May I continue or should I stop? the effects of regulatory focus and message framings on video game players’ self-control

Two types of motivations exist in terms of regulatory focus: a promotion orientation concerned with advancement and achievement and a prevention orientation concerned with safety and security. The central premise of this research is that promotion-focused and prevention-focused players differ in their sensitivity to message frames and therefore respond with different levels of self-control. This study adopted a 2 (message frames: positive vs. negative) × 2 (regulatory focus: promotion vs. prevention) between-subjects design; the results confirmed the hypotheses that, for promotion-focused players, negative messages are significantly effective in preventing them from becoming addicted to the games; meanwhile, for prevention-focused players, positive messages significantly influenced players, leading them to become addicted. Hence, video games’ negative and addiction-related messages should be enhanced whereas positive messages should be cautiously released.Regulatory focus, regulatory fit, message frames, self-control, video game

Buyer success and failure in bargaining and its consequences

This study aims to investigate the process of buyers’ subsequent attitudes and subsequent actions and their relationships depended on the bargaining outcomes. Depth interviews were employed in order to explore the success, the failure, and the consequent actions in dyadic bargaining under the condition of one buyer and one seller. Ten international respondents were invited to be interviewed. Approximately one hour of each interview is taken, while English is the medium of the interviews. After the interviews, respondents were given five USD as an incentive. The results show that successful bargainers tended to be younger people and easterner, compared to unsuccessful bargainers who tended to be older people and westerner. When buying product in computer and vehicle category, it might provide higher chance in getting the discount, while buying product in garment category gave the partial tendency to win the bargain. Since garment seems to have fewer profit margins when compared to the other category like computer or vehicle, it thus is obligatory for the seller to avoid discounting this kind of product. During the interviews, author found that confident interviewees shared their successful bargaining experiences; whereas, interviewees with very calm and quiet attitude seemed to express about their unsuccessful bargaining stories. This research also provides insights of buyer as bargainer profoundly. It therefore helps the seller, especially in computer, garment, and vehicle industry, knows how to balance mutual-interest and maintain the strong relationship with customer

May I continue or should I stop? the effects of regulatory focus and message framings on video game players’ self-control

Two types of motivations exist in terms of regulatory focus: a promotion orientation concerned with advancement and achievement and a prevention orientation concerned with safety and security. The central premise of this research is that promotion-focused and prevention-focused players differ in their sensitivity to message frames and therefore respond with different levels of self-control. This study adopted a 2 (message frames: positive vs. negative) × 2 (regulatory focus: promotion vs. prevention) between-subjects design; the results confirmed the hypotheses that, for promotion-focused players, negative messages are significantly effective in preventing them from becoming addicted to the games; meanwhile, for prevention-focused players, positive messages significantly influenced players, leading them to become addicted. Hence, video games’ negative and addiction-related messages should be enhanced whereas positive messages should be cautiously released

A novel mutation in the WFS1 gene identified in a Taiwanese family with low-frequency hearing impairment

<p>Abstract</p> <p>Background</p> <p>Wolfram syndrome gene 1 (<it>WFS1</it>) accounts for most of the familial nonsyndromic low-frequency sensorineural hearing loss (LFSNHL) which is characterized by sensorineural hearing losses equal to and below 2000 Hz. The current study aimed to contribute to our understanding of the molecular basis of LFSNHL in an affected Taiwanese family.</p> <p>Methods</p> <p>The Taiwanese family with LFSNHL was phenotypically characterized using audiologic examination and pedigree analysis. Genetic characterization was performed by direct sequencing of <it>WFS1 </it>and mutation analysis.</p> <p>Results</p> <p>Pure tone audiometry confirmed that the family members affected with LFSNHL had a bilateral sensorineural hearing loss equal to or below 2000 Hz. The hearing loss threshold of the affected members showed no progression, a characteristic that was consistent with a mutation in the <it>WFS1 </it>gene located in the DFNA6/14/38 locus. Pedigree analysis showed a hereditarily autosomal dominant pattern characterized by a full penetrance. Among several polymorphisms, a missense mutation Y669H (2005T>C) in exon 8 of <it>WFS1 </it>was identified in members of a Taiwanese family diagnosed with LFSNHL but not in any of the control subjects.</p> <p>Conclusion</p> <p>We discovered a novel heterozygous missense mutation in exon 8 of <it>WFS1 </it>(i.e., Y669H) which is likely responsible for the LFSNHL phenotype in this particular Taiwanese family.</p

Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies

We present the large-scale 3-point correlation function (3PCF) of the SDSS DR12 CMASS sample of $777,202$ Luminous Red Galaxies, the largest-ever sample used for a 3PCF or bispectrum measurement. We make the first high-significance ($4.5\sigma$) detection of Baryon Acoustic Oscillations (BAO) in the 3PCF. Using these acoustic features in the 3PCF as a standard ruler, we measure the distance to $z=0.57$ to $1.7\%$ precision (statistical plus systematic). We find $D_{\rm V}= 2024\pm29\;{\rm Mpc\;(stat)}\pm20\;{\rm Mpc\;(sys)}$ for our fiducial cosmology (consistent with Planck 2015) and bias model. This measurement extends the use of the BAO technique from the 2-point correlation function (2PCF) and power spectrum to the 3PCF and opens an avenue for deriving additional cosmological distance information from future large-scale structure redshift surveys such as DESI. Our measured distance scale from the 3PCF is fairly independent from that derived from the pre-reconstruction 2PCF and is equivalent to increasing the length of BOSS by roughly 10\%; reconstruction appears to lower the independence of the distance measurements. Fitting a model including tidal tensor bias yields a moderate significance ($2.6\sigma)$ detection of this bias with a value in agreement with the prediction from local Lagrangian biasing.Comment: 15 pages, 7 figures, submitted MNRA

Strong and broadly tunable plasmon resonances in thick films of aligned carbon nanotubes

Low-dimensional plasmonic materials can function as high quality terahertz and infrared antennas at deep subwavelength scales. Despite these antennas' strong coupling to electromagnetic fields, there is a pressing need to further strengthen their absorption. We address this problem by fabricating thick films of aligned, uniformly sized carbon nanotubes and showing that their plasmon resonances are strong, narrow, and broadly tunable. With thicknesses ranging from 25 to 250 nm, our films exhibit peak attenuation reaching 70%, quality factors reaching 9, and electrostatically tunable peak frequencies by a factor of 2.3x. Excellent nanotube alignment leads to the attenuation being 99% linearly polarized along the nanotube axis. Increasing the film thickness blueshifts the plasmon resonators down to peak wavelengths as low as 1.4 micrometers, promoting them to a new near-infrared regime in which they can both overlap the S11 nanotube exciton energy and access the technologically important infrared telecom band.Comment: 19 pages, 5 figures, main text followed by supporting informatio

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space

We perform a tomographic baryon acoustic oscillations analysis using the two-point galaxy correlation function measured from the combined sample of BOSS DR12, which covers the redshift range of $0.2<z<0.75$. Splitting the sample into multiple overlapping redshift slices to extract the redshift information of galaxy clustering, we obtain a measurement of $D_A(z)/r_d$ and $H(z)r_d$ at nine effective redshifts with the full covariance matrix calibrated using MultiDark-Patchy mock catalogues. Using the reconstructed galaxy catalogues, we obtain the precision of $1.3\%-2.2\%$ for $D_A(z)/r_d$ and $2.1\%-6.0\%$ for $H(z)r_d$. To quantify the gain from the tomographic information, we compare the constraints on the cosmological parameters using our 9-bin BAO measurements, the consensus 3-bin BAO and RSD measurements at three effective redshifts in \citet{Alam2016}, and the non-tomographic (1-bin) BAO measurement at a single effective redshift. Comparing the 9-bin with 1-bin constraint result, it can improve the dark energy Figure of Merit by a factor of 1.24 for the Chevallier-Polarski-Linder parametrisation for equation of state parameter $w_{\rm DE}$. The errors of $w_0$ and $w_a$ from 9-bin constraints are slightly improved when compared to the 3-bin constraint result.Comment: 14 pages, 21 figures, 7 Tables. Submitted to MNRA

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering

With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 $h^{-1}$Mpc). We analyze the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift $z=0.59$, to obtain constraints on the Hubble expansion rate $H(z)$, the angular-diameter distance $D_A(z)$, the normalized growth rate $f(z)\sigma_8(z)$, and the physical matter density $\Omega_mh^2$. We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g., ones induced by stars and seeing. We provide accurate measurements $\{D_A(0.59)r_{s,fid}/r_s$ $\rm Mpc$, $H(0.59)r_s/r_{s,fid}$ $km s^{-1} Mpc^{-1}$, $f(0.59)\sigma_8(0.59)$, $\Omega_m h^2\}$ = $\{1427\pm26$, $97.3\pm3.3$, $0.488 \pm 0.060$, $0.135\pm0.016\}$, where $r_s$ is the comoving sound horizon at the drag epoch and $r_{s,fid}=147.66$ Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g., cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e., CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, $w$, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, $\Omega_k$, is 0.3 per cent. We do not find deviation from flat $\Lambda$CDM.Comment: 15 pages, 11 figures. The latest version matches and the accepted version by MNRAS. A bug in the first version has been identified and fixed in the new version. We have redone the analysis with newest data (BOSS DR12