Loading...
Search for: gravitation
0.012 seconds
Total 194 records

    Gravitational reduction of the wave function based on bohmian quantum potential

    , Article International Journal of Modern Physics A ; Volume 33, Issue 22 , 2018 ; 0217751X (ISSN) Rahmani, F ; Golshani, M ; Jafari, G ; Sharif University of Technology
    Abstract
    In objective gravitational reduction of the wave function of a quantum system, the classical limit of the system is obtained in terms of the objective properties of the system. On the other hand, in Bohmian quantum mechanics the usual criterion for getting classical limit is the vanishing of the quantum potential or the quantum force of the system, which suffers from the lack of an objective description. In this regard, we investigated the usual criterion of getting the classical limit of a free particle in Bohmian quantum mechanics. Then we argued how it is possible to have an objective gravitational classical limit related to the Bohmian mechanical concepts like quantum potential or... 

    Brane cosmology with string antisymmetric field

    , Article 12th Regional Conference on Mathematical Physics, Islamabad, 27 March 2006 through 1 April 2006 ; 2007 , Pages 73-78 ; 9812705910 (ISBN); 9789812705914 (ISBN) Ardalan, F ; Sharif University of Technology
    World Scientific Publishing Co. Pte Ltd  2007
    Abstract
    The equations of a string inspired noncommutative gravity model on a brane are shown to admit a first integral, generalizing the five dimensional Friedman equation for the FRW Hubble parameter. Copyright © 2007 by World Scientific Publishing Co. Pvt. Ltd  

    A public code for astrometric microlensing with contour integration

    , Article Monthly Notices of the Royal Astronomical Society ; Volume 505, Issue 1 , 2021 , Pages 126-135 ; 00358711 (ISSN) Bozza, V ; Khalouei, E ; Bachelet, E ; Sharif University of Technology
    Oxford University Press  2021
    Abstract
    We present the first public code for the calculation of the astrometric centroid shift occurring during microlensing events. The computation is based on the contour integration scheme and covers single and binary lensing of finite sources with arbitrary limb darkening profiles. This allows for general detailed investigations of the impact of finite source size in astrometric binary microlensing. The new code is embedded in version 3.0 of vbbinarylensing, which offers a powerful computational tool for extensive studies of microlensing data from current surveys and future space missions. © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society  

    Hydrofoil attack angle effect on hydrodynamic resistance of semi-planning catamaran

    , Article 24th International Conference on Offshore Mechanics and Arctic Engineering, 2005, Halkidiki, 12 June 2005 through 17 June 2005 ; Volume 2 , 2005 , Pages 695-702 Rad, M ; Nakisa, M ; Golnezhad, G ; Askari, M ; Sharif University of Technology
    2005
    Abstract
    The present paper contains results of experimental study on a semi-planing catamaran. The aim of this study is to find the effect of hydrofoil usage on resistance of semi-planing catamaran and achieving optimal attack angle, arrangement of hydrofoils and displacement center of gravity. Tests have been done without and with hydrofoils in certain arrangement with different angles of attack then the results are compared. Results show that considerable resistance reduction obtained in semi-planing vessels which equipped with hydrofoil in optimized angle of attack in service speed range. Meanwhile the hydrofoils arrangement and the angle of attack are important so unsuitable design causes the... 

    Study of a strategy for parallax microlensing detection towards the Magellanic Clouds

    , Article Astronomy and Astrophysics ; Volume 412, Issue 1 , 2003 , Pages 81-90 ; 00046361 (ISSN) Rahvar, S ; Moniez, M ; Ansari, R ; Perdereau, O ; Sharif University of Technology
    EDP Sciences  2003
    Abstract
    In this article, we have investigated the possibility to distinguish between different galactic models through microlensing parallax studies. We show that a systematic search for parallax effects can be done using the currently running alert systems and complementary photometric telescopes, to distinguish between different lens distance distributions. We have considered two galactic dark compact object distributions, with total optical depths corresponding to the EROS current upper limits. These models correspond to two extreme hypotheses on a three component galactic structure made of a thin disk, a thick disk, and a spherically symmetric halo. Our study shows that for sub-solar mass... 

