84 research outputs found
AERIAL ROBOTICS WITH ARTIFICAL INTELLIGENCE, DESIGN AND APPLICATIONS
No full text<p>First of All I want to express my heart full thanks to Supervisor of my Ph.D. research work Dr. GARG, Calorx Teacher’s University, Ahmedabad. He helped me in every stage of my research work and sincerely guides me about all the issue and new dimensions of research work. I am thankful to all faculty members of department of computer science & electronics engineering.</p>
<p>I am dedicating this thesis to my parents, P B Venu Nath, R Sivakumari and my brother Vinu V Nath.</p>
The development of supergravity grand unification: Circa 1982 1985
No full textThe development in the early eighties of supergravity grand unified models with gravity-mediated breaking of supersymmetry has led to a remarkable progress in the study of supersymmetry at colliders, in dark matter and in a variety of other experimental searches in the intervening years since that time. The purpose of this note is to review this development and describe our construction of this theory in the period 1982-1985. © 2012 World Scientific Publishing Company.Aad G, 2012, PHYS LETT B, V716, P1, DOI 10.1016-j.physletb.2012.08.020; Ahmed Z, 2010, SCIENCE, V327, P1619, DOI 10.1126-science.1186112; Ahmed Z, 2009, PHYS REV LETT, V102, DOI 10.1103-PhysRevLett.102.011301; Akula S, 2012, PHYS REV D, V85, DOI 10.1103-PhysRevD.85.075001; ALVAREZGAUME L, 1983, NUCL PHYS B, V221, P495, DOI 10.1016-0550-3213(83)90591-6; Aprile E., ARXIV11042549ASTROPH; ARNOWITT R, 1983, PHYS REV LETT, V50, P232, DOI 10.1103-PhysRevLett.50.232; ARNOWITT R, 1985, PHYS LETT B, V156, P215, DOI 10.1016-0370-2693(85)91512-6; ARNOWITT R, 1992, PHYS REV LETT, V69, P725, DOI 10.1103-PhysRevLett.69.725; Arnowitt R., 1962, GRAVITATION INTRO CU; Arnowitt R, 2008, PHYS REV LETT, V100, DOI 10.1103-PhysRevLett.100.231802; ARNOWITT R, 1975, PHYS LETT B, VB 56, P81, DOI 10.1016-0370-2693(75)90504-3; Arnowitt R. L., 1983, WORKSH PROBL UN SUP; BAER H, 1994, PHYS REV D, V50, P2148, DOI 10.1103-PhysRevD.50.2148; BAER H, 1986, PHYS REV LETT, V57, P294, DOI 10.1103-PhysRevLett.57.294; Baer H., 2006, WEAK SCALE SUPERSYMM; BAER H, 1985, PHYS LETT B, V155, P278, DOI 10.1016-0370-2693(85)90654-9; BAER H, 1994, PHYS REV D, V50, P4508, DOI 10.1103-PhysRevD.50.4508; BARBIERI R, 1982, PHYS LETT B, V119, P343, DOI 10.1016-0370-2693(82)90685-2; BARBIERI R, 1982, PHYS LETT B, V113, P219, DOI 10.1016-0370-2693(82)90825-5; BARGER V, 1994, PHYS REV D, V49, P4908, DOI 10.1103-PhysRevD.49.4908; Bornhauser S, 2012, EUR PHYS J C, V72, DOI 10.1140-epjc-s10052-012-1887-3; Bouchet FR, 2007, MOD PHYS LETT A, V22, P1857, DOI 10.1142-S0217732307025078; Bueno A., 2007, JHEP, V0704, P041, DOI 10.1088-1126-6708-2007-04-041; CANDELAS P, 1985, NUCL PHYS B, V258, P46, DOI 10.1016-0550-3213(85)90602-9; CHAMSEDDINE AH, 1981, PHYS REV D, V24, P3065, DOI 10.1103-PhysRevD.24.3065; CHAMSEDDINE AH, 1977, NUCL PHYS B, V129, P39, DOI 10.1016-0550-3213(77)90018-9; CHAMSEDDINE AH, 1981, NUCL PHYS B, V185, P403, DOI 10.1016-0550-3213(81)90326-6; CHAMSEDDINE AH, 1982, PHYS REV LETT, V49, P970, DOI 10.1103-PhysRevLett.49.970; CHAMSEDDINE AH, 1983, PHYS LETT B, V129, P445, DOI 10.1016-0370-2693(83)90137-5; Chamseddine AH, 2001, NUCL PHYS B-PROC SUP, V101, P145, DOI 10.1016-S0920-5632(01)01501-8; Chatrchyan S, 2012, PHYS LETT B, V716, P30, DOI 10.1016-j.physletb.2012.08.021; CREMMER E, 1982, PHYS LETT B, V116, P231, DOI 10.1016-0370-2693(82)90332-X; CREMMER E, 1983, NUCL PHYS B, V212, P413, DOI 10.1016-0550-3213(83)90679-X; CREMMER E, 1979, NUCL PHYS B, V147, P105, DOI 10.1016-0550-3213(79)90417-6; DESER S, 1976, PHYS LETT B, V62, P335, DOI 10.1016-0370-2693(76)90089-7; DICUS DA, 1983, PHYS REV LETT, V51, P1030, DOI 10.1103-PhysRevLett.51.1030; DICUS DA, 1983, PHYS LETT B, V129, P451, DOI 10.1016-0370-2693(83)90138-7; DIMOPOULOS S, 1982, PHYS LETT B, V112, P133, DOI 10.1016-0370-2693(82)90313-6; DIMOPOULOS S, 1981, NUCL PHYS B, V193, P150, DOI 10.1016-0550-3213(81)90522-8; DIMOPOULOS S, 1981, PHYS REV D, V24, P1681, DOI 10.1103-PhysRevD.24.1681; Drees M., 2004, SPARTICLES; ELIASSON E, 1984, PHYS LETT B, V147, P65, DOI 10.1016-0370-2693(84)90593-8; Ellis J, ARXIV12023262HEPPH; ELLIS J, 1984, NUCL PHYS B, V247, P373, DOI 10.1016-0550-3213(84)90555-8; ELLIS J, 1982, NUCL PHYS B, V202, P43, DOI 10.1016-0550-3213(82)90220-6; ELLIS J, 1983, PHYS LETT B, V121, P123, DOI 10.1016-0370-2693(83)90900-0; ELLIS J, 1984, NUCL PHYS B, V238, P453, DOI 10.1016-0550-3213(84)90461-9; FAYET P, 1975, NUCL PHYS B, VB 90, P104, DOI 10.1016-0550-3213(75)90636-7; Feldman D, 2007, PHYS REV LETT, V99, DOI 10.1103-PhysRevLett.99.251802; FERRARA S, 1978, PHYS LETT B, V76, P404, DOI 10.1016-0370-2693(78)90893-6; FERRARA S, 1983, PHYS LETT B, V123, P214, DOI 10.1016-0370-2693(83)90425-2; FREEDMAN DZ, 1976, PHYS REV D, V13, P3214, DOI 10.1103-PhysRevD.13.3214; GIRARDELLO L, 1982, NUCL PHYS B, V194, P65, DOI 10.1016-0550-3213(82)90512-0; GIUDICE GF, 1988, PHYS LETT B, V206, P480, DOI 10.1016-0370-2693(88)91613-9; GOLDBERG H, 1983, PHYS REV LETT, V50, P1419, DOI 10.1103-PhysRevLett.50.1419; GOLFAND YA, 1971, JETP LETT-USSR, V13, P323; HABER HE, 1985, PHYS REP, V117, P75, DOI 10.1016-0370-1573(85)90051-1; Hagiwara K, 2011, J PHYS G NUCL PARTIC, V38, DOI 10.1088-0954-3899-38-8-085003; HALL