Rani Mohanraj, Shuba Kumar, Sylvia Jayakumar
et al.
Polished white rice (WR), high in refined carbohydrates, the main staple in South India is associated with enhanced risk of diabetes. Brown Rice (BR), with lower glycemic load, high fibre content and micronutrients, is a healthier choice. Two hundred and twelve Persons with Diabetes (PwD) attending a tertiary diabetes care centre in a city in South India responded to a questionnaire documenting types, frequency and reasons for rice consumption, awareness and beliefs about BR. A sub-set of 10, participated in qualitative interviews, which additionally, explored the influence of traditional beliefs on and consumption patterns of rice, barriers to BR consumption and willingness to accept it in their diet. Ninety-three percent reported consuming WR with traditional usage (97 %) being the main reason for its preference. Brand image, grain size, texture and taste, of rice were other decisional considerations. Awareness about health benefits of BR was limited, with 69 % and 51 % believing it to be nutritious and helping to reduce blood sugar respectively. Appearance, texture, taste and cost were deterrents to its use. Over half agreed to switch to BR if they believed it would improve their health. Participants with a shorter duration of diabetes were more willing to change to BR. The study highlights the need to promote greater literacy regarding health benefits of BR and other forms of less polished rice. Larger trials examining the effectiveness of BR viz-a viz other types of less polished rice on blood glucose levels, metabolic factors and nutritional content among PwD are needed.
History of scholarship and learning. The humanities, Social sciences (General)
Preface Introduction Part I. The Intellectual Context: The Conditions of Enquiry: 1. Manuscripts John F. D'Amico 2. Printing and censorship Paul F. Grendler 3. The Renaissance concept of philosophy Cesare Vasoli 4. Translation, terminology and style in philosophical discourse Brain P. Copenhaver 5. Humanism Paul Oskar Kristeller Part II. Philosophy and its Parts: Logic and Language: 6. Traditional logic E. J. Ashworth 7. Humanistic logic Lisa Jardine Part III. Natural Philosophy: 8. Traditional natural philosophy William A. Wallace 9. The new philosophy of nature Alfonso Ingegno 10. Astrology and magic Brian P. Copenhaver 11. Moral philosophy Jill Kraye 12. Political philosophy Quentin Skinner Part IV. Psychology: 13. The concept of psychology Katharine Park and Eckhard Kessler 14. The organic soul Katharine Park 15. The intellective soul Eckhard Kessler 16. Metaphysics Charles H. Lohr Part V. Problems of Knowledge and Action: 17. Fate, fortune, providence and human freedom Antonino Poppi 18. Theories of knowledge Richard H. Popkin 19. Epistemology of the sciences Nicholas Jardine Part VI. Philosophy and Humanistic Disciplines: 20. Rhetoric and poetics Brian Vickers 21. The theory of history Donald R. Kelley Supplementary material Appendices 22. The availability of ancient works Anthony Grafton 23. The rise of the philosophical textbook Charles B. Schmitt Bibliographies Michael J. Wilmott and Charles B. Schmitt Bibliography Michael J. Wilmott and Charles B. Schmitt Index.
The relevance of addressing the understanding of the geography of religion as a section of religious studies is on the one hand due to the growing popularity of this discipline in the modern scientific space, and on the other its insufficient conceptualisation. The high interest in the geography of religion on the part of the scientific community is caused by its focus on the comprehension of theoretical and practical problems related to the spatial characteristics of religious life. Nowadays, the study of territorial aspects of the coexistence of different religious traditions acquires a special urgency due to the combination of globalisation trends and the desire to preserve authentic identity. Historically, the problem field and scientific apparatus of the geography of religion has been formed with reliance on theoretical developments and methodological tools of philosophy and various scientific disciplines, which supports terminological and methodological polyphony within this discipline and hinders its conceptualisation. The aim of this work is to identify possible grounds for attributing the geography of religion to the sections of religious studies. To achieve this goal the following tasks were solved: the origins of the formation of geography of religion were revealed; the approach to the formation of geography of religion from the perspective of geographical science was analysed; the influence of philosophy of religion on the methodological foundations of geography of religion was shown; the main vectors of interrelation between geography of religion and religious studies were determined. The research is limited to the European tradition of studying the relationship between religion and geography. The study is based on the texts of the classics of philosophical thought, as well as the works of Russian and foreign scholars devoted to the comprehension of the geography of religion as a scientific discipline. To reconstruct the thinkers' position on the issues raised, to identify their dependence on the intellectual context and to compare them, such methods as historical and philosophical analysis of the text, discourse analysis and comparative analysis were used. The result of the study was the substantiation of the conclusion about the possibility and expediency of attributing the geography of religion to the branches of religious studies. Such positioning of geography of religion does not contradict the modern understanding of the problem field and tasks of this discipline as they are formulated within the framework of geographical science, and at the same time allows us to identify promising research strategies in interaction with various religious studies disciplines such as: philosophy of religion, history of religion, anthropology of religion, sociology of religion and psychology of religion.
