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                <text>Towards an Epistemology of Reading: Defining the Process of Reading in Modern Terms</text>
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                <text>Enlightenment; Epistemology; Hermeneutics; Modernism; Ontology; Phenomenology; Reading</text>
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                <text>The chaotic space caused by information explosion in present times has made the process and purpose of reading to be always questioned. Technological advancement has made reading appear as a mere mockery at the very outset. But the world still prioritizes knowledge that is acquired through observation, valuation and interpretation. At the time of Big Data, there still persists a sense of agency to define a given information as episteme. The present essay emphasizes on looking at reading as a modern phenomenon by presupposing the epistemological presence at the centre of any rational pursuit. Based on the Kantian precepts on enlightenment, the paper attempts to understand this presence of knowledge by delving into the major disciplines of modern philosophy that help in observing, valuing and interpreting the act of reading in present times. More than laying terms for defining the text within the modern space, the study essentializes reading in a virtually driven algorithmic world.  AesthetixMS 2021</text>
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                <text>Arun D.M.</text>
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                <text>Rupkatha Journal on Interdisciplinary Studies in Humanities, Vol-13, No. 4</text>
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                <text>Aesthetics Media Services</text>
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                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 9752935</text>
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                <text>Arun D.M., Department of English, Pondicherry University, Puducherry, India, Department of English and Cultural Studies, BGR Campus, CHRIST (Deemed to be University), Bangalore, India</text>
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                <text>Effects of dark matter in star formation</text>
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                <text>Dark matter; Early universe; Maximal luminosity; Structure formation</text>
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                <text>The standard model for the formation of structure assumes that there existed small fluctuations in the early universe that grew due to gravitational instability. The origins of these fluctuations are as yet unclear. In this work we propose the role of dark matter in providing the seed for star formation in the early universe. Very recent observations also support the role of dark matter in the formation of these first stars. With this we set observable constraints on luminosities, temperatures, and lifetimes of these early stars with an admixture of dark matter.  2019, Springer Nature B.V.</text>
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                <text>Arun K.; Gudennavar S.B.; Prasad A.; Sivaram C.</text>
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                <text>Astrophysics and Space Science, Vol-364, No. 2</text>
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                <text>Restricted Access</text>
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                <text>ISSN: 0004640X</text>
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                <text>Arun K., Department of Physics and Electronics, Christ (Deemed to be University), Bengaluru, 560029, Karnataka, India, Department of Physics, Christ Junior College, Bengaluru, 560029, Karnataka, India; Gudennavar S.B., Department of Physics and Electronics, Christ (Deemed to be University), Bengaluru, 560029, Karnataka, India; Prasad A., Center for Space Plasma &amp;amp; Aeronomic Research, The University of Alabama in Huntsville, Huntsville, 35899, AL, United States; Sivaram C., Indian Institute of Astrophysics, Bengaluru, 560034, Karnataka, India</text>
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          <element elementId="50">
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            <description>A name given to the resource</description>
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                <text>Alternate models to dark energy</text>
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          <element elementId="49">
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            <description>The topic of the resource</description>
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              <elementText elementTextId="134827">
                <text>Dark energy; Dark matter; Varying gravitational constant; Varying proton mass</text>
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            <description>An account of the resource</description>
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                <text>One of the unresolved questions currently in cosmology is that of the non-linear accelerated expansion of the universe. This has been attributed to the so called Dark Energy (DE). The accelerated expansion of the universe is deduced from measurements of Type Ia supernovae. Here we propose alternate models to account for the Type Ia supernovae measurements without invoking dark energy.  2017 COSPAR</text>
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              <elementText elementTextId="134829">
                <text>Arun K.; Gudennavar S.B.; Prasad A.; Sivaram C.</text>
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                <text>Advances in Space Research, Vol-61, No. 1, pp. 567-570.</text>
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              <elementText elementTextId="134831">
                <text>Elsevier Ltd</text>
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                <text>&lt;a href="https://doi.org/10.1016/j.asr.2017.08.006" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1016/j.asr.2017.08.006&lt;/a&gt;