L, 1983, PHYS REV D, V27, P2359, DOI 10.1103-PhysRevD.27.2359; Heinemeyer S, 2004, NUCL PHYS B, V699, P103, DOI 10.1016-j.nuclphysb.2004.08.014; Herten G., COMMUNICATION; Hoecker A, 2011, NUCL PHYS B-PROC SUP, V218, P189, DOI 10.1016-j.nuclphysbps.2011.06.031; IBANEZ L, 1982, PHYS LETT B, V118, P73, DOI 10.1016-0370-2693(82)90604-9; IBANEZ L, 1982, PHYS LETT B, V110, P215; IBANEZ LE, 1984, NUCL PHYS B, V233, P511, DOI 10.1016-0550-3213(84)90581-9; IBANEZ LE, 1985, NUCL PHYS B, V256, P218, DOI 10.1016-0550-3213(85)90393-1; IBANEZ LE, 1983, PHYS LETT B, V126, P54, DOI 10.1016-0370-2693(83)90015-1; INOUE K, 1982, PROG THEOR PHYS, V68, P927, DOI 10.1143-PTP.68.927; KANE GL, 1994, PHYS REV D, V49, P6173, DOI 10.1103-PhysRevD.49.6173; Komatsu E., 2007, ASTROPHYS J SUPPL SE, V170, P377; Komatsu E., 2003, ASTROPHYS J, V148, P175; Komatsu E, 2011, ASTROPHYS J SUPPL S, V192, DOI 10.1088-0067-0049-192-2-18; KOSOWER DA, 1983, PHYS LETT B, V133, P305, DOI 10.1016-0370-2693(83)90152-1; KRAUSS LM, 1983, NUCL PHYS B, V227, P556, DOI 10.1016-0550-3213(83)90574-6; Martin S.P., 1998, PERSPECTIVES SUPERSY, P1; NATH P, 1985, PHYS REV D, V32, P2348, DOI 10.1103-PhysRevD.32.2348; NATH P, 1975, PHYS LETT B, VB 56, P177, DOI 10.1016-0370-2693(75)90297-X; Nath P., 1983, 2588 NUB; Nath P., 1987, MOD PHYS LETT A, V2, P331, DOI 10.1142-S0217732387000446; NATH P, 1983, PHYS LETT B, V121, P33, DOI 10.1016-0370-2693(83)90196-X; Nath P., 1984, APPL N 1 SUPERGRAVIT; NATH P, 1983, NUCL PHYS B, V227, P121, DOI 10.1016-0550-3213(83)90145-1; Nath P., 1984, SUPERSYMMETRY SUPERG, P113; NILLES HP, 1984, PHYS REP, V110, P1, DOI 10.1016-0370-1573(84)90008-5; NILLES HP, 1983, PHYS LETT B, V124, P337, DOI 10.1016-0370-2693(83)91467-3; NILLES HP, 1983, PHYS LETT B, V120, P346, DOI 10.1016-0370-2693(83)90460-4; OVRUT BA, 1982, PHYS LETT B, V119, P105, DOI 10.1016-0370-2693(82)90255-6; Polonyi J., 1977, FKI197793 U BUD; RAMOND P, 1971, PHYS REV D, V3, P2415, DOI 10.1103-PhysRevD.3.2415; ROSS GG, 1992, NUCL PHYS B, V377, P571, DOI 10.1016-0550-3213(92)90302-R; Rubbia A, 2009, J PHYS CONF SER, V171, DOI 10.1088-1742-6596-171-1-012020; SAKAI N, 1981, Z PHYS C PART FIELDS, V11, P153, DOI 10.1007-BF01573998; SAKAI N, 1982, NUCL PHYS B, V197, P533, DOI 10.1016-0550-3213(82)90457-6; SEN A, 1984, PHYS REV D, V30, P2608, DOI 10.1103-PhysRevD.30.2608; SONI SK, 1983, PHYS LETT B, V126, P215, DOI 10.1016-0370-2693(83)90593-2; STELLE KS, 1978, PHYS LETT B, V77, P376, DOI 10.1016-0370-2693(78)90581-6; Tonelli G., COMMUNICATION; VOLKOV DV, 1972, JETP LETT+, V16, P438; WEINBERG S, 1982, PHYS REV D, V26, P287, DOI 10.1103-PhysRevD.26.287; WEINBERG S, 1976, PHYS LETT B, V62, P111, DOI 