The Gaia-Sausage-Enceladus merger was a major event in the history of the Milky Way. Studies on Milky Way satellite dwarf galaxies show that key elemental abundance patterns, which probe different nucleosynthetic channels, reflect the host galaxy's star formation history. We gather Mg, Fe, Ba, and Eu abundance measurements for Gaia-Sausage-Enceladus stars from the SAGA database and use [Fe/Mg], [Ba/Mg], [Eu/Mg], and [Eu/Ba], as a function of [Fe/H] to constrain the star formation history of Gaia-Sausage-Enceladus. We use the known star formation histories and elemental abundance patterns of the Sculptor and Fornax dwarf spheroidal galaxies as comparison. The elemental abundance ratios of [Fe/Mg], [Ba/Mg], [Eu/Mg], and [Eu/Ba] all increase with [Fe/H] in Gaia-Sausage- Enceladus. The [Eu/Mg] begins to increase at [Fe/H]= -2.0 and continues steadily, contrasting with the Sculptor dSph galaxy. The [Eu/Ba] increases and remains high across the [Fe/H] range, contrasting with that of the Sculptor dSph galaxy and deviating from the Fornax dSph galaxy at high [Fe/H]. The [Ba/Mg] is higher than those of the Sculptor dSph galaxy at the lowest [Fe/H] and gradually increases, similar to the Fornax dSph galaxy. We constrain three main properties of the Gaia-Sausage-Enceladus star formation history: 1) star formation started gradually, 2) it extended for over 2 Gyr, and 3) it was quenched around [Fe/H] of -0.5, likely when it fell into the Milky Way.
Stellar halos of galaxies retain crucial clues to their mass assembly history. It is in these galactic components that the remains of cannibalised galactic building blocks are deposited. For the case of the Milky Way, the opportunity to analyse the stellar halo's structure on a star-by-star basis in a multi-faceted approach provides a basis from which to infer its past and assembly history in unrivalled detail. Moreover, the insights that can be gained about the formation of the Galaxy not only help constrain the evolution of our Milky Way, but may also help place constraints on the formation of other disc galaxies in the Universe. This paper includes a summary of work undertaken during a PhD thesis aiming to make progress toward answering the most fundamental question in the field of Galactic archaeology: "How did the Milky Way form?" Through the effort to answer this question, we summarise new insights into aspects of the history of assembly and evolution of our Galaxy and measurements of the structure of various of its Galactic components.
We develop and apply a new framework for reconstructing the ionization history during the epoch of recombination with combinations of cosmic microwave background (CMB), baryon acoustic oscillation (BAO) and supernova data. We find a wide range of ionization histories that are consistent with current CMB data, and also that cosmological parameter constraints are significantly weakened once freedom in recombination is introduced. BAO data partially break the degeneracy between cosmological parameters and the recombination model, and are therefore important in these reconstructions. The 95% confidence upper limits on H0 are 80.1 (70.7) km/s/Mpc given CMB (CMB+BAO) data, assuming no other changes are made to the standard cosmological model. Including Cepheid-calibrated supernova data in the analysis drives a preference for non-standard recombination histories with visibility functions that peak early and exhibit appreciable skewness. Forthcoming measurements from SPT-3G will reduce the uncertainties in our reconstructions by about a factor of two.
There are about 6000 stars, that can be seen with the naked eye and have been observed for centuries for various purposes. More modern investigations using advanced telescopes show that our Milky Way, a quite common galaxy, consists of about 100 -- 400 billion stars. And, it is estimated that there are between 200 billion to 2 trillion galaxies in the observable universe -- all of them consist mostly of stars, and sending observable signals which also represents nothing more than a superposition of the light of individual stars. So we can conclude that the most common observable objects in the Universe are $\textit{stars}$. In this chapter, we focus on the long history of the observation of stars (compared to studies in other fields of science) to find out more about the nature of these objects.
Acute disseminated encephalomyelitis (ADEM) is a severe acute inflammatory process of the Central Nervous System (CNS) consisting of multiple foci of perivascular demyelination. It is a relatively frequent complication of infections and immunization among children. Systemic lupus Erythematosus (SLE), is a chronic autoimmune disease, of unknown etiology, that touches multiple organs simultaneously or additionally, with serious morbidity and mortality. More frequent in females, it can be associated with other auto-immune diseases. ADEM is rarely reported as the initial presentation of SLE, even rarer in the pediatric population. We present one case of a 13 years old girl with a history of ADEM, who was diagnosed with SLE eight months later.
To investigate the dynamic response of permeable asphalt mixture pavements, a discrete element model was developed using PFC2D under the coupling of seepage and stress fields. This study examines the excess pore water pressure and dynamic behavior of permeable asphalt mixture pavements under the coupling of seepage and stress fields. The findings indicate that the excess pore water pressure amplifies compressive strain and stress at the base of the permeable asphalt mixture over time, while exhibiting alternating positive and negative fluctuations as a roller traverses the pavement.