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              <elementText elementTextId="134834">
                <text>All Open Access; Green Open Access</text>
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                <text>ISSN: 2731177; CODEN: ASRSD</text>
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                <text>English</text>
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                <text>Arun K., Department of Physics, Christ University, Bengaluru, 560029, Karnataka, India, Department of Physics, Christ Junior College, Bengaluru, 560029, Karnataka, India; Gudennavar S.B., Department of Physics, Christ University, Bengaluru, 560029, Karnataka, India; Prasad A., Udaipur Solar Observatory, Physical Research Laboratory, Dewali, Bari Road, Udaipur, 313001, India; Sivaram C., Indian Institute of Astrophysics, Bengaluru, 560034, Karnataka, India</text>
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                <text>Dark matter, dark energy, and alternate models: A review</text>
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          <element elementId="49">
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              <elementText elementTextId="135830">
                <text>Cosmological constant; Dark energy; Dark matter; Dieterici gas; Modifications of general relativity; MOND</text>
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                <text>The nature of dark matter (DM) and dark energy (DE) which is supposed to constitute about 95% of the energy density of the universe is still a mystery. There is no shortage of ideas regarding the nature of both. While some candidates for DM are clearly ruled out, there is still a plethora of viable particles that fit the bill. In the context of DE, while current observations favour a cosmological constant picture, there are other competing models that are equally likely. This paper reviews the different possible candidates for DM including exotic candidates and their possible detection. This review also covers the different models for DE and the possibility of unified models for DM and DE. Keeping in mind the negative results in some of the ongoing DM detection experiments, here we also review the possible alternatives to both DM and DE (such as MOND and modifications of general relativity) and possible means of observationally distinguishing between the alternatives.  2017 COSPAR</text>
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                <text>Arun K.; Gudennavar S.B.; Sivaram C.</text>
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                <text>Advances in Space Research, Vol-60, No. 1, pp. 166-186.</text>
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                <text>Arun K., Department of Physics, Christ University, Bengaluru, 560029, Karnataka, India, Department of Physics, Christ Junior College, Bengaluru, 560029, Karnataka, India; Gudennavar S.B., Department of Physics, Christ University, Bengaluru, 560029, Karnataka, India; Sivaram C., Indian Institute of Astrophysics, Bengaluru, 560034, Karnataka, India</text>
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                <text>One of the possible resolutions of the compactness problem in gamma-ray bursts (GRBs) is by invoking the Lorentz factors associated with the relativistic bulk motion. This model applies to GRBs where sufficient energy is converted to accelerate the ejected matter to relativistic speeds. In some situations, this may not be a possible mechanism, and as a result, the gamma rays are trapped in the region. In this work, we look at such possible scenarios and where the neutrino pair production process can dominate. As a result, the neutrinos can escape freely. This could give rise to a scenario where the release of neutrinos precedes the gamma-ray emission that is much attenuated. This model can thus possibly explain why fewer GRBs are observed than what is expected.  2023, Indian Association for the Cultivation of Science.</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85162710642&amp;amp;doi=10.1007%2Fs12648-023-02814-9&amp;amp;partnerID=40&amp;amp;md5=a4b786c11c8fcae7765e2cf2b062dd03" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85162710642&amp;amp;doi=10.1007%2fs12648-023-02814-9&amp;amp;partnerID=40&amp;amp;md5=a4b786c11c8fcae7765e2cf2b062dd03&lt;/a&gt;</text>
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                <text>ISSN: 9731458</text>
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                <text>Arun K., CHRIST (Deemed to be University), Bangalore, 560 029, India; Sivaram C., Indian Institute of Astrophysics, Bangalore, 560 034, India</text>
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                <text>Synthetic biology for sustainable food ingredients production: recent trends</text>
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                <text>Cell factory; Fermentation; Food ingredients; Metabolic engineering; Synthetics biology</text>
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            </elementTextContainer>
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                <text>Problems with food security result from increased population, global warming, and decrease in cultivable land. With the advancements in synthetic biology, microbial synthesis of food is considered to be an efficient alternate approach that could permit quick food biosynthesis in an eco-friendly method. Furthermore, synthetic biology can be assumed to the synthesis of healthy or specially designed food components like proteins, lipids, amino acids and vitamins and widen the consumption of feedstocks, thus offering possible resolutions to high-quality food synthesis. This review describes the impact of synthetic biology for the microbial synthesis of various food ingredients production.  2022, Jiangnan University.</text>
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                <text>Arun K.B.; Anoopkumar A.N.; Sindhu R.; Binod P.; Aneesh E.M.; Madhavan A.; Awasthi M.K.</text>
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                <text>Systems Microbiology and Biomanufacturing, Vol-3, No. 1, pp. 137-149.</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85142627279&amp;amp;doi=10.1007%2Fs43393-022-00150-3&amp;amp;partnerID=40&amp;amp;md5=65b4f950b63f96e70044eadb515bc156" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85142627279&amp;amp;doi=10.1007%2fs43393-022-00150-3&amp;amp;partnerID=40&amp;amp;md5=65b4f950b63f96e70044eadb515bc156&lt;/a&gt;</text>
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            <name>Rights</name>
            <description>Information about rights held in and over the resource</description>
            <elementTextContainer>
              <elementText elementTextId="195949">
                <text>Restricted Access</text>
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                <text>ISSN: 26627655</text>
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                <text>Arun K.B., Rajiv Gandhi Centre for Biotechnology, Jagathy, Kerala, Thiruvananthapuram, 695 014, India, Department of Life Sciences, CHRIST (Deemed to be University), Karnataka, Bengaluru, 560029, India; Anoopkumar A.N., Department of Zoology, Centre for Research in Emerging Tropical Diseases (CRET-D), University of Calicut, Kerala, Malappuram, India; Sindhu R., Department of Food Technology, T K M Institute of Technology, Kerala, Kollam, 691 505, India; Binod P., Microbial Processes and Technology Division, CSIR-National Institute for Interdisciplinary Science and Technology (CSIR-NIIST), Kerala, Trivandrum, 695 019, India; Aneesh E.M., Department of Zoology, Centre for Research in Emerging Tropical Diseases (CRET-D), University of Calicut, Kerala, Malappuram, India; Madhavan A., Rajiv Gandhi Centre for Biotechnology, Jagathy, Kerala, Thiruvananthapuram, 695 014, India, School of Biotechnology, Amrita Vishwa Vidyapeetham, Kerala, Amritapuri, India; Awasthi M.K., College of Natural Resources and Environment, Northwest A &amp;amp; F University, Shaanxi, Yangling, 712 100, China</text>
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            <elementTextContainer>
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                <text>Integrated biorefinery development for pomegranate peel: Prospects for the production of fuel, chemicals and bioactive molecules</text>
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          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
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              <elementText elementTextId="196347">
                <text>Bioactives; Biofertilizer; Biofuel; Biorefinery; Pomegranate peel</text>
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                <text>Current experimental evidence has revealed that pomegranate peel is a significant source of essential bio compounds, and many of them can be transformed into valorized products. Pomegranate peel can also be used as feedstock to produce fuels and biochemicals. We herein review this pomegranate peel conversion technology and the prospective valorized product that can be synthesized from this frequently disposed fruit waste. The review also discusses its usage as a carbon substrate to synthesize bioactive compounds like phenolics, flavonoids and its use in enzyme biosynthesis. Based on reported experimental evidence, it is apparent that pomegranate peel has a large number of applications, and therefore, the development of an integrated biorefinery concept to use pomegranate peel will aid in effectively utilizing its significant advantages. The biorefinery method displays a promising approach for efficiently using pomegranate peel; nevertheless, further studies should be needed in this area.  2022 Elsevier Ltd</text>
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                <text>Arun K.B.; Madhavan A.; Anoopkumar A.N.; Surendhar A.; Liz Kuriakose L.; Tiwari A.; Sirohi R.; Kuddus M.; Rebello S.; Kumar Awasthi M.; Varjani S.; Reshmy R.; Mathachan Aneesh E.; Binod P.; Sindhu R.</text>
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                <text>Bioresource Technology, Vol-362</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85137086726&amp;amp;doi=10.1016%2Fj.biortech.2022.127833&amp;amp;partnerID=40&amp;amp;md5=2b7c117f889289351cc043a96c817e98" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85137086726&amp;amp;doi=10.1016%2fj.biortech.2022.127833&amp;amp;partnerID=40&amp;amp;md5=2b7c117f889289351cc043a96c817e98&lt;/a&gt;</text>
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                <text>ISSN: 9608524; PubMed ID: 36029981; CODEN: BIRTE</text>
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                <text>Microbes or microbial enzymes can catalyze the synthesis of bioorganic compounds, and this process is defined as biocatalysis. Biocatalysis has become an essential technique in organic biotransformation, typically applied in chemical industries. Biocatalysts generally show high activity and excellent enantio, stereo, regio, and chemo-selectivity. They offer practical and cost-effective ways to synthesize semi-synthetic analogues and novel drug molecules. Many bacteria and fungi-derived enzymes could catalyze highly specific hydroxylations of various substrates that are highly complex to synthesize by chemical methods. This chapter details and discusses different biocatalytic microbial platforms that permit to produce the chiral drug intermediates.  2023 selection and editorial matter, Ranjna Sirohi, Amit Kumar Rai, Luciana Porto de Souza Vandenberghe, and Binod Parameswaran; individual chapters, the contributors</text>
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                <text>Arun K.B., Department of Life Sciences CHRIST (Deemed to be University), Karnataka, Bengaluru, India; Sindhu R., Department of Food Technology, TKM Institute of Technology, Kerala, Kollam, India; Nair B.G., School of Biotechnology, Amrita Vishwa Vidyapeetham Amritapuri, Kerala, Kollam, India; Parameswaran B., Microbial Processes and Technology Division CSIR, National Institute for Interdisciplinary Science and Technology (NIIST), Kerala, Thiruvananthapuram, India; Pandey A., Center for Innovation and Translational Research CSIR  Indian Institute of Toxicology Research (CSIR-IITR), India, Centre for Energy and Environmental Sustainability, Uttar Pradesh, Lucknow, India; Awasthi M.K., Awasthi College of Natural Resources and Environment, Northwest A&amp;amp;F University, Shaanxi, Yangling, China; Kuddus M., Department of Biochemistry, University of Hail, Saudi Arabia; Madhavan A., School of Biotechnology, Amrita Vishwa Vidyapeetham Amritapuri, Kerala, Kollam, India</text>
