Effect of n?3 HUFA levels in rotifers and Artemia on growth and survival of larval black sea bream ( Sparus macrocephalus )

Requirement for dietary n−3 HUFA (n−3 highly unsaturated fatty acid) for growth and survival of black sea bream (Sparus macrocephalus) larvae was studied using rotifers andArtemia at various levels of n−3 HUFA. Five treatments with rotifers andArtemia differing in n−3 HUFA were prepared by enriching them with various oil emulsions. Results indicated that dietary n−3 HUFA significantly influence fish n−3 HUFA levels and are essential for growth and survival of black sea bream larvae. The results also indicated that the incorporation of n−3HUFA TG (triacylglycerols) into tissues of larval black sea bream was more effective from natural fish oil in comparison with n−3 HUFA fatty acid ethyl esters from ethyl-esterified oil. Project No. 39770588 supported by the NSFC.     

The genotoxic effects of benzo[a]pyrene and methamidophos on black porgy evaluated by comet assay

In this study, two common pollutants （benzo[a]pyrene and methamidophos） in marine environment were tested by comet assay for their inducement of in vivo genotoxic effect to the blood cells of black porgy （ Acanthopagrus schlegeli）. The fish was exposed to 2 μg/L of benzo[a]pyrene （BaP） and methamidophos, and their mixture. The assay was performed on whole blood at 2 h, 5 h, 24 h and 96 h exposure intervals. A significant increase in DNA damage was observed in each treatment with the pollutants. Additive effect of BaP and methamidophos was also found in the experiment. However, the decrease ratios of DNA damage for 5 h and 96 h exposure interals compared with 2 h and 24 h exposure ones, respectively, were noticed. This phenomenon may be explained by the function of repairing process via enzyme cytochrome P450 in the animal. Evidence of the genotoxicity of organophosphorus pesticides （OPs） and polynuclear aromatic hydrocarbons （PAHs） on marine fish are discussed in this paper.     

浙江建德市耕地表层土壤硒分布、来源及生态效应

硒是重要的生命元素之一,对动物及人体健康具有重要意义。系统总结了建德市耕地表层土壤硒地球化学特征,分析了土壤硒的分布规律及其与黑色岩系之间的成因联系,探讨了黑色岩系富硒机制,研究了水稻植株中硒富集规律。结果表明,建德市耕地表层土壤硒含量介于0.06~11.5 mg/kg之间,均值为0.35 mg/kg,不同地质背景、成土母质、土壤类型中土壤硒含量差异显著。根据土壤硒和重金属含量,圈出清洁富硒土壤2 647 hm²,主要分布于寒武系灰岩、碳质页岩、钙质泥岩等岩石出露区,指示土壤富硒与这套寒武系“黑色岩系”有密切关系。古沉积学研究认为,黑色岩系形成于缺氧滞水的沉积环境,富含有机质的海底沉积物大量吸附来自地幔的硒,成岩后形成富含硒等元素的黑色岩系。水稻根系土中硒形态组成分析表明,醋酸溶解态硒占比较小,残渣态占比较大,说明水稻根系土中硒可利用性较低。稻米、莲子、草莓及其根系土采样分析表明,稻米对土壤硒的富集系数最高,水稻植株中硒含量具有根>叶>茎≈籽实的特征。     

EGUP与黑洞熵的修正值

目前,人们对黑洞Bekenstein-Hawking熵的量子修正值产生了极大的兴趣,尤其是黑洞熵对数修正项的系数.在广义不确定关系(GUP)的基础上,通过引入了推广的广义不确定关系(EGUP),运用面积定理计算了3类时空的黑洞熵的修正值,得到的黑洞熵的修正项的系数是正的.这种计算方法不仅对单视界时空适用,而且对有内视界的黑洞时空依然成立,并且在EGUP基础上计算出黑洞熵的修正值.相比GUP基础上得到的黑洞熵,EGUP可以应用于大尺度时空下,所以应用范围更广.此计算方法简洁明了,物理意义明确,可为黑洞熵对数修正值系数的确定提供参考.     