10.1016-0370-2693(76)90062-9; WEINBERG S, 1982, PHYS REV LETT, V48, P1776, DOI 10.1103-PhysRevLett.48.1776; WEINBERG S, 1983, PHYS REV LETT, V50, P387, DOI 10.1103-PhysRevLett.50.387; WESS J, 1974, NUCL PHYS B, VB 70, P39, DOI 10.1016-0550-3213(74)90355-1; WESS J, 1974, NUCL PHYS B, VB 78, P1, DOI 10.1016-0550-3213(74)90112-6; WITTEN E, 1981, NUCL PHYS B, V188, P513, DOI 10.1016-0550-3213(81)90006-7; WITTEN E, 1982, NUCL PHYS B, V202, P253, DOI 10.1016-0550-3213(82)90071-2; YUAN TC, 1984, Z PHYS C PART FIELDS, V26, P407, DOI 10.1007-BF0145256733
Moral essayes : contain'd in several treatises on many important duties /
No full textArmorial book-plate of Nath. Cholmley Esqr.Title of v. 4 varies.Title within double line border.Signatures: v. 1. A⁴, B-O⁸; v. 2. A-N⁸; v. 3. A⁴, B-P⁸, Q⁴ (A₁, blank? wanting; A₃ incorrectly signed B₃); v. 4. A⁴, B-P⁸.Nicole is credited with authorship even though t.p. has plural author statement.Volumes 1, 3, "third edition, with amendments"; v. 2, "second edition".Mode of access: Internet
Behaviour of buried pipelines subjected to external loading.
No full textThe research presented in this Thesis was carried out at the University of Sheffield under
the supervision of Dr I. C. Pyrah and Dr W. F. Anderson, and Mr G. Leach at British Gas
Engineering Research Station (ERS). The research was financially supported by a British
Gas Research Scholarship and by the Overseas Research Students Awards Scheme.
The Author would like to express his sincere gratitude to his supervisors for their invaluable
help, guidance and encouragement during the development of the research.
The Author is also grateful to Dr S. R. Mi for his interest and assistance throughout the
research. Special thanks also go to Dr S. J. Wheeler for his supervision during the first year
of the research and sound advice in the initial stage of the work.
The Author would like to express his gratitude to all members of the geotechnics group at
the University of Sheffield for the useful discussions and comments. Special thanks and
appreciation are extended to the staff at the ERS, particularly Mr E. Middleton for
providing the data of the field tests and constructive comments.
The laboratory tests were performed at ERS Soils Laboratory for which the Author is
thankful to the laboratory staff. The Author must also thank British Gas for providing the
computer hardware and software for performing the numerical analyses, and the printing
facilities to produce the Thesis. Thanks also go to Mr D. Reay and Mr B. Bellwood at the
Gas Research Centre of British Gas for ensuring continuous financial support throughout
the award period.