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                <text>Optimal Shortest Path Routing over Wireless Sensor Networks Using Constrained Genetic Firefly Optimization Algorithm</text>
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                <text>Dynamic source routing (DSR); Firefly algorithm; Genetic algorithm; NS-2 simulator; Particle swarm optimization (PSO); Shortest path routing</text>
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                <text>In Wireless Sensor Networks (WSNs), a large number of sensor nodes are placed over a specific area in any real-life application. The sensor node is small, with limited battery life, memory, and computing capacity. Due to the limited power of the battery, WSNs must expand the system life by minimizing the energy usage. In the existing system, the methods have limitations related to optimal shortest routing path, node energy consumption, network reconfiguration, and so on. In order to overcome these issues, aConstrained Genetic FireFly Optimization Algorithm (CGFFOA) is proposed. The CGFFOA algorithm is designed to select the best shortest path routing through the selection of Cluster Head (CH) nodes based on the better energy utilization, delay, and high throughput sensor nodes. It is used to optimize the routing path based on the energy, hop count, inter and intra cluster delay, and lifetime. The simulation findings therefore conclude that, with regard to reduced energy consumption, higher throughput, and lower end-to-end delay, the proposed CGFFOA algorithm is preferable to existing methods such as Particle Swarm Optimization (PSO) and Dynamic Source Routing (DSR).  2023, The Author(s), under exclusive license to Springer Nature Singapore Pte Ltd.</text>
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                <text>Arun Kokatnoor S.; Reddy V.; Krishnan B.</text>
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                <text>Lecture Notes in Networks and Systems, Vol-608, pp. 643-654.</text>
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                <text>Springer Science and Business Media Deutschland GmbH</text>
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                <text>&lt;a href="https://doi.org/10.1007/978-981-19-9225-4_47" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1007/978-981-19-9225-4_47&lt;/a&gt;
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              <elementText elementTextId="175791">
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                <text>ISSN: 23673370; ISBN: 978-981199224-7</text>
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                <text>Arun Kokatnoor S., Department of Computer Science and Engineering, School of Engineering and Technology, CHRIST (Deemed to be University), Karnataka, Bangalore, India; Reddy V., Department of Computer Science and Engineering, School of Engineering and Technology, CHRIST (Deemed to be University), Karnataka, Bangalore, India; Krishnan B., Department of Computer Science and Engineering, School of Engineering and Technology, CHRIST (Deemed to be University), Karnataka, Bangalore, India</text>
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                <text>SWITCHING INTENTION AND SWITCHING BEHAVIOR OF ADULTS IN THE NON-LIFE INSURANCE SECTOR: MEDIATING ROLE OF BRAND LOVE</text>
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            <name>Subject</name>
            <description>The topic of the resource</description>
            <elementTextContainer>
              <elementText elementTextId="102120">
                <text>barriers; brand love; insurance; non-life insurance; switching behaviors; switching intentions</text>
              </elementText>
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            <name>Description</name>
            <description>An account of the resource</description>
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                <text>In this digital era, customers in the insurance sector always look for better insurance products and services at an affordable price. When customers are unsure about service, they switch over to a better service provider. This behavior is more relevant to non-life insurance. However, the switching behavior of customers is hampered by certain switchover barriers such as brand consciousness, brand pride, brand loyalty, etc. This study focuses on exploring switching intentions and switching behaviors of adults in India keeping brand love as a mediator. A structured questionnaire was employed to collect the primary data from adults having non-life insurance products to analyze switching intentions and switching behaviors. The collected data were analyzed employing SPSS software and Hayes Process Model and appropriate statistical tools. The study results show that the switching intentions of adults vary based on their age, annual income, and education. Mean scores reveal that the lesser the age, the higher the intention to switch over. Further, based on annual income, adults who earn up to Rs 2 lakhs annually have more switching-over intentions (Mean score: 3.9719) followed by adults who earn Rs more than 2 lakhs to 5 lakhs annually (Mean score: 3.7590). Mean scores of education levels regarding switching intentions are higher among more educated adults and less among those who are qualified up to the school level.  Arun Kumar N., Girish S., Suresha B., Mahesh E., 2023.</text>
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              <elementText elementTextId="102122">
                <text>Arun Kumar N.; Girish S.; Suresha B.; Mahesh E.</text>
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              <elementText elementTextId="102123">
                <text>Insurance Markets and Companies, Vol-14, No. 1, pp. 1-7.</text>
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                <text>LLC CPC Business Perspectives</text>
