01115nam a2200265 i 4500991001625969707536030521s1997 us b 001 0 eng d0312101686 (v. 2)b12174087-39ule_inst956.6The Armenian people from ancient to modern times /edited by Richard G. Hovannisian.New York :St. Martin's Press,1997XII, 493 p. ;22 cmV. 2: Foreign dominion to statehood: the fifteenth century to the twentieth centuryBibliografia: p. [445]-467. IndiciPopolo armenoStoriaArmeniaStoriaHovannisian, Richard G.Foreign dominion to statehood: the fifteenth century to the twentieth century.b1217408711-10-1221-05-03991001625969707536LE015 956 - 6712015000067562le007LE015-0305-E51.60-l- 01310.i1252095021-05-03Armenian people from ancient to modern times144890UNISALENTOle00721-05-03ma -engus 4104098nam 2200913z- 450 9910367746403321202102113-03921-765-8(CKB)4100000010106253(oapen)https://directory.doabooks.org/handle/20.500.12854/44151(oapen)doab44151(EXLCZ)99410000001010625320202102d2019 |y 0engurmn|---annantxtrdacontentcrdamediacrrdacarrierCosmological Inflation, Dark Matter and Dark EnergyMDPI - Multidisciplinary Digital Publishing Institute20191 online resource (236 p.)3-03921-764-X Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In addition, according to the rotation curve of galaxies, the existence of dark matter, which does not shine, is also suggested. If primordial gravitational waves are detected in the future, the mechanism for realizing inflation can be revealed. Moreover, there exist two main candidates for dark matter. The first is a new particle, the existence of which is predicted in particle physics. The second is an astrophysical object which is not found by electromagnetic waves. Furthermore, there are two representative approaches to account for the accelerated expansion of the current universe. One is to assume the unknown dark energy in general relativity. The other is to extend the gravity theory to large scales. Investigation of the origins of inflation, dark matter, and dark energy is one of the most fundamental problems in modern physics and cosmology. The purpose of this book is to explore the physics and cosmology of inflation, dark matter, and dark energy.and components common to several branches of physics and astronomyapparatusastronomical and space-research instrumentationBaryon Acoustic Oscillation (BAO)brans-dicke theorycomparative planetologycomposite dark matterCosmic Microwave Background (CMB) temperaturecosmo-particle physicscosmoligical parameterscosmological modelcosmological parameterscosmologydark atomsdark energyDark Energydark energy modeldark energy modelsdark matterDark Matterde Sitter vacuumdosmological parametersdynamical Chern-Simons modified gravityEinstein-Aether theory of gravityextragalactic objects and systemsfield theoryfundamental astronomygalactic rotation curveHawking radiationhigher dimension gauged super-gravity black holeHubble constanthyper-colorinstrumentsjunction conditionsloop quantum cosmologymemoryn/anormal galaxiesnull hypersurfacesparametrizationsparticle physicsproperties of specific particlesQCDquantum gravityquantum optical systemsquantum opticsquantum tunneling phenomenonscalar-tensor gravityspacetime symmetrystatistical analysisSupernovaeBamba Kazuharuauth1323469BOOK9910367746403321Cosmological Inflation, Dark Matter and Dark Energy3035588UNINA