Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the S8S_8 tension remains present

The baryonic feedback effect is considered as a possible solution to the so-called $S_8$ tension indicated in cosmic shear cosmology. The baryonic effect is more significant on smaller scales, and affects the cosmic shear two-point correlation functions (2PCFs) with different scale- and redshift-dependencies from those of the cosmological parameters. In this paper, we use the Hyper Suprime-Cam Year 3 (HSC-Y3) data to measure the cosmic shear 2PCFs ($\xi_{\pm}$) down to 0.28 arcminutes, taking full advantage of the high number density of source galaxies in the deep HSC data, to explore a possible signature of the baryonic effect. While the published HSC analysis used the cosmic shear 2PCFs on angular scales, which are sensitive to the matter power spectrum at $k\lesssim 1~h{\rm Mpc}^{-1}$, the smaller scale HSC cosmic shear signal allows us to probe the signature of matter power spectrum up to $k\simeq 20~h{\rm Mpc}^{-1}$. Using the accurate emulator of the nonlinear matter power spectrum, DarkEmulator2, we show that the dark matter-only model can provide an acceptable fit to the HSC-Y3 2PCFs down to the smallest scales. In other words, we do not find any clear signature of the baryonic effects or do not find a systematic shift in the $S_8$ value with the inclusion of the smaller-scale information as would be expected if the baryonic effect is significant. Alternatively, we use a flexible 6-parameter model of the baryonic effects, which can lead to both enhancement and suppression in the matter power spectrum compared to the dark matter-only model, to perform the parameter inference of the HSC-Y3 2PCFs. We find that the small-scale HSC data allow only a fractional suppression of up to 5 percent in the matter power spectrum at $k\sim 1~h{\rm Mpc}^{-1}$, which is not sufficient to reconcile the $S_8$ tension.Comment: 30 pages, 16 figure

Change in specific interactions between lactose repressor protein and DNA induced by ligand binding: molecular dynamics and molecular orbital calculations

<div><p>Lactose repressor protein (LacR) plays an essential role in controlling the transcription mechanism of genomic information from DNA to mRNA. It has been elucidated that a ligand binding to LacR regulates allosterically the specific interactions between LacR and operator DNA. However, the effect of the ligand binding on the specific interactions has not been clarified at an atomic level. In this study, we performed classical molecular dynamics (MD) and <i>ab initio</i> fragment molecular orbital simulations to elucidate the effect of ligand binding at atomic and electronic levels. The MD simulations for the solvated complexes with LacR-dimer, DNA and ligand demonstrate that the binding of an inducer IPTG to LacR-dimer significantly changes the structure of LacR-monomer to cause strong interactions between LacR-monomers, resulting in weakening the interactions between LacR-dimer and DNA. In contrast, the binding of an anti-inducer ONPF to LacR-dimer was found to enhance the interactions between LacR-dimer and DNA. These findings are consistent with the functions of IPTG and ONPF as an inducer and an anti-inducer, respectively. We therefore proposed a simplified model for the effect of the ligand binding on the specific interactions between LacR-dimer and DNA.</p></div

Novel excitations near quantum criticality in geometrically frustrated antiferromagnet CsFeCl3

The investigation of materials that exhibit quantum phase transition provides valuable insights into fundamental problems in physics. We present neutron scattering under pressure in a triangular-lattice antiferromagnet that has a quantum disorder in the low-pressure phase and a noncollinear structure in the high-pressure phase. The neutron spectrum continuously evolves through critical pressure; a single mode in the disordered state becomes soft with the pressure and it splits into gapless and gapped modes in the ordered phase. Extended spin-wave theory reveals that the longitudinal and transverse fluctuations of spins are hybridized in the modes because of noncollinearity, and previously unidentified magnetic excitations are formed. We report a new hybridization of the phase and amplitude fluctuations of the order parameter near a quantum critical point in a spontaneously symmetry-broken state.ISSN:2375-254

Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B

We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight