Comment on "The Jones-Hore theory of radical-ion-pair reactions is not self-consistent" (arXiv:1010.3888v3)

A short comment on "The Jones-Hore theory of radical-ion-pair reactions is not self-consistent" (arXiv:1010.3888v3) is presented. In the comment, it is pointed out that the paper includes a misconception about the Jones-Hore approach in Chem. Phys. Lett. 488 (2010) 90-93. The re-formulation is presented and it is demonstrated that the Jones-Hore theory is consistent at least on the point claimed by I. K. Kominis in the paper

Overcoming velvet bean seed dormancy by "dry heat"

Avaliou-se a germinação de sementes recém-colhidas de mucuna preta (Mucuna aterrima) após tratamento com "calor seco", em estufa elétrica com ventilação forçada, nas temperaturas de 35, 45 e 55°C, por períodos de exposição correspondentes a 0, 2, 4, 6, 8,16,24, 48, 72 e 96 horas. A temperatura de 55°C foi adequada para a superação da impermeabilidade do tegumento da semente, sendo mais efetivos os períodos de exposição entre 16 e 24 horas.The germination of freshly harvested velvet bean (Mucuna aterrima) seeds was evaluated after "dry heat" treatments under 35, 45 and 55°C, during periods of 0, 2, 4, 6, 8, 16, 24, 48, 72 and 96 hours. The temperature of 55°C was satisfactory to overcome the impermeability of the seed coat, and the exposing periods between 16 and 24 hours were the most effective

Determinant-Gravity: Cosmological implications

We analyze the action $\int d^4x \sqrt{\det||{\cal B} g_{\mu\nu}+ {\cal C} R_{\mu\nu}}||$ as a possible alternative or addition to the Einstein gravity. Choosing a particular form of ${\cal B}(R)= \sqrt {R}$ we can restore the Einstein gravity and, if ${\cal B}=m^2$, we obtain the cosmological constant term. Taking ${\cal B} = m^2 + {\cal B}_1 R$ and expanding the action in $1/m^2$, we obtain as a leading term the Einstein Lagrangian with a cosmological constant proportional to $m^4$ and a series of higher order operators. In general case of non-vanishing ${\cal B}$ and ${\cal C}$ new cosmological solutions for the Robertson-Walker metric are obtained.Comment: revtex format, 5 pages,8 figures,references adde

Detection and prevention of financial abuse against elders

This article is made available through the Brunel Open Access Publishing Fund. Copyright @ The Authors. This article is published under the Creative Commons Attribution (CC BY 3.0) licence. Anyone may reproduce, distribute, translate and create derivative works of this article (for both commercial and non-commercial purposes), subject to full attribution to the original publication and authors. The full terms of this licence may be seen at http://creativecommons.org/licences/ by/3.0/legalcode.Purpose – This paper reports on banking and finance professionals' decision making in the context of elder financial abuse. The aim was to identify the case features that influence when abuse is identified and when action is taken. Design/methodology/approach – Banking and finance professionals (n=70) were shown 35 financial abuse case scenarios and were asked to judge how certain they were that the older person was being abused and the likelihood of taking action. Findings – Three case features significantly influenced certainty of financial abuse: the nature of the financial problem presented, the older person's level of mental capacity and who was in charge of the client's money. In cases where the older person was more confused and forgetful, there was increased suspicion that financial abuse was taking place. Finance professionals were less certain that financial abuse was occurring if the older person was in charge of his or her own finances. Originality/value – The research findings have been used to develop freely available online training resources to promote professionals' decision making capacity (www.elderfinancialabuse.co.uk). The resources have been advocated for use by Building Societies Association as well as CIFAS, the UK's Fraud Prevention Service.The research reported here was funded by the UK cross council New Dynamicsof Ageing Programme, ESRC Reference No. RES-352-25-0026, with Mary L.M. Gilhooly asPrincipal Investigator. Web-based training tools, developed from the research findings, weresubsequently funded by the ESRC follow-on fund ES/J001155/1 with Priscilla A. Harries asPrincipal Investigator

Variação dos componentes da produção de dois cultivares de soja, UFV-1 e IAC-7, em função da época de semeadura