    Detecting Exoplanets via Binary-Source Microlensing Events with Spitzer and WFIST

    , Ph.D. Dissertation Sharif University of Technology Bagheri, Fatemeh (Author) ; Rahvar, Sohrab (Supervisor)
    Abstract
    We investigate the possibility of exoplanet detection orbiting source stars in microlensing events through the Spitzer and WFIRST follow-up observations.We perform a Monto Carlo simulation on the detection rate of exoplanets via microlensing, assuming that each source star has at least one exoplanet. The exoplanet can reflect part of the light from the parent star or emit internal thermal radiation. In this new detection channel, we use microlensing as an amplifier to magnify the reflection light from the planet.In the literature, this mode of detecting exoplanets has been investigated much less than the usual mode in which the exoplanets are considered as one companion in binary lens... 

    Data Analysis of Gaia and OGLE Projects and Determination Properties of Gravitational Microlensing

    , M.Sc. Thesis Sharif University of Technology Mozaheb, Saeed (Author) ; Rahvar, Sohrab (Supervisor)
    Abstract
    At the beginning of the 20th century, Albert Einstein introduced the equations of general relativity, opening a new avenue for investigating various phenomena. One of the predictions of these equations, gravitational lensing, was observed by Eddington during his lifetime, confirming the theory's ability to describe nature. Gravitational lensing can be categorized into three types: strong lensing, weak lensing, and microlensing. The current focus of research is on observing the separation phenomenon in gravitational microlensing. The observation of gravitational microlensing provides valuable insights into the composition of celestial bodies in the universe. Calculating the mass of different... 

    Motion of deformable ring made of IPMC

    , Article Proceedings of SPIE - The International Society for Optical Engineering ; Vol. 8409 , 2012 ; ISSN: 0277786X ; ISBN: 9780819490872 Firouzeh, A ; Alasty, A ; Ozmaeian, M ; Sharif University of Technology
    Abstract
    In this paper application of Ionic Polymer Metal Composite (IPMC) as actuator in a deformable ring capable of locomotion is studied. Such a deformable ring moves as a result of gravitational force acting on its body when its shape changes. It can be used in exploration, search and rescue missions in future, where using conventional robots with rigid bodies and actuators is impossible. Large deformation induced by small stimulating voltage, low stiffness the sensing characteristics that in future work can be used in feedback control make IPMC a good choice for such an application. In this work first a model for IPMC is introduce that can be used in simulating deformation of IPMC in different... 

    Motion of deformable ring made of IPMC

    , Article Proceedings of SPIE - The International Society for Optical Engineering ; Volume 8409 , 2012 ; 0277786X (ISSN); 9780819490872 (ISBN) Firouzeh, A ; Alasty, A ; Ozmaeian, M ; National Institute of Standards and Technology; Asia Pacific Committee of Smart and Nano Materials; Nanyang Technol. Univ., Adv. Mater. Res. Cent.; The National Natural Science Foundation of China; Chinese Society of Composite Materials ; Sharif University of Technology
    2012
    Abstract
    In this paper application of Ionic Polymer Metal Composite (IPMC) as actuator in a deformable ring capable of locomotion is studied. Such a deformable ring moves as a result of gravitational force acting on its body when its shape changes. It can be used in exploration, search and rescue missions in future, where using conventional robots with rigid bodies and actuators is impossible. Large deformation induced by small stimulating voltage, low stiffness the sensing characteristics that in future work can be used in feedback control make IPMC a good choice for such an application. In this work first a model for IPMC is introduce that can be used in simulating deformation of IPMC in different... 