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                <text>&lt;a href="https://doi.org/10.21511/ins.14(1).2023.01" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.21511/ins.14(1).2023.01&lt;/a&gt;
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            <description>Information about rights held in and over the resource</description>
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              <elementText elementTextId="102127">
                <text>All Open Access; Gold Open Access</text>
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                <text>ISSN: 26163551</text>
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                <text>Arun Kumar N., School of Commerce, Finance, and Accountancy, CHRIST (Deemed University), India; Girish S., School of Commerce, Finance, and Accountancy, CHRIST (Deemed University), India; Suresha B., School of Business and Management, CHRIST (Deemed University), India; Mahesh E., School of Social Sciences, CHRIST (Deemed University), India</text>
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                <text>Gender of the Firm Owner and Export Determinants of the Firms in India: an Empirical Analysis</text>
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              <elementText elementTextId="82286">
                <text>Binary Logistic Regression; Exports; Firm Characteristics; Gender; Policies; Resource Stock</text>
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                <text>This study aims to analyse the factors that influence the export decision of firms in India. These factors are unorthodox to the macroeconomic variables, for example, specific firm characteristics and resource stock variables that an enterprise in India may or may not have command over. The most significant of the firm characteristic variables is the gender of the firm owner. Given the binary identity of the explained variable (Export Status of a Firm), the paper uses Binary Logistic Regression. It reports the odds ratio for the individual variable interpretation. The study has also examined descriptive findings and model fit using the Hosmer. The study ceases a statistically significant relationship between the gender of the firm owner and the export decision of a firm. The odds of the firm being an exporter increases when the firm owner is a female. Further, the study also interprets several firm characteristics and resource stock variables that had an impact on the export decision of a firm in India.  2024 AESSRA. All rights reserved.</text>
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                <text>Arun P.; Patavardhan R.; Kshama A.V.</text>
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                <text>ISSN: 4242513</text>
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                <text>Arun P., Department of Economics, Christ University, Bengaluru, Bannerghatta Road Campus, Bannerghatta Main Road, Hulimavu, Karnataka, Bengaluru, India; Patavardhan R., Department of Economics, Christ University, Bengaluru, Bannerghatta Road Campus, Bannerghatta Main Road, Hulimavu, Karnataka, Bengaluru, India; Kshama A.V., Department of Economics, Christ University, Bengaluru, Bannerghatta Road Campus, Bannerghatta Main Road, Hulimavu, Karnataka, Bengaluru, India</text>
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                <text>Clustering of low-mass stars around Herbig Be star IL Cep - Evidence of 'Rocket Effect' using Gaia EDR3 ?</text>
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                <text>stars: formation; stars: kinematics and dynamics; stars: variables: T Tauri, Herbig Ae/Be</text>
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                <text>We study the formation and the kinematic evolution of the early-type Herbig Be star IL Cep and its environment. The young star is a member of the Cep OB3 association, at a distance of 798  9 pc, and has a 'cavity' associated with it. We found that the B0V star HD 216658, which is astrometrically associated with IL Cep, is at the centre of the cavity. From the evaluation of various pressure components created by HD 216658, it is established that the star is capable of creating the cavity. We identified 79 co-moving stars of IL Cep at 2-pc radius from the analysis of Gaia EDR3 astrometry. The transverse velocity analysis of the co-moving stars shows that they belong to two different populations associated with IL Cep and HD 216658, respectively. Further analysis confirms that all the stars in the IL Cep population are mostly coeval (?0.1 Myr). Infrared photometry revealed that there are 26 Class II objects among the co-moving stars. The stars without circumstellar disc (Class III) are 65 per cent of all the co-moving stars. There are nine intense H ? emission candidates identified among the co-moving stars using IPHAS H ? narrow-band photometry. The dendrogram analysis on the Hydrogen column density map identified 11 molecular clump structures on the expanding cavity around IL Cep, making it an active star-forming region. The formation of the IL Cep stellar group due to the 'rocket effect' by HD 216658 is discussed.  2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.</text>
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                <text>Arun R.; Mathew B.; Maheswar G.; Baug T.; Kartha S.S.; Selvakumar G.; Manoj P.; Shridharan B.; Anusha R.; Narang M.</text>
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                <text>Monthly Notices of the Royal Astronomical Society, Vol-507, No. 1, pp. 267-281.</text>
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                <text>&lt;a href="https://doi.org/10.1093/mnras/stab2088" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1093/mnras/stab2088&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85114996333&amp;amp;doi=10.1093%2Fmnras%2Fstab2088&amp;amp;partnerID=40&amp;amp;md5=1c636b191e051bac653749e4edd1dc83" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85114996333&amp;amp;doi=10.1093%2fmnras%2fstab2088&amp;amp;partnerID=40&amp;amp;md5=1c636b191e051bac653749e4edd1dc83&lt;/a&gt;</text>
