Synergistic Effects Between Commitment and Contingency

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    This research explored how we can improve tsunami evacuation behavior, which has been a major social issue since the 2011 Great East Japan Earthquake and Tsunami. We introduce Nige-Tore, a smartphone app for supporting tsunami evacuation drills, which was developed within an interdisciplinary research framework. Nige-Tore serves as an effective interface tool that successfully visualizes the dynamic interactions between human actions (evacuation behavior) and natural phenomena (tsunami behavior). Drill participants can check, on their smartphone, the estimated inundation area of the approaching tsunami, along with their own current evacuation trajectory. The results of real-world trials using Nige-Tore show that the app is more powerful than conventional devices and methods that have been used in tsunami evacuation training, such as hazard maps and traditional drills that do not make use of any apps, because Nige-Tore provides an interface that enables commitment and contingency thinking—which at first glance appear to represent different orientations—to not only coexist but to synergize. “Commitment” (devotion or involvement) refers to the act of immersing oneself in and viewing as absolute one particular scenario or its potential to be actualized, given conditions in which infinite scenarios may be actualized, depending on the interactions between human systems and natural systems. “Contingency” thinking (an accidental or incidental state) refers to the act of relativizing and separating oneself from any particular scenario or its potential to be actualized, given the same conditions. The synergistic effect of “commitment” and “contingency” thinking also expands people’s capacity to cope with unexpected and unforeseen events
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