Refractory Black Carbon Results and a Method Comparison between Solid-state Cutting and Continuous Melting Sampling of a West Antarctic Snow and Firn Core

This work presents the refractory black carbon(rBC)results of a snow and firn core drilled in West Antarctica(79°55'34.6"S,94°21'13.3"W)during the 2014?15 austral summer,collected by Brazilian researchers as part of the First Brazilian West Antarctic Ice Sheet Traverse.The core was drilled to a depth of 20 m,and we present the results of the first 8 m by comparing two subsampling methods—solid-state cutting and continuous melting—both with discrete sampling.The core was analyzed at the Department of Geological Sciences,Central Washington University(CWU),WA,USA,using a single particle soot photometer(SP2)coupled to a CETAC Marin-5 nebulizer.The continuous melting system was recently assembled at CWU and these are its first results.We also present experimental results regarding SP2 reproducibility,indicating that sample concentration has a greater influence than the analysis time on the reproducibility for low rBC concentrations,like those found in the Antarctic core.Dating was carried out using mainly the rBC variation and sulfur,sodium and strontium as secondary parameters,giving the core 17 years(1998?2014).The data show a well-defined seasonality of rBC concentrations for these first meters,with geometric mean summer/fall concentrations of 0.016μg L^?1 and geometric mean winter/spring concentrations of 0.063μg L^?1.The annual rBC concentration geometric mean was 0.029μg L^?1(the lowest of all rBC cores in Antarctica referenced in this work),while the annual rBC flux was 6.1μg m^?2 yr^?1(the lowest flux in West Antarctica records so far).     

GRB 130427A/SN 2013cq与伽玛射线暴-超新星成协

从1998年4月初步确认GRB 980425/SN 1998bw成协,至2013年9月确认GRB130831A/SN 2013fu成协,共有11对伽玛暴与超新星成协事件通过光谱学方法得到确认。对伽玛暴-超新星成协的详细研究大大深化了人们对伽玛暴与Ic型超新星的认识,并推进了人们对大质量恒星演化、死亡以及爆发机制的研究:对它们的多波段余辉的性质以及超新星光谱的观测与分析间接地揭示出伽玛暴-超新星中心引擎的性质。这些事件中,GRB 130427A/SN 2013cq具有特殊的重要性:它是近距离宇宙中唯一的高能、高亮度的伽玛暴,它的GeV辐射挑战了当前的伽玛暴辐射机制,伴随它的明亮光学闪提供了爆炸本性的有用线索,伴随它的SN 2013cq是伽玛暴成协的超新星中动能最大的超新星之一,对伴随它的中微子探测的零结果也对伽玛暴的瞬时辐射模型给出了有用的限制。总结了GRB 130427A/SN 2013cq的重要观测结果,这对于探索伽玛暴-超新星成协的本质及伽玛暴瞬时辐射和余辉的细节性质有非常重要的研究价值。     

A simple way to classify supermassive black holes

We propose a classification of supermassive black holes (SMBHs) based on their efficiency in the conversion of infalling mass in emitted radiation. We use a theoretical model that assumes a conservation of angular momentum between the gas falling inside the hole and the photons emitted outwards, and suggests the existence of the scaling relation M_•‐R_eσ³, where M_• is the mass of the central SMBH, whereas R_e and σ are the effective radius and velocity dispersion of the host galaxies (bulges), respectively. We apply our model on a data set of 57 galaxies of different morphological types and with M_• measurements, obtained through the analysis of Spitzer /IRAC 3.6‐µ m images. In order to find the best fit of the corresponding scaling law, we use the FITEXY routine to perform a least‐squares regression of M_• on R_eσ³ for the considered sample of galaxies. Our analysis shows that the relation is tight and our theoretical model allows to easily estimate the efficiency of mass conversion into radiation of the central SMBHs. Finally we propose a new appealing way to classify the SMBHs in terms of this parameter. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

A Fundamental Plane of Black Hole Activity: Pushing Forward the Unification Scheme

We examine the disc-jet connection in stellar mass and supermassive black holes by investigating the properties of their compact emission in the hard X-ray and radio bands. We compile a sample of ∼100 active galactic nuclei with measured mass, 5 GHz core emission, and 2–10 keV luminosity, together with eight galactic black holes with a total of ∼50 simultaneous observations in the radio and X-ray bands. Using this sample, we study the correlations between the radio (L_R) and the X-ray (L_X) luminosity and the black hole mass (M). We find that the radio luminosity is correlated with both M and L_X, at a highly significant level. We show how this result can be used to extend the standard unification by orientation scheme to encompass unification by mass and accretion rate.