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              <elementText elementTextId="115137">
                <text>All Open Access; Green Open Access</text>
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                <text>ISSN: 358711; CODEN: MNRAA</text>
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                <text>Arun R., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Mathew B., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Maheswar G., Indian Institute of Astrophysics, Sarjapur Road, Koramangala, Bangalore, 560034, India; Baug T., S.N. Bose National Centre for Basic Sciences, Block-JD, Sector-III, Salt Lake, Kolkata, 700106, India; Kartha S.S., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Selvakumar G., Indian Institute of Astrophysics, Sarjapur Road, Koramangala, Bangalore, 560034, India; Manoj P., Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, 400005, India; Shridharan B., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Anusha R., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Narang M., Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, 400005, India</text>
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          <element elementId="50">
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                <text>Fullerenes in the circumstellar medium of Herbig Ae/Be stars: insights from the Spitzer mid-infrared spectral catalog</text>
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          <element elementId="49">
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            <elementTextContainer>
              <elementText elementTextId="94603">
                <text>astrochemistry; infrared: general; ISM: molecules; stars: variables: T Tauri, Herbig Ae/Be</text>
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              <elementText elementTextId="94604">
                <text>This study presents the largest mid-infrared spectral catalogue of Herbig Ae/Be stars to date, containing the Spitzer Infrared Spectrograph spectra of 126 stars. Based on the catalogue analysis, two prominent infrared vibrational modes of C60 bands at 17.4 and 18.9 ?m are detected in the spectra of nine sources, while 7.0 ?m feature is identified in the spectra of HD 319896. The spectral index analysis and the comparison of the known sources with C60 features indicated that there exist two different types of emission classes among the sample of stars. The infrared spectra of six Herbig Ae/Be stars in this study resemble that of reflection nebulae, and their association with previously known reflection nebulae is confirmed. In the case of three Herbig Ae/Be stars, we report the tentative evidence of C60 emission features originating from the circumstellar disc or nearby diffused emission region. The detection fraction of C60 in the total HAeBe star sample is ?7 per cent, whereas the detection fraction is 30 per cent for HAeBe stars associated with nebulosity. In the catalog, C60 is exclusively present in the circumstellar regions of B type Herbig Ae/Be stars, with no evidence of its presence detected in stars with later spectral types. The present study has increased the number of young stellar objects and reflection nebulae detected with C60 multifold, which can help in understanding the excitation and formation pathway of the species.  2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.</text>
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              <elementText elementTextId="94605">
                <text>Arun R.; Mathew B.; Manoj P.; Maheswar G.; Shridharan B.; Kartha S.S.; Narang M.</text>
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              <elementText elementTextId="94606">
                <text>Monthly Notices of the Royal Astronomical Society, Vol-523, No. 2, pp. 1601-1613.</text>
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              <elementText elementTextId="94607">
                <text>Oxford University Press</text>
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                <text>&lt;a href="https://doi.org/10.1093/mnras/stad1511" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1093/mnras/stad1511&lt;/a&gt;
&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85161702882&amp;amp;doi=10.1093%2Fmnras%2Fstad1511&amp;amp;partnerID=40&amp;amp;md5=12e06089e8d7aa423421d22d9b70416c" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85161702882&amp;amp;doi=10.1093%2fmnras%2fstad1511&amp;amp;partnerID=40&amp;amp;md5=12e06089e8d7aa423421d22d9b70416c&lt;/a&gt;</text>
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            <name>Rights</name>
            <description>Information about rights held in and over the resource</description>
            <elementTextContainer>
              <elementText elementTextId="94610">
                <text>All Open Access; Green Open Access</text>
              </elementText>
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                <text>ISSN: 358711; CODEN: MNRAA</text>
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              <elementText elementTextId="94613">
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              <elementText elementTextId="94614">
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            <description>The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant</description>
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              <elementText elementTextId="94615">
                <text>Arun R., Indian Institute of Astrophysics, Sarjapur Road, Koramangala, Bangalore, 560034, India, Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Mathew B., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Manoj P., Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, 400005, India; Maheswar G., Indian Institute of Astrophysics, Sarjapur Road, Koramangala, Bangalore, 560034, India; Shridharan B., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Kartha S.S., Department of Physics and Electronics, CHRIST (Deemed to be University), Bangalore, 560029, India; Narang M., Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, 400005, India, Institute of Astronomy and Astrophysics, Academia Sinica, No. 1, Section 4, Roosevelt Road, Taipei, 10617, Taiwan</text>