    Flux and color variations of the quadruply imaged quasar HE 0435-1223

    , Article Astronomy and Astrophysics ; Volume 528 , April , 2011 ; 00046361 (ISSN) Ricci, D ; Poels, J ; Elyiv, A ; Finet, F ; Sprimont, P. G ; Anguita, T ; Bozza, V ; Browne, P ; Burgdorf, M ; Calchi Novati, S ; Dominik, M ; Dreizler, S ; Glitrup, M ; Grundahl, F ; Harpsøe, K ; Hessman, F ; Hinse, T. C ; Hornstrup, A ; Hundertmark, M ; Jørgensen, U. G ; Liebig, C ; Maier, G ; Mancini, L ; Masi, G ; Mathiasen, M ; Rahvar, S ; Scarpetta, G ; Skottfelt, J ; Snodgrass, C ; Southworth, J ; Teuber, J ; Thöne, C. C ; Wambsganß, J ; Zimmer, F ; Zub, M ; Surdej, J ; Sharif University of Technology
    Abstract
    Aims: We present VRi photometric observations of the quadruply imaged quasarHE0435-1223, carried out with the Danish 1.54 m telescope at the La Silla Observatory. Our aim was to monitor and study the magnitudes and colors of each lensed component as a function of time. Methods. We monitored the object during two seasons (2008 and 2009) in the VRi spectral bands, and reduced the data with two independent techniques: difference imaging and point spread function (PSF) fitting. Results. Between these two seasons, our results show an evident decrease in flux by ≈ 0.2-0.4 magnitudes of the four lensed components in the three filters. We also found a significant increase (≈ 0.05-0.015) in their V -... 

    Data Analysis of MOA for Gravitational Microlensing Events with Durations Less than 2 Days by Using Brown Dwarfs Population

    , M.Sc. Thesis Sharif University of Technology Hassani, Sheida (Author) ; Rahvar, Sohrab (Supervisor)
    Abstract
    Gravitational Microlensing is one of the most powerful methods of detecting very low mass objects like Exoplanets and Brown dwarfs. The most important parameter that we can extract from a microlensing event is Einstein radius crossing time t_E. In this thesis, with performing Monte-Carlo simulation, we will obtain t_E distribution for brown dwarf population. Then we will show that this population can be a good candidate for very short microlensing events with t_E<2 days. The data set used in this analysis was taken in 2006 and 2007 seasons by the MOA-II survey, with the 1.8-m MOA-II telescope located at the Mt. John University Observatory, New Zealand  

    Wave Optics Effects in Microlensing of a Binary Lenses

    , Ph.D. Dissertation Sharif University of Technology Mehrabi Rahmanpour, Ahmad (Author) ; Rahvar, Sohrab (Supervisor)
    Abstract
    In this thesis, we investigate two subjects in gravitational microlensing. In first part we study wave optics effect in light curve of a binary system. Gravitational lensing occurs when light deflects in a gravitational field. This deflection produces multi-images from real one. In microlensing regime, images can not be detected separately and gravitational lensing appears as magnifying source’s flux . Microlensing has been studied mostly in geometric optics regime. At larger wavelengths, mostly at radio wavelengths, we expect to see the effects of wave optics in microlensing. Stars at radio wave are faint and to detect them we need a powerful radio telescope. In the near future, SKA (Square... 

    On the Concepts and Roles of Energy and Entropyin Gravitational Physics and Cosmology(Canonical Approaches in Definition of Conserved Quantities in Gravitational Physics)

    , Ph.D. Dissertation Sharif University of Technology Aghapour Hasiri, Sajad (Author) ; Golshani, Mehdi (Supervisor) ; Jafari, Ghadir (Co-Supervisor)
    Abstract
    In this thesis, inspired by foundational discussions about the concepts of energy and entropy in the gravitational theory, we study the definitions of these concepts and the roles they play in that theory. The definitions considered in this thesis are derived from canonical formalism. To this end, first of all, the variational principle and the canonical structure in the gravitational theory, especially in situations where the spacetime is bounded, is carefully studied and the boundary and corner actions as well as the canonical structure on the boundaries in three cases of non-null, null and general boundaries are derived. Based on this study, two canonical approaches, namely the... 

