1,039 research outputs found

    Variability of stellar granulation and convective blueshift with spectral type and magnetic activity. I. K and G main sequence stars

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    In solar-type stars, the attenuation of convective blueshift by stellar magnetic activity dominates the RV variations over the low amplitude signal induced by low mass planets. Models of stars that differ from the Sun will require a good knowledge of the attenuation of the convective blueshift to estimate its impact on the variations. It is therefore crucial to precisely determine not only the amplitude of the convective blueshift for different types of stars, but also the dependence of this convective blueshift on magnetic activity, as these are key factors in our model producing the RV. We studied a sample of main sequence stars with spectral types from G0 to K2 and focused on their temporally averaged properties: the activity level and a criterion allowing to characterise the amplitude of the convective blueshift. We find the differential velocity shifts of spectral lines due to convection to depend on the spectral type, the wavelength (this dependence is correlated with the Teff and activity level), and on the activity level. This allows us to quantify the dependence of granulation properties on magnetic activity for stars other than the Sun. The attenuation factor of the convective blueshift appears to be constant over the considered range of spectral types. We derive a convective blueshift which decreases towards lower temperatures, with a trend in close agreement with models for Teff lower than 5800 K, but with a significantly larger global amplitude. We finally compare the observed RV variation amplitudes with those that could be derived from our convective blueshift using a simple law and find a general agreement on the amplitude. Our results are consistent with previous results and provide, for the first time, an estimation of the convective blueshift as a function of Teff, magnetic activity, and wavelength, over a large sample of G and K main sequence stars

    On the expressive power of read-once determinants

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    We introduce and study the notion of read-kk projections of the determinant: a polynomial f∈F[x1,…,xn]f \in \mathbb{F}[x_1, \ldots, x_n] is called a {\it read-kk projection of determinant} if f=det(M)f=det(M), where entries of matrix MM are either field elements or variables such that each variable appears at most kk times in MM. A monomial set SS is said to be expressible as read-kk projection of determinant if there is a read-kk projection of determinant ff such that the monomial set of ff is equal to SS. We obtain basic results relating read-kk determinantal projections to the well-studied notion of determinantal complexity. We show that for sufficiently large nn, the n×nn \times n permanent polynomial PermnPerm_n and the elementary symmetric polynomials of degree dd on nn variables SndS_n^d for 2≤d≤n−22 \leq d \leq n-2 are not expressible as read-once projection of determinant, whereas mon(Permn)mon(Perm_n) and mon(Snd)mon(S_n^d) are expressible as read-once projections of determinant. We also give examples of monomial sets which are not expressible as read-once projections of determinant

    Aquilegia, Vol. 29 No. 4, September-October 2005: Newsletter of the Colorado Native Plant Society

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    https://epublications.regis.edu/aquilegia/1106/thumbnail.jp

    Magnetic frustration in a stoichiometric spin-chain compound, Ca3_3CoIrO6_6

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    The temperature dependent ac and dc magnetization and heat capacity data of Ca3_3CoIrO6_6, a spin-chain compound crystallizing in a K4_4CdCl6_6-derived rhombohedral structure, show the features due to magnetic ordering of a frustrated-type below about 30 K, however without exhibiting the signatures of the so-called "partially disordered antiferromagnetic structure" encountered in the isostructural compounds, Ca3_3Co2_2O6_6 and Ca3_3CoRhO6_6. This class of compounds thus provides a variety for probing the consequences of magnetic frustration due to topological reasons in stoichiometric spin-chain materials, presumably arising from subtle differences in the interchain and intrachain magnetic coupling strengths. This compound presents additional interesting situations in the sense that, ac susceptibility exhibits a large frequency dependence in the vicinity of 30 K uncharacteristic of conventional spin-glasses, with this frustrated magnetic state being robust to the application of external magnetic fields.Comment: Physical Review (Rapid Communications), in pres

    Spin Gaps in High Temperature Superconductors

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    The phenomenology and theory of spin gap effects in high temperature superconductors is summarized. It is argued that the spin gap behavior can only be explained by a model of charge 0 spin 1/2 fermions which become paired into singlets and that there are both theoretical and experimental reasons for believing that the pairing is greatly enhanced in the bilayer structure of the YBa2Cu3O6+xYBa_2Cu_3O_{6+x} system. This article will appear in the Proceedings of the Stanford Conference on Spectroscopies in Novel Superconductors. To obtain postscript files containing the figures send mail to [email protected]: 9 pages, revtex. To obtain figures contact [email protected]

    Caloric Restriction Alters Postprandial Responses of Essential Brain Metabolites in Young Adult Mice

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    Caloric restriction (CR) has been shown to extend longevity and protect brain function in aging. However, the effects of CR in young adult mice remain largely unexplored. In addition to the fundamental, long-term changes, recent studies demonstrate that CR has a significant impact on transient, postprandial metabolic flexibility and turnover compared to control groups. The goal of this study was to identify the brain metabolic changes at a transient (2 h) and steady (6 h) postprandial state in young mice (5–6 months of age) fed with CR or ad libitum (AL; free eating). Using metabolomics profiling, we show that CR mice had significantly higher levels of neurotransmitters (e.g., glutamate, N-acetylglutamate), neuronal integrity markers (e.g., NAA and NAAG), essential fatty acids (e.g., DHA and DPA), and biochemicals associated carnitine metabolism (related to reduced oxidative stress and inflammation) in the cerebral cortex and hippocampus at 2-h. These biochemicals remained at high levels at the 6-h postprandial time-point. The AL mice did not show the similar increases in essential fatty acid and carnitine metabolism until the 6-h time-point, and failed to show increases in neurotransmitters and neuronal integrity markers at any time-point. On the other hand, metabolites related to glucose utilization—glycolysis and pentose phosphate pathway (PPP)—were low in the CR mice throughout the 6-h period and significantly increased at the 6-h time-point in the AL mice. Our findings suggest that CR induces distinct postprandial responses in metabolites that are essential to maintain brain functions. CR mice produced higher levels of essential brain metabolites in a shorter period after a meal and sustained the levels for an extended period, while maintaining a lower level of glucose utilization. These early brain metabolism changes in the CR mice might play a critical role for neuroprotection in aging. Understanding the interplay between dietary intervention and postprandial metabolic responses from an early age may have profound implications for impeding brain aging and reducing risk for neurodegenerative disorders
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