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We intend to understand cosmological structure formation within the framework of superfluid models of dark matter with finite temperatures. Of particular interest is the evolution of small-scale structures where the pressure and superfluid…

宇宙学与河外天体物理 · 物理学 2020-10-28 S. T. H. Hartman , H. A. Winther , D. F. Mota

We calculate the bispectrum of the gravitational field fluctuations generated during warm inflation, where dissipation of the vacuum potential during inflation is the mechanism for structure formation. The bispectrum is non--zero because of…

天体物理学 · 物理学 2011-05-10 S. Gupta , A. Berera , A. F. Heavens , S. Matarrese

We study the cosmic microwave background (CMB) anisotropy due to spherically symmetric nonlinear structures in flat universes with dust and a cosmological constant. By modeling a time-evolving spherical compensated void/lump by…

天体物理学 · 物理学 2009-02-20 Nobuyuki Sakai , Kaiki Taro Inoue

We begin by enumerating the many processes in gravitation and cosmology where quantum noise and fluctuations play an active role such as particle creation, galaxy formation and entropy generation. Using the influence functional we first…

天体物理学 · 物理学 2007-05-23 Bei-lok Hu , Andrew Matacz

The dynamics of a quantum system with internal degrees of freedom undergoing spontaneous collapse in the position basis are analysed; e.g., neutral mesons or neutrinos. Surprisingly, the value of the Heaviside function $\theta(x)$ at $x=0$…

量子物理 · 物理学 2016-02-18 K. Simonov , B. C. Hiesmayr

The extragalactic background radiation produced by distant galaxies emitting in the far infrared limits the sensitivity of telescopes operating in this range due to confusion. We have constructed a model of the infrared background based on…

宇宙学与河外天体物理 · 物理学 2017-10-19 S. V. Pilipenko , M. V. Tkachev , A. A. Ermash , T. I. Larchenkova , E. V. Mikheeva , V. N. Lukash

Wave function collapse models are considered as the modified theories of standard quantum mechanics at the macroscopic level. By introducing nonlinear stochastic terms in the Schr\"odinger equation, these models make predictions,…

量子物理 · 物理学 2017-02-02 Jing Zhang , Tiancai Zhang , Jie Li

The collapse of an inclined cohesive granular layer triggered by a certain perturbation can be a model for not only landslides on Earth but also relaxations of asteroidal surface terrains. To understand such terrain dynamics, we conduct a…

软凝聚态物质 · 物理学 2018-08-16 S. Takizawa , H. Niiya , T. Tanabe , H. Nishimori , H. Katsuragi

This work presents a self-heating study of a 40-nm bulk-CMOS technology in the ambient temperature range from 300 K down to 4.2 K. A custom test chip was designed and fabricated for measuring both the temperature rise in the MOSFET channel…

应用物理 · 物理学 2021-06-16 P. A. 't Hart , M. Babaie , A. Vladimirescu , F. Sebastiano

We use a simple model to investigate the effect of polarized Galactic foreground emission on the ability of planned CMB missions to detect and model CMB polarization. Emission from likely polarized sources (synchrotron and spinning dust)…

天体物理学 · 物理学 2007-05-23 A. Kogut , G. Hinshaw

Under the assumption that the concordance Lambda cold dark matter (CDM) model is the correct model, we test the cosmic microwave background (CMB) anisotropy data for systematic effects by examining the band pass temperature residuals with…

天体物理学 · 物理学 2007-05-23 Louise M. Griffiths , Charles H. Lineweaver

Hot intergalactic gas in clusters, groups, and filaments emanates a continuous background of 0.5-2.0 keV X-rays that ought to be detectable with the new generation of X-ray observatories. Here we present selected results from a program to…

天体物理学 · 物理学 2009-11-06 G. Mark Voit , Greg L. Bryan

Detection of millikelvin-level signals from the 'Cosmic Dawn' requires an unprecedented level of sensitivity and systematic calibration. We report the theory behind a novel calibration algorithm developed from the formalism introduced by…

天体物理仪器与方法 · 物理学 2022-09-15 I. L. V. Roque , W. J. Handley , N. Razavi-Ghods

Analyses of the cosmic microwave background (CMB) radiation maps made by the Wilkinson Microwave Anisotropy Probe (WMAP) have revealed anomalies not predicted by the standard inflationary cosmology. In particular, the power of the…

地球与行星天体物理 · 物理学 2014-11-20 V. Dikarev , O. Preuss , S. Solanki , H. Krueger , A. Krivov

We present numerical simulations of reduced magnetohydrodynamic (RMHD) turbulence in a magnetic flux tube at the center of a polar coronal hole. The model for the background atmosphere is a solution of the momentum equation, and includes…

太阳与恒星天体物理 · 物理学 2016-04-27 A. A. van Ballegooijen , M. Asgari-Targhi

One of the longstanding issues in numerical relativity is to enable a simulation taking account of microphysical processes (e.g., weak interactions and neutrino cooling). We develop an approximate and explicit scheme in the fully general…

高能天体物理现象 · 物理学 2010-12-09 Yuichiro Sekiguchi

A brief review is given of the Continuous Spontaneous Localization (CSL) model in which a classical field interacts with quantized particles to cause dynamical wavefunction collapse. One of the model's predictions is that particles…

量子物理 · 物理学 2007-05-23 Philip Pearle , James Ring , Juan I. Collar , Frank T. Avignone

The CONUS experiment is searching for coherent elastic neutrino nucleus scattering of reactor anti-neutrinos with four low energy threshold point-contact high-purity germanium spectrometers. An excellent background suppression within the…

Even the most sensitive cosmic microwave background anisotropy experiments have signal to noise ratios <=5, so that an accurate determination of the properties of the cosmological signal requires a careful assessment of the experimental…

天体物理学 · 物理学 2009-10-30 C. M. Gutierrez

We discuss gamma-ray bursts that have very hard spectra, consistent with black-body radiation, throughout their duration. We find that the temperature decay during a pulse can be well described by a broken power-law in time, with an…

天体物理学 · 物理学 2009-11-10 Felix Ryde