    The Effect of Radiation Pressure on Dust and Gas Dynamics in Accretion Disks

    , M.Sc. Thesis Sharif University of Technology Mohammadi, Amir Hossein (Author) ; Rahvar, Sohrab (Supervisor)
    Abstract
    The purpose of this study is to investigate the effect of radiation pressure on accretion disks. The radiation density causes the separation of electrons from ions which leads to the creation of an internal electric dipole. In this study Radiation density is calculated using the Eddington limit. Afterwards radiation pressure is calculated with the use of collisions between photons and electrons in the plasma. Collisions are assumed to happen only between photons and electrons, due to the larger cross section of electrons compared to protons. The mentioned assumption causes the creation of an electric dipole and with it an internal electric field. The separation of the charges is assumed to... 

    Inclusive b-jet production in pp collisions at √s = 7 TeV

    , Article Journal of High Energy Physics ; Volume 2012, Issue 4 , 2012 ; 11266708 (ISSN) Chatrchyan, S ; Khachatryan, V ; Sirunyan, A. M ; Tumasyan, A ; Adam, W ; Bergauer, T ; Dragicevic, M ; Ero, J ; Fabjan, C ; Friedl, M ; Fruhwirth, R ; Ghete, V. M ; Hammer, J ; Hoch, M ; Hormann, N ; Hrubec, J ; Jeitler, M ; Kiesenhofer, W ; Krammer, M ; Liko, D ; Mikulec, I ; Pernicka, M ; Rahbaran, B ; Rohringer, C ; Rohringer, H ; Schöfbeck, R ; Strauss, J ; Taurok, A ; Teischinger, F ; Wagner, P ; Waltenberger, W ; Walzel, G ; Widl, E ; Wulz, C. E ; Mossolov, V ; Shumeiko, N ; Gonzalez, J. S ; Bansal, S ; Benucci, L ; Cornelis, T ; De Wolf, E. A ; Janssen, X ; Luyckx, S ; Maes, T ; Mucibello, L ; Ochesanu, S ; Roland, B ; Rougny, R ; Selvaggi, M ; Van Haevermaet, H ; Van Mechelen, P ; Van Remortel, N ; Van Spilbeeck, A ; Blekman, F ; Blyweert, S ; DHondt, J ; Suarez, R.G ; Kalogeropoulos, A ; Maes, M ; Olbrechts, A ; Van Doninck, W ; Van Mulders, P ; Van Onsem, G.P ; Villella, I ; Charaf, O ; Clerbaux, B ; De Lentdecker, G ; Dero, V ; Gay, A. P. R ; Hammad, G. H ; Hreus, T ; Leonard, A ; Marage, P. E ; Thomas, L ; Vander Velde, C ; Vanlaer, P ; Wickens, J ; Adler, V ; Beernaert, K ; Cimmino, A ; Costantini, S ; Garcia, G ; Grunewald, M ; Klein, B ; Lellouch, J ; Marinov, A ; Mccartin, J ; Rios, A. A. O ; Ryckbosch, D ; Strobbe, N ; Thyssen, F ; Tytgat, M ; Vanelderen, L ; Verwilligen, P ; Walsh, S ; Yazgan, E ; Zaganidis, N ; Basegmez, S ; Bruno, G ; Ceard, L ; De Favereau De Jeneret, J ; Delaere, C ; Du Pree, T ; Favart, D ; Forthomme, L ; Giammanco, A ; Grégoire, G ; Hollar, J ; Lemaitre, V ; Liao, J ; Militaru, O ; Nuttens, C ; Pagano, D ; Pin, A ; Piotrzkowski, K ; Schul, N ; Beliy, N ; Caebergs, T ; Daubie, E ; Alves, G. A ; Martins Jr., M. C ; De Jesus Damiao, D ; Martins, T ; Pol, M.E ; Souza, M. H. G ; Aldá Jr., W. L ; Carvalho, W ; Custódio, A ; Da Costa, E. M ; De Oliveira Martins, C ; De Souza, S. F ; Figueiredo, D. M ; Mundim, L ; Nogima, H ; Oguri, V ; Da Silva, W. L. P ; Santoro, A ; Do Amaral, S. M. S ; Jorge, L. S ; Sznajder, A. A ; Anjos, T. S ; Bernardes, C. A ; Dias, F. A ; Tomei, T. R. F. P ; Gregores, E. M ; Lagana, C ; Marinho, F ; Mercadante, P. G ; Novaes, S. F ; Padula, S. S ; Genchev, V ; Iaydjiev, P ; Piperov, S ; Rodozov, M ; Stoykova, S ; Sultanov, G ; Tcholakov, V ; Trayanov, R ; Vutova, M ; Dimitrov, A ; Hadjiiska, R ; Karadzhinova, A ; Kozhuharov, V ; Litov, L ; Pavlov, B ; Petkov, P ; Bian, J. G ; Chen, G. M ; Chen, H. S ; Jiang, C. H ; Liang, D ; Liang, S ; Meng, X ; Tao, J ; Wang, J ; Wang, J ; Wang, X ; Wang, Z ; Xiao, H ; Xu, M ; Zang, J ; Zhang, Z ; Asawatangtrakuldee, C ; Ban, Y ; Guo, S ; Guo, Y ; Li, W ; Liu, S ; Mao, Y ; Qian, S. J ; Teng, H ; Wang, S ; Zhu, B ; Zou, W ; Cabrera, A ; Gomez Morenon,B ; Osorio Oliveros, A. F ; Sanabria, J. C ; Godinovic, N ; Lelas, D ; Plestina, R ; Polic, D ; Puljak, I ; Antunovic, Z ; Dzelalija, M ; Kovac, M ; Brigljevic, V ; Duric, S ; Kadija, K ; Luetic, J ; Morovic, S ; Attikis, A ; Galanti, M ; Mousa, J ; Nicolaou, C ; Ptochos, F ; Razis, P. A ; Finger, M ; Finger Jr., M ; Assran, Y ; Kamel, A. E ; Khalil, S ; Mahmoud, M. A ; Radi, A ; Hektor, A ; Kadastik, M ; Müntel, M ; Raidal, M ; Rebane, L ; Tiko, A ; Azzolini, V ; Eerola, P ; Fedi, G ; Voutilainen, M ; Czellar, S ; Harkonen, J ; Heikkinen, A ; Karimaki, V ; Kinnunen, R ; Kortelainen, M. J ; Lampen, T ; Lassila Perini, K ; Lehti, S ; Linden, T ; Luukka, P ; Mäenpaa, T ; Peltola, T ; Tuominen, E ; Tuominiemi, J ; Tuovinen, E ; Ungaro, D ; Wendland, L ; Banzuzi, K ; Korpela, A ; Tuuva, T ; Sillou, D ; Besancon, M ; Choudhury, S ; Dejardin, M ; Denegri, D ; Fabbro, B ; Faure, J. L ; Ferri, F ; Ganjour, S ; Givernaud, A ; Gras, P ; De Monchenault, G. H ; Jarry, P ; Locci, E ; Malcles, J ; Millischer, L ; Rander, J ; Rosowsky, A ; Shreyber, I ; Titov, M ; Baffioni, S ; Beaudette, F ; Benhabib, L ; Bianchini, L ; Bluj, M ; Broutin, C ; Busson, P ; Charlot, C ; Daci, N ; Dahms, T ; Dobrzynski, L ; Elgammal, S ; De Cassagnac, R. G ; Haguenauer, M ; Mine, P ; Mironov, C ; Ochando, C ; Paganini, P ; Sabes, D ; Salerno, R ; Sirois, Y ; Thiebaux, C ; Veelken, C ; Zabi, A ; Agram, J. L ; Andrea, J ; Bloch, D ; Bodin, D ; Brom, J. M ; Cardaci, M ; Chabert, E. C ; Collard, C ; Conte, E ; Drouhin, F ; Ferro, C ; Fontaine, J.-C ; Gele, D ; Goerlach, U ; Juillot, P ; Karim, M ; Le Bihan, A. C ; Van Hove, P ; Fassi, F ; Mercier, D ; Baty, C ; Beauceron, S ; Beaupere, N ; Bedjidian, M ; Bondu, O ; Boudoul, G ; Boumediene, D ; Brun, H ; Chasserat, J ; Chierici, R ; Contardo, D ; Depasse, P ; El Mamouni, H ; Falkiewicz, A ; Fay, J ; Gascon, S ; Gouzevitch, M ; Ille, B ; Kurca, T ; Le Grand, T ; Lethuillier, M ; Mirabito, L ; Perries, S ; Sordini, V ; Tosi, S ; Tschudi, Y ; Verdier, P ; Viret, S ; Lomidze, D ; Anagnostou, G ; Beranek, S ; Edelhoff, M ; Feld, L ; Heracleous, N ; Hindrichs, O ; Jussen, R ; Klein, K ; Merz, J ; Ostapchuk, A ; Perieanu, A ; Raupach, F ; Sammet, J ; Schael, S ; Sprenger, D ; Weber, H ; Wittmer, B ; Zhukov, V ; Ata, M ; Caudron, J ; Dietz Laursonn, E ; Erdmann, M ; Guth, A ; Hebbeker, T ; Heidemann, C ; Hoepfner, K ; Klimkovich, T ; Klingebiel, D ; Kreuzer, P ; Lanskey, D ; Lingemann, J ; Magass, C ; Merschmeyer, M ; Meyer, A ; Olschewski, M ; Papacz, P ; Pieta, H ; Reithler, H ; Schmitz, S. A ; Sonnenschein, L ; Steggemann, J ; Teyssier, D ; Weber, M ; Bontenackels, M ; Cherepanov, V ; Davids, M ; Flügge, G ; Geenen, H ; Geisler, M ; Ahmad, W. H ; Hoehle, F ; Kargoll, B ; Sharif University of Technology
    2012
    Abstract
    The inclusive b-jet production cross section in pp collisions at a center-ofmass energy of 7TeV is measured using data collected by the CMS experiment at the LHC. The cross section is presented as a function of the jet transverse momentum in the range 18 < pT < 200 GeV for several rapidity intervals. The results are also given as the ratio of the b-jet production cross section to the inclusive jet production cross section. The measurement is performed with two different analyses, which differ in their trigger selection and b-jet identification: a jet analysis that selects events with a b jet using a sample corresponding to an integrated luminosity of 34 pb -1, and a muon analysis requiring a... 

