15,989 research outputs found

    The Implementation of Accounting for Environmental Liabilities

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    This study aims to discuss the accounting implementation by the Indonesia Companies in recognizing, measuring, presenting, and disclosing environmental obligations that occur as a result of the company\u27s operations. The analysis is carried out by reviewing disclosures on environmental management activities that have been carried out by the company, which has financial reports and annual reports. The method used is descriptive qualitative method with the data used are secondary data, financial statements, and annual reports obtained from the official website of the Indonesia Stock Exchange from 2015 to 2017 fiscal years. The samples employed in this study is thirteen food and beverage subsector companies listed on the Indonesia Stock Exchange from 2015 to 2017. The results of this study suggest that from 2015 to 2017, the food and beverage sub-sector companies have not reported any environmental obligations in the form of social-environmental responsibilities in the financial statements. The companies report their environmental responsibility activities as a company expense reported on the income statement. Accounting for environmental obligations related to recognition, measurement, recording, disclosure, and reporting has not been regulated in financial accounting standards, so reporting environmental obligations is still voluntary

    Symplectic structures on quadratic Lie algebras

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    We study quadratic Lie algebras over a field K of null characteristic which admit, at the same time, a symplectic structure. We see that if K is algebraically closed every such Lie algebra may be constructed as the T*-extension of a nilpotent algebra admitting an invertiblederivation and also as the double extension of another quadratic symplectic Lie algebra by the one-dimensional Lie algebra. Finally, we prove that every symplectic quadratic Lie algebra is a special symplectic Manin algebra and we give an inductive classification in terms of symplectic quadratic double extensions

    The energy spectrum observed by the AGASA experiment and the spatial distribution of the sources of ultra-high energy cosmic rays

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    Seven and a half years of continuous monitoring of giant air showers triggered by ultra high-energy cosmic rays have been recently summarized by the AGASA collaboration. The resulting energy spectrum indicates clearly that the cosmic ray spectrum extends well beyond the Greisen-Zatsepin-Kuzmin (GZK) cut-off at ∼5×1019\sim 5 \times 10^{19} eV. Furthermore, despite the small number statistics involved, some structure in the spectrum may be emerging. Using numerical simulations, it is demonstrated in the present work that these features are consistent with a spatial distribution of sources that follows the distribution of luminous matter in the local Universe. Therefore, from this point of view, there is no need for a second high-energy component of cosmic rays dominating the spectrum beyond the GZK cut-off.Comment: 14 pages, 4 figures, Astrophys. J. Letters (submitted

    On the significance of the observed clustering of ultra-high energy cosmic rays

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    Three pairs of possibly correlated ultra-high energy cosmic ray events were reported by Hayashida et al (1996). Here we calculate the propagation of the corresponding particles through both the intergalactic and galactic magnetic fields. The large scale disc and halo magnetic components are approximated by the models of Stanev (1997). The intergalactic magnetic field intensity is modulated by the actual density of luminous matter along the corresponding lines of sight, calculated from the CfA redshift catalogue (Huchra et al, 1995). The results indicate that, if the events of each pair had a common source and were simultaneously produced, they either originated inside the galactic halo or otherwise very unlikely events were observed. On the other hand, an estimate of the arrival probability of ultra-high energy cosmic rays, under the assumption that the distribution of luminous matter in the nearby universe traces the distribution of the sources of the particles and intensity of the intergalactic magnetic field, suggests that the pairs are chance clusterings.Comment: Ap. J. Letters Accepted - 13 pages + 4 figure
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