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          <element elementId="50">
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                <text>On the Mass Accretion Rate and Infrared Excess in Herbig Ae/Be Stars</text>
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          <element elementId="49">
            <name>Subject</name>
            <description>The topic of the resource</description>
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              <elementText elementTextId="130272">
                <text>accretion, accretion disks; protoplanetary disks; stars: emission-line, Be; stars: pre-main sequence; stars: variables: T Tauri, Herbig Ae/Be</text>
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                <text>The present study makes use of the unprecedented capability of the Gaia mission to obtain the stellar parameters such as distance, age, and mass of HAeBe stars. The accuracy of Gaia DR2 astrometry is demonstrated from the comparison of the Gaia DR2 distances of 131 HAeBe stars with the previously estimated values from the literature. This is one of the initial studies to estimate the age and mass of a confirmed sample of HAeBe stars using both the photometry and distance from the Gaia mission. Mass accretion rates are calculated from H? line flux measurements of 106 HAeBe stars. Since we used distances and the stellar masses derived from the Gaia DR2 data in the calculation of the mass accretion rate, our estimates are more accurate than previous studies. The mass accretion rate is found to decay exponentially with age, from which we estimated a disk dissipation timescale of 1.9 0.1 Myr. The mass accretion rate and stellar mass exhibit a power-law relation of the form . From the distinct distribution in the values of the infrared spectral index, n2-4.6, we suggest the possibility of difference in the disk structure between Herbig Be and Herbig Ae stars.  2019. The American Astronomical Society. All rights reserved..</text>
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              <elementText elementTextId="130274">
                <text>Arun R.; Mathew B.; Manoj P.; Ujjwal K.; Kartha S.S.; Viswanath G.; Narang M.; Paul K.T.</text>
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              <elementText elementTextId="130275">
                <text>Astronomical Journal, Vol-157, No. 4</text>
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              <elementText elementTextId="130276">
                <text>Institute of Physics Publishing</text>
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              <elementText elementTextId="130279">
                <text>All Open Access; Bronze Open Access; Green Open Access</text>
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                <text>ISSN: 46256</text>
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                <text>Arun R., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Mathew B., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Manoj P., Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai, 400005, India; Ujjwal K., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Kartha S.S., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Viswanath G., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Narang M., Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai, 400005, India; Paul K.T., Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India</text>
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                <text>Discovery of an M-type companion to the Herbig Ae Star V1787 Ori</text>
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                <text>binaries: visual; stars: pre-main-sequence; stars: variables: T Tauri, Herbig Ae/Be</text>
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                <text>The intermediate-mass Herbig Ae star V1787 Ori is a member of the L1641 star-forming region in the Orion A molecular cloud. We report the detection of an M-type companion to V1787 Ori at a projected separation of 6.66 arcsec (corresponding to 2577 au), from the analysis of VLT/NACO adaptive optics Ks-band image. Using astrometric data from Gaia DR2, we show that V1787 Ori A and B share similar distance (d ?387 pc) and proper motion, indicating that they are physically associated. We estimate the spectral type of V1787 Ori B to be M5  2 from colour-spectral type calibration tables and template matching using SpeX spectral library. By fitting PARSEC models in the Pan-STARRS colour-magnitude diagram, we find that V1787 Ori B has an age of 8.1$^{+1.7}_{-1.5}$ Myr and a mass of 0.39$^{+0.02}_{-0.05}$ M. We show that V1787 Ori is a pre-main-sequence wide binary system with a mass ratio of 0.23. Such a low-mass ratio system is rarely identified in Herbig Ae/Be binary systems. We conclude this work with a discussion on possible mechanisms for the formation of V1787 Ori wide binary system.   2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.</text>
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                <text>Arun R.; Mathew B.; Rengaswamy S.; Manoj P.; Narang M.; Kartha S.S.; Maheshwar G.</text>
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                <text>Monthly Notices of the Royal Astronomical Society, Vol-501, No. 1, pp. 1243-1252.</text>
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&lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85100356179&amp;amp;doi=10.1093%2Fmnras%2Fstaa3652&amp;amp;partnerID=40&amp;amp;md5=a1decf917f96ac41f60abeda90c6c772" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/inward/record.uri?eid=2-s2.0-85100356179&amp;amp;doi=10.1093%2fmnras%2fstaa3652&amp;amp;partnerID=40&amp;amp;md5=a1decf917f96ac41f60abeda90c6c772&lt;/a&gt;</text>
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                <text>All Open Access; Green Open Access</text>
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                <text>ISSN: 358711; CODEN: MNRAA</text>
