Books/Book Chapters/Edited Books
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Item SWOC Analysis of Educational Institutions in Lucknow(Sandpiper publisher Lucknow, 2025) Amna Siddiqui, Asma FarooqueItem Role of Advertising Standard Council of India(ASCI) in Regulation of Advertisements of FMCG in Lucknow(Sandpiper publisher Lucknow, 2025) Qambar Husain, Asma FarooqueItem Comparative Anlysis of Structural, Electronic and Thermal Properties of ALRE (RE = Y, Pr, Gd)(Book Rivers, 2025) Afroj A Khan, Seema Srivastava, Vipul Srivastava, Ghizal F AnsariThe properties of AlRE in B2 structure have been analysed using the first-principles method. The structural and electronic properties were investigated using the generalized gradient approximation (GGA) method and by TBLMTO method in the context of density functional theory. The electronic band structure calculations carried out to obtain the total energy of the AlRE (RE= Y, Pr, Gd) inter-metallic compound using the first principles FP-LAPW method by Shugani et al and that using TB-LMTO method by Srivastava et al have been compared with experimental data.The equilibrium cell volume Vo is found to be 315.90 a.u3 and 294.82 a.u.3 (43.69) for AlY by FP-LAPW and TB-LMTO respectively.While Vo for AlPr and AlGd is 322.36 a.u.3 , 297.58 a.u.3 (44.099) and 307.57 a.u3, 283.55 a.u.3 (42.02 ).The computed lattice parameter (3.604 Å) and bulk modulus (62.40 GPa) by TB-LMTO and 3.522 and 79.5for AlY by FP-LAPW method while 3.628Å, 65.5GPa for AlPr, 3.572Å, 49.42GPa for AlGd by TB-LMTO and3.533Å, 55.11GPa for AlPr, 3.47Å, 70.60GPa for AlGd by FP-LAPW method. The electronic band structure and energy-dependent density of states reveal the metallic nature of the titled Rare-earth inter- metallic compounds.Item Quark Gluon Plasma: Its Formation and Various Signatures(Book Rivers, 2025) Salman Ahamad KhanThis chapter gives an introduction to the Quark Gluon Plasma (QGP), a primordial state of matter which was present in the early universe just after the few microsecond of the big bang and is also predicted to be in the core of some compact stars. We have discussed the formation of this novel state of matter in the ultra-relativistic heavy ion collision experiments at relativistic heavy ion collider (RHIC) at BNL in USA and large hadron collider (LHC) at CERN. A brief overview of the major signatures of QGP has been presented. A qualitative discussion about the various theoretical techniques employed to study the properties of the QGP has also been done.Item Non-Extensive Statistical Mechanics: Introduction and Its Application in Heavy-Ion Physics(Book Rivers, 2025) Salman Ahamad Khan, Mohd ShahalamThis chapter presents an introduction to the non-extensive statistical mechanics and its application in the high energy physics specially in the context of the matter created in the heavy ion collision experiments at RHIC (BNL) and LHC (CERN). The non-extensive Tsallis distribution function and the computation of various thermodynamical quantities in the non extensive framework have been defined. The fitting of the hadron transverse momentum using the power law distribution has been explained. Apart from that some transport and screening properties of non-extensive quark gluon plasma have also been discussed.Item Cosmic Acceleration: History and Evolution(Book Rivers, 2025) Mohd Shahalam, Salman Ahamad KhanLate time cosmic acceleration of the Universe is one of the biggest and most interesting discovery of our time. It is supported by a number of observational investigations such as Type Ia supernova, cosmic microwave background radiation, surveys of large scale structure, and Planck 2018 results. In the standard framework based upon Einstein gravity, cosmic acceleration can be explained by an exotic fluid with large negative pressure filling the Universe, dubbed `dark energy'. The simplest candidate for dark energy is the cosmological constant Λ. In this chapter, we shall focus on the basic ingredients of the standard model of Universe, Friedmann-Lemaitre-Robertson-Walker metric, cosmological parameters, evidences of late time cosmic acceleration, cosmological observations, and the theoretical models of dark energy in the form of exotic matter and the large scale modification of gravity.Item Dynamical System Analysis in Cosmology(Book Rivers, 2025) Muskan Khan, Mohd ShahalamIn this chapter, we explore the dynamics of the standard cosmological model by framing it as a Newtonian dynamical system. The total energy density ρeff, is specified by the expansion factor a(t), allowing us to interpret the cosmological constant and curvature terms as specialized types