Monte-Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters

We consider non-gravitational heating effects on galaxy clusters on the basis of the Monte-Carlo modeling of merging trees of dark matter halos combined with the thermal evolution of gas inside each halo. Under the assumption of hydrostatic equilibrium and the isothermal gas profiles, our model takes account of the metallicity evolution, metallicity-dependent cooling of gas, supernova energy feedback, and heating due to jets of radio galaxies in a consistent manner. The observed properties of galaxy clusters can be explained in models with higher non-gravitational heating efficiency than that in the conventional model. Possibilities include jet heating by the Fanaroff-Riley Type II radio galaxies, and the enhanced star formation efficiency and/or supernova energy feedback, especially at high redshifts.Comment: 29 pages, 12 figures. To appear in PASJ, February 25, 200

Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation

We examine the reliability of the merger trees generated for the Monte-Carlo modeling of galaxy formation. In particular we focus on the cold gas fraction predicted from the merger trees with different assumptions on the progenitor distribution function, the timestep, and the mass resolution. We show that the cold gas fraction is sensitive to the accuracy of the merger trees at small-mass scales of progenitors at high redshifts. One can reproduce the Press-Schechter prediction to a reasonable degree by adopting a fairly large number of redshift bins, N_{step} ~ 1000 in generating merger trees, which is a factor of ten larger than the canonical value used in previous literature.Comment: 9 pages, 10 figures. To appear in PASJ, October 25, 200

"Measuring the Cost of Imperfect Information in the Tokyo Housing Market"

The cost of imperfect information is estimated in the real estate market of resale condominiums in central Tokyo by using a new, comprehensive data set of resale condominium transactions. The results suggest a substantial cost. Specifically, if information were perfectly available and marketing time is null, sellers would get benefits of 10.58% based on average interest rate, 31.28% on gross rent and 22.59% on net rent, against imputed rent of their property. Buyers spend 1,042,000 Yen on search activities for one transaction, which would be saved if information were prefect. This cost amounts to be equivalent to 13.2% of buyers' average annual income.

Statistical ensembles for phase coexistence states specified by noncommutative additive observables

Coexisting phases in a phase coexistence state cannot be distinguished by thermodynamic forces, such as temperature and chemical potential, because the forces take the same values over all coexisting phases. Therefore, to investigate a phase coexistence state, it is necessary to employ an ensemble in which all additive observables that distinguish the coexisting phases have macroscopically definite values. Although the microcanonical ensemble is conventionally employed as such an ensemble, it becomes ill-defined when some of the additive observables do not commute with each other, and a new ensemble has been craved. We propose a novel class of ensembles such that the additive observables, which are generally noncommutative, always have macroscopically definite values even in a first-order phase transition region. Using these ensembles, we propose a concrete method to construct phase coexistence states of general quantum systems. Furthermore, these ensembles are convenient for practical calculations because of good analytic properties. To demonstrate that our formulation successfully gives phase coexistence states of quantum systems, we apply it to a two-dimensional system whose coexisting phases are distinguished by an additive observable (order parameter) that does not commute with the Hamiltonian. To the author's best knowledge, this is the first work that obtains phase coexistence states separated by phase interfaces at finite temperature in such a quantum system