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                <text>Arun R., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Mathew B., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Rengaswamy S., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Manoj P., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Narang M., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Kartha S.S., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India; Maheshwar G., Department of Physics and Electronics, Christ Deemed to Be University, Bangalore, 560029, India</text>
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                <text>Studies on dark matter dark energy and possible alternate models  </text>
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                <text>Physics and Electronics</text>
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                <text>The nature of dark matter (DM) and dark energy (DE) which is supposed to constitute about 95% of the energy density of the universe is still a mystery. There is no shortage of ideas regarding the nature of both. While some candidates for DM are clearly ruled out, there is still a plethora of viable particles that fit the bill. In the context of DE, while current observations favour a cosmological constant picture, there are other competing models which may be equally likely. The standard model for the formation of structure assumes that there newlineexisted small fluctuations in the early universe that grew due to gravitational instability. The origin of these fluctuations are still unclear. In this study, we proposed the role of dark matter in providing the seed for star formation in the early universe, which is supported by very recent observations. With this we set observable constraints on luminosities, temperatures, and lifetimes of the early stars with an admixture of dark matter. We also studied the effects of the background repulsive dark energy density for large scale cosmic structures. The relation, and#119872;and#8260;and#119877;2 and#8776; 1and#119892;/and#119888;and#119898;2, seems to hold true for primeval galaxies as well as those at present epoch. From this, we set constraints on the nature and evolution of dark energy. Besides, we also set constraints on the size of galaxy clusters and superclusters due to the repulsive cosmological dark energy. This could indicate as to why large scale cosmic structures much larger than and#8764;200 Mpc are not seen.This study also looked at the evolution of the concept of the cosmological constant from its inception a little over a hundred years ago when Einstein introduced the cosmological constant in his General Theory of Relativity newlinein order to obtain a static universe to conform to the philosophical view of newlinethe universe at that time to it possibly making up close to about 70% of the energy density of the universe.</text>
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              <elementText elementTextId="66092">
                <text>Arun, Kenath</text>
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                <text>Christ(Deemed to be University)</text>
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            <name>Date</name>
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              <elementText elementTextId="66096">
                <text>Gudennavar, Shivappa B and Sivaram, C</text>
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            <description>Information about rights held in and over the resource</description>
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              <elementText elementTextId="66097">
                <text>Open Access</text>
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                <text>&lt;a href="http://hdl.handle.net/10603/314597" target="_blank" rel="noreferrer noopener"&gt;http://hdl.handle.net/10603/314597&lt;/a&gt;</text>
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                <text>Energy and Environmental Applications of Polymer Based Mixed Metal Oxide Nanocomposites  </text>
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                <text>The dependence of human lives on fossil fuels is very inevitably high for the development of society. This leads to the exploitation of these non-renewable sources, which brings forth society, which is another major issue that has to be tackled. In this study, we have focused on addressing the energy and environmental needs of society using different catalysts. The polymer based mixed metal oxide catalysts are used for the utility towards multiple applications. The energy issues can be mitigated through newlinesupercapacitance studies and water splitting studies. The water splitting studies can newlineproduce hydrogen, an efficient and eco-friendly fuel, and supercapacitors can store newlineenergy effectively. Water pollution is another problem faced by our society, which newlinereduces the availability of freshwater sources. This can be overcome by following newlineeffective and cost-efficient adsorption techniques. Another major threat that prevails in our society is corrosion. Corrosion inhibition studies are followed to tackle this issue and provide a corrosion-free environment. The various polymers used in this study are polyaniline, polypyrrole, poly (3,4-ethylenedioxythiophene), and chitosan. These polymers are mixed with different metal oxides, and the synergy between the polymers and metal oxides provides efficiency towards the mentioned applications. The successful formation of composites is confirmed using various characterization techniques. Several electrochemical studies like cyclic voltammetry, galvanostatic charge-discharge studies, electrochemical impedance spectroscopy, linear sweep voltammetry, and potentiodynamic techniques are employed to analyze the efficacy of the composites towards supercapacitance, water splitting, and corrosion inhibition studies. The batch adsorption studies are executed for water purification studies. The synthesized multifunctional composites can be used as potential candidates for addressing the energy and environmental needs of our society in a sustainable manner.</text>
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                <text>Arun, Varghese</text>
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                <text>K R, Sunaja Devi.</text>
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