    OGLE-2014-BLG-1186: Gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?

    , Article Monthly Notices of the Royal Astronomical Society ; Volume 484, Issue 4 , 2019 , Pages 5608-5632 ; 00358711 (ISSN) Dominik, M ; Bachelet, E ; Bozza, V ; Street, R. A ; Han, C ; Hundertmark, M ; Udalski, A ; Bramich, D. M ; Alsubai, K. A ; Calchi Novati, S ; Ciceri, S ; D'Ago, G ; Figuera Jaimes, R ; Haugbølle, T ; Hinse, T. C ; Horne, K ; Jørgensen, U. G ; Juncher, D ; Kains, N ; Korhonen, H ; Mancini, L ; Menzies, J ; Popovas, A ; Rabus, M ; Rahvar, S ; Scarpetta, G ; Schmidt, R ; Skottfelt, J ; Snodgrass, C ; Southworth, J ; Starkey, D ; Steele, I. A ; Surdej, J ; Tsapras, Y ; Wambsganss, J ; Wertz, O ; Pietrukowicz, P ; Szymanski, M. K ; Mróz, P ; Skowron, J ; Soszynski, I ; Ulaczyk, K ; Poleski, R ; Wyrzykowski, Ł ; Kozłowski, S ; Sharif University of Technology
    Oxford University Press  2019
    Abstract
    Discussing the particularly long gravitational microlensing event OGLE-2014-BLG-1186 with a time-scale tE ∼ 300 d, we present a methodology for identifying the nature of localised deviations from single-lens point-source light curves, which ensures that (1) the claimed signal is substantially above the noise floor, (2) the inferred properties are robustly determined and their estimation is not subject to confusion with systematic noise in the photometry, (3) alternative viable solutions within the model framework are not missed. Annual parallax and binarity could be separated and robustly measured from the wing and the peak data, respectively. We find matching model light curves that involve... 