Finally, the Author wishes to thank his family and friends for their endless support and
encouragement throughout the period of study in the UK. Without them, this Thesis may
never have been completed
LRS Bianchi Type V perfect fluid cosmological model in f (R,T) theory
No full textThis article deals with the study of Bianchi type V cosmological model filled with perfect fluid in the context of f (R,T) gravity. R and T represents the Ricci scalar and trace of the energy-momentum tensor respectively. The modified Einstein's field equations are solved under the consideration of hybrid exponential law (HEL) for two cases of f (R,T). The presented models are shear free.The accepted manuscript in pdf format is listed with the files at the bottom of this page. The presentation of the authors' names and (or) special characters in the title of the manuscript may differ slightly between what is listed on this page and what is listed in the pdf file of the accepted manuscript; that in the pdf file of the accepted manuscript is what was submitted by the author
Transport Properties of 3D And 2D Disordered Electronic Materials
No full textIn the real world, the crystalline states are exceptions rather than the rule. Disorder exists in varying forms and degrees, ranging from a few impurities or voids in otherwise perfect crystals to the strongly disordered amorphous materials and alloys. Due to the lack of periodicity and translational symmetry of disordered materials, one might expect that the universal features of crystalline materials would disappear as well. Yet the possibility of corresponding universal features in the electronic structure of disordered materials which are different from perfect crystals, made the study of the disordered material is one of the most intriguing topics in solid-state physics. This doctoral dissertation addresses application oriented challenges and some of the related basic science questions about transport properties of two such disordered materials of different dimensionality. Ion-implanted Silicon Carbide (SiC) near degeneracy is studied as an example of a three dimensional (3D) disordered material. Epitaxial gaphene grown on SiC and systematically damaged by the introduction of low temperature plasma is studied an example of two dimensional (2D) disordered material.This work is embargoed by the author and will not be publicly available until January 1, 2016
The Non-fictions of V.S. Naipaul: A Critical Exploration
No full textV. S. Naipaul is an eminent literary figure in the field of modern fiction, non-fiction, and travelogue writing in English literature. He earned a number of literary awards and accolades, including the covetous Nobel Prize and Booker Prize. His non-fiction e.g., An Area of Darkness, India: A Wounded Civilization, The Loss of El Dorado, India: A Million Mutinies Now and Beyond Belief are a realistic portrayal of the various types of religion, culture, customs, and people of India. As an author, the main purpose of V. S. Naipaul is to deliver the truth; because poets are the unacknowledged legislators of mankind. The fact that V. S. Naipaul has presented in his non-fiction is more authentic and realistic than that of his fiction. Nonetheless, it is fictional work that is elaborately explored, discussed, and analyzed in abundance. On the other hand, his non-fiction, by and far, remains aloof. In the last few decades, non-fictions are also taking the ground strongly. Now non-fiction writings are being analyzed, elucidated, and explored based on various theoretical principles of literary criticism.
V. S. Naipaul carried the new genre to new heights and achievements. He is of Indian descent and known for his pessimistic works set in developing countries. He visited India several times, like Pearl S. Buck and E. M. Forster. So, his presentation of Indian religion, society, culture, and politics are very realistic. His vision and ideas are very close to the modern thoughts and visions of both the east and the west
Advanced Nanostructured Concepts in Solar Cells using III-V and Silicon-Based Materials
No full textabstract: As existing solar cell technologies come closer to their theoretical efficiency, new concepts that overcome the Shockley-Queisser limit and exceed 50% efficiency need to be explored. New materials systems are often investigated to achieve this, but the use of existing solar cell materials in advanced concept approaches is compelling for multiple theoretical and practical reasons. In order to include advanced concept approaches into existing materials, nanostructures are used as they alter the physical properties of these materials. To explore advanced nanostructured concepts with existing materials such as III-V alloys, silicon and/or silicon/germanium and associated alloys, fundamental aspects of using these materials in advanced concept nanostructured solar cells must be understood. Chief among these is the determination and predication of optimum electronic band structures, including effects such as strain on the band structure, and the material's opto-electronic properties. Nanostructures have a large impact on band structure and electronic properties through quantum confinement. An additional large effect is the change in band structure due to elastic strain caused by lattice mismatch between the barrier and nanostructured (usually self-assembled QDs) materials. To develop a material model for advanced concept solar cells, the band structure is calculated for single as well as vertical array of quantum dots with the realistic effects such as strain, associated with the epitaxial growth of these materials. The results show significant effect of strain in band structure. More importantly, the band diagram of a vertical array of QDs with different spacer layer thickness show significant change in band offsets, especially for heavy and light hole valence bands when the spacer layer thickness is reduced. These results, ultimately, have significance to develop a material model for advance concept solar cells that use the QD nanostructures as absorbing medium. The band structure calculations serve as the basis for multiple other calculations. Chief among these is that the model allows the design of a practical QD advanced concept solar cell, which meets key design criteria such as a negligible valence band offset between the QD/barrier materials and close to optimum band gaps, resulting in the predication of optimum material combinations.Dissertation/ThesisPh.D. Electrical Engineering 201
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