of fluid. Our study extends to the analysis of autonomous dynamical system, focusing on the asymptotic behavior of the models under consideration. We introduced a set of first-order differential equations to describe the evolution of variables x(t) and y(t), identifying critical points and analyzing their stability through eigenvalues. The stability of these points, classified as stable, unstable and saddle points, provides insights into the dynamical behavior of the universe. We delve into scalar field models, specifically quintessence, to understand their role in the accelerated expansion of the universe. The cosmological dynamics of the scalar field, governed by a potential V(φ), are analyzed using dimensionless variables and autonomous system. We choose two models: a single exponential potential and a double exponential potential, examining their fixed point analysis. In case of single exponential potential, the system exhibits a critical point that is stable for certain parameter values, indicating a stable attractor. However, the double exponential potential model demonstrates the capability to achieve both scaling and stable accelerating solutions. Concurrently, that feature is not possible with a single exponential potential. Through phase space analysis, we visualize the trajectories and stability of these models, providing a comprehensive understanding of the cosmological dynamics driven by scalar fields. Our findings contribute to the theoretical framework of cosmology, addressing key questions about the expansion of the universe and the cosmic acceleration.Item Psycho-Physiological Impact of Emotions(The Lawjical Junction and MJS Publishing House, 2024) Neha Roshni YooshingThis chapter explores the complex interactions between emotions and how they affect behaviour and human health on a psycho-physiological level. Emotions are not just psychological phenomena; they also have an impact on our overall well-being through physiological alterations. We can learn more about the critical function emotions play in forming our social interaction and overall health by investigating how emotions affect physiological systems. Important topics are covered, with a focus on how different emotions have varying effects on health outcomes. These topics include the bidirectional interaction between mind and body, stress response mechanisms, and neurobiological foundations. This chapter offers a thorough knowledge of how better emotional regulation can improve one's own wellbeing and promote more positive social interactions.Item The Psychology of Decision Making: Discovering the factors influencing choices(Imaginex Inks Publication, 2024) Neha Roshni YooshingThis chapter delves into the psychology of decision making, examining the diverse factors that influence how choices are made. It begins with an introduction to decision-making theories, tracing their historical evolution and highlighting key frameworks like Rational Choice Theory, Behavioral Economics, and Dual-Process Theories. Cognitive aspects such as heuristics, biases, and information processing are explored, alongside the impact of emotions and social influences. Environmental and contextual factors, including physical cues and situational contexts, are analyzed for their role in shaping decisions. Practical applications are considered, providing strategies for improving individual and organizational decision making.Item Bio-hydrogen production from lignocellulosic biomass: A Green Approach(Elite Publishing House, 2025) Arshia Akhtar, HaroonBio-hydrogen (bio-H2), a carbon-low fuel known for its high energy efficiency, is gaining prominence as a renewable energy source amid increasing concerns about climate change and energy demand. Utilizing lignocellulosic biomass holds promise for establishing a clean energy infrastructure. Despite various technologies available for producing bio-H2 from lignocellulosic biomass, such as direct and indirect biophotolysis and fermentations, they suffer from drawbacks like low yields and slow production rates. Bio-H2, distinguishable among biofuels for its carbon neutrality, is achievable through thermochemical conversion methods, presenting an economically viable solution. While certain thermochemical conversion technologies are still in research and development, leveraging organic biomass for hydrogen production is strongly recommended due to its ability to yield larger quantities of the final product and its compatibility with existing infrastructure. This chapter aims to provide current insights into lignocellulose hydrogen conversion progress, tapping into its globally abundant availability.