A study was made on early, normal and delayed planting dates on the seed yield and its components of two late varieties of soybean, UFV-1 and IAC-7. The field experiment was carried out at Campinas Experimental Station in eutrophic Latossolo Roxo during the years 1979/80 and 1980/81. In the first year planting were made every twenty days starting from October 5 and in the second year every thirty days starting from September 17, the total being eight and seven in the consecutive years. The parameters studied were: seed yield, nodes/ /plant, podes/plant and seed weight. The planting dates affected the seed yield and its components in both varieties. The number of nodes and pods/plant were more affected than the seed weight. Each variety had the same behavior with regard to the number of nodes and pods/plant and the same cannot be said to seed weight. In the first year the seed weight was not affected by the planting date and in the second, late plantings decreased the values of this parameter. The variability of yield components was more effective for highest yields planting dates. Number of nodes and pods/plant exercised a greater influence on the seed yield than the seed weight.Estudaram-se os efeitos de épocas de semeadura antecipadas, normais e retardadas, na produção e em seus componentes, em dois cultivares de soja, UFV-1 e IAC-7. O trabalho foi desenvolvido em condições de campo, no município de Campinas, SP, em um Latossolo Roxo eutrófico, durante os anos agrícolas de 1979/ /80 e 1980/81. No primeiro ano, as semeaduras foram efetuadas a cada 20 dias, à partir de 5/10 e no segundo ano, mensais à partir de 17/09, sendo consideradas oito e sete épocas respectivamente à cada ano. Foram determinadas as seguintes características: produção de sementes, número de nós por planta, número de vagens por planta e peso de 100 sementes. A época de semeadura influenciou a produção e seus componentes, nos dois cultivares. Dos componentes avaliados o número de nós e o número de vagens por planta foram mais afetados do que o peso da semente. Cada cultivar apresentou o mesmo tipo de comportamento quanto ao número de nós e de vagens por planta, não ocorrendo o mesmo com o peso da semente, que no primeiro ano não foi afetado pela época de semeadura e no segundo, diminuiu de valor com o atraso na semeadura. As variações nos componentes da produção são mais acentuadas nas épocas de maior produção. O número de nós e de vagens por planta são características de maior determinação na produção de sementes

Normal-state conductivity in underdoped La_{2-x}Sr_xCuO_4 thin films: Search for nonlinear effects related to collective stripe motion

We report a detailed study of the electric-field dependence of the normal-state conductivity in La_{2-x}Sr_xCuO_4 thin films for two concentrations of doped holes, x=0.01 and 0.06, where formation of diagonal and vertical charged stripes was recently suggested. In order to elucidate whether high electric fields are capable of depinning the charged stripes and inducing their collective motion, we have measured current-voltage characteristics for various orientations of the electric field with respect to the crystallographic axes. However, even for the highest possible fields (~1000 V/cm for x=0.01 and \~300 V/cm for x=0.06) we observed no non-linear-conductivity features except for those related to the conventional Joule heating of the films. Our analysis indicates that Joule heating, rather than collective electron motion, may also be responsible for the non-linear conductivity observed in some other 2D transition-metal oxides as well. We discuss that a possible reason why moderate electric fields fail to induce a collective stripe motion in layered oxides is that fairly flexible and compressible charged stripes can adjust themselves to the crystal lattice and individual impurities, which makes their pinning much stronger than in the case of conventional rigid charge-density waves.Comment: 10 pages, 10 figures, accepted for publication in Phys. Rev.

Interplanetary and Geomagnetic Consequences of Interacting CMEs of 13-14 June 2012

We report on the kinematics of two interacting CMEs observed on 13 and 14 June 2012. Both CMEs originated from the same active region NOAA 11504. After their launches which were separated by several hours, they were observed to interact at a distance of 100 Rs from the Sun. The interaction led to a moderate geomagnetic storm at the Earth with Dst index of approximately, -86 nT. The kinematics of the two CMEs is estimated using data from the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) onboard the Solar Terrestrial Relations Observatory (STEREO). Assuming a head-on collision scenario, we find that the collision is inelastic in nature. Further, the signatures of their interaction are examined using the in situ observations obtained by Wind and the Advance Composition Explorer (ACE) spacecraft. It is also found that this interaction event led to the strongest sudden storm commencement (SSC) (approximately 150 nT) of the present Solar Cycle 24. The SSC was of long duration, approximately 20 hours. The role of interacting CMEs in enhancing the geoeffectiveness is examined.Comment: 17 pages, 5 figures, Accepted in Solar Physics Journa

Anthropogenic Space Weather

Anthropogenic effects on the space environment started in the late 19th century and reached their peak in the 1960s when high-altitude nuclear explosions were carried out by the USA and the Soviet Union. These explosions created artificial radiation belts near Earth that resulted in major damages to several satellites. Another, unexpected impact of the high-altitude nuclear tests was the electromagnetic pulse (EMP) that can have devastating effects over a large geographic area (as large as the continental United States). Other anthropogenic impacts on the space environment include chemical release ex- periments, high-frequency wave heating of the ionosphere and the interaction of VLF waves with the radiation belts. This paper reviews the fundamental physical process behind these phenomena and discusses the observations of their impacts.Comment: 71 pages, 35 figure