    Constraining galactic models through parallax and astrometry of microlensing events

    , Article Astronomy and Astrophysics ; Volume 438, Issue 1 , 2005 , Pages 153-157 ; 00046361 (ISSN) Rahvar, S ; Ghassemi, S ; Sharif University of Technology
    2005
    Abstract
    Various models for the Galactic distribution of massive compact halo objects (MACHOs) have been proposed for the interpretation of microlensing toward the Large Magellanic Cloud (LMC). A direct way to fit the best model is by measuring the lens parameters, which can be obtained by measuring the Einstein crossing time and the parallax effect on the microlensing light curve and by astrometry of centroids of images. In this work, the theoretical distribution of these parameters is obtained for the various power-law Galactic dark halo models and MACHO mass functions (MF). For self-lensing as one of the models for the interpretation of LMC events, the maximum shift of image centroids and the... 

    Multiobjective optimal reactive power dispatch and voltage control: A new opposition-based self-adaptive modified gravitational search algorithm

    , Article IEEE Systems Journal ; Volume 7, Issue 4 , 2013 , Pages 742-753 ; 19328184 (ISSN) Niknam, T ; Narimani, M. R ; Azizipanah Abarghooee, R ; Bahman Firouzi, B ; Sharif University of Technology
    2013
    Abstract
    This paper presents a novel opposition-based self-adaptive modified gravitational search algorithm (OSAMGSA) for optimal reactive power dispatch and voltage control in power-system operation. The problem is formulated as a mixed integer, nonlinear optimization problem, which has both continuous and discrete control variables. In order to achieve the optimal value of loss, voltage deviation, and voltage stability index, it is necessary to find the optimal value of control variables such as the tap positions of tap changing transformers, generator voltages, and compensation capacitor. Therefore, this complicated problem needs to be solved by an accurate optimization algorithm. This paper... 

    Propagation of light in Schwarzschild geometry

    , Article Proceedings of SPIE - The International Society for Optical Engineering, 25 January 2010 through 28 January 2010 ; Volume 7597 , 2010 ; 0277786X (ISSN) ; 9780819479938 (ISBN) Khorasani, S ; Sharif University of Technology
    2010
    Abstract
    In this paper, the equivalent medium of Schwarzschild metric is discussed. The corresponding ray-tracing equations are integrated for the equivalent medium of the Schwarzschild geometry, which describes the curved space around a spherically symmetric, irrotational, and uncharged blackhole. We make comparison to the well-known expression by Einstein. While Einstein's estimate is reasonably good for large closest distances of approach to the star, it disregards the optical anisotropy of space. Instead, Virbhadra's estimate which takes the effects of anisotropy of Schwarzschild metric is shown to be more consistent with numerical simulations. Hence, a true physical anisotropy in the velocity of... 

    A nonlinear model predictive controller based on the gravitational search algorithm

    , Article Optimal Control Applications and Methods ; Volume 42, Issue 6 , 2021 , Pages 1734-1761 ; 01432087 (ISSN) Nobahari, H ; Alizad, M ; Nasrollahi, S ; Sharif University of Technology
    John Wiley and Sons Ltd  2021
    Abstract
    A heuristic nonlinear model predictive controller is proposed, based on the gravitational search algorithm. The proposed method models a constrained nonlinear model predictive control problem in the form of a dynamic optimization and uses a set of virtual particles, moving within the search space, to find the best control sequence in an online manner. Particles affect the movement of each other through the gravitational forces. The optimality of the points, experienced by the particles, is evaluated by a cost function. This function reduces the tracking error, control effort, and control chattering. The better control sequence a particle finds, the more mass is assigned to that particle....