Matches in SemOpenAlex for { <https://semopenalex.org/work/W2892768713> ?p ?o ?g. }
- W2892768713 endingPage "728" @default.
- W2892768713 startingPage "715" @default.
- W2892768713 abstract "Abstract In this paper we study the qualitative dynamical evolution of atomic population imbalance and tunneling current between two Bose–Einstein condensate (BEC) interacting with each other in the presence of the intra- and inter-species collisions while the Rabi coupling between them is switched on, too. In particular, we consider the influence of dissipation process in our model to get more realized physical results. In this regard, to solve the Hamiltonian of the system, the Heisenberg operator method is used, by which the analytical solutions of the related differential equations are obtained. The population imbalance between the two BECs and the respected atomic tunneling current are then explicitly deduced for two initial state, i.e., number and coherent states in different conditions. The analytical as well as numerical results confirm the dependence of the mentioned quantities on the chosen initial state and the total number of atoms in the system which is in consistence with experimental observations. As is observed, a new kind of macroscopic quantum self-trapping (MQST) effect is also occurred in the population imbalance at certain conditions. Two distinct types of collapse-revival phenomena, depending on the relative strength of tunneling and collisional interactions, can be seen in the behavior of atomic population imbalance and tunneling current. Interestingly, collapse-revival phenomenon is disappeared in the intermediate regime and a new oscillatory step-like pattern is observed in the dynamics of the system." @default.
- W2892768713 created "2018-10-05" @default.
- W2892768713 creator A5008541539 @default.
- W2892768713 creator A5074821123 @default.
- W2892768713 date "2019-01-01" @default.
- W2892768713 modified "2023-10-16" @default.
- W2892768713 title "Dissipative evolution of two-mode Bose–Einstein condensate in the presence of nonlinear interactions: Heisenberg operator approach" @default.
- W2892768713 cites W1549085211 @default.
- W2892768713 cites W1644604237 @default.
- W2892768713 cites W1851420901 @default.
- W2892768713 cites W1963599007 @default.
- W2892768713 cites W1966992699 @default.
- W2892768713 cites W1972740052 @default.
- W2892768713 cites W1973406635 @default.
- W2892768713 cites W1977669849 @default.
- W2892768713 cites W1979743129 @default.
- W2892768713 cites W1986784134 @default.
- W2892768713 cites W1987838605 @default.
- W2892768713 cites W1991602497 @default.
- W2892768713 cites W1993826630 @default.
- W2892768713 cites W1994956962 @default.
- W2892768713 cites W1998157779 @default.
- W2892768713 cites W1998374617 @default.
- W2892768713 cites W2002468852 @default.
- W2892768713 cites W2011050002 @default.
- W2892768713 cites W2011842467 @default.
- W2892768713 cites W2012269360 @default.
- W2892768713 cites W2013883737 @default.
- W2892768713 cites W2017321175 @default.
- W2892768713 cites W2019062653 @default.
- W2892768713 cites W2019460814 @default.
- W2892768713 cites W2023777298 @default.
- W2892768713 cites W2025232537 @default.
- W2892768713 cites W2025363053 @default.
- W2892768713 cites W2026488334 @default.
- W2892768713 cites W2029333308 @default.
- W2892768713 cites W2033301349 @default.
- W2892768713 cites W2035176060 @default.
- W2892768713 cites W2040252582 @default.
- W2892768713 cites W2042608342 @default.
- W2892768713 cites W2043934058 @default.
- W2892768713 cites W2044444923 @default.
- W2892768713 cites W2054558389 @default.
- W2892768713 cites W2057010378 @default.
- W2892768713 cites W2057859588 @default.
- W2892768713 cites W2061309565 @default.
- W2892768713 cites W2062485010 @default.
- W2892768713 cites W2063045829 @default.
- W2892768713 cites W2064464534 @default.
- W2892768713 cites W2066163409 @default.
- W2892768713 cites W2068091367 @default.
- W2892768713 cites W2072452827 @default.
- W2892768713 cites W2077634892 @default.
- W2892768713 cites W2080739875 @default.
- W2892768713 cites W2080917542 @default.
- W2892768713 cites W2083823507 @default.
- W2892768713 cites W2084398895 @default.
- W2892768713 cites W2085177269 @default.
- W2892768713 cites W2085847765 @default.
- W2892768713 cites W2091008124 @default.
- W2892768713 cites W2091504440 @default.
- W2892768713 cites W2092020630 @default.
- W2892768713 cites W2110958255 @default.
- W2892768713 cites W2121254344 @default.
- W2892768713 cites W2123178714 @default.
- W2892768713 cites W2125867770 @default.
- W2892768713 cites W2132639490 @default.
- W2892768713 cites W2161753757 @default.
- W2892768713 cites W2292050036 @default.
- W2892768713 cites W2299339269 @default.
- W2892768713 cites W2498458003 @default.
- W2892768713 cites W2506356478 @default.
- W2892768713 cites W2735055545 @default.
- W2892768713 cites W2746378825 @default.
- W2892768713 cites W2964345672 @default.
- W2892768713 cites W3098787394 @default.
- W2892768713 cites W3104483578 @default.
- W2892768713 doi "https://doi.org/10.1016/j.physa.2018.09.110" @default.
- W2892768713 hasPublicationYear "2019" @default.
- W2892768713 type Work @default.
- W2892768713 sameAs 2892768713 @default.
- W2892768713 citedByCount "7" @default.
- W2892768713 countsByYear W28927687132019 @default.
- W2892768713 countsByYear W28927687132020 @default.
- W2892768713 countsByYear W28927687132021 @default.
- W2892768713 countsByYear W28927687132023 @default.
- W2892768713 crossrefType "journal-article" @default.
- W2892768713 hasAuthorship W2892768713A5008541539 @default.
- W2892768713 hasAuthorship W2892768713A5074821123 @default.
- W2892768713 hasConcept C101370240 @default.
- W2892768713 hasConcept C104317684 @default.
- W2892768713 hasConcept C111919701 @default.
- W2892768713 hasConcept C121332964 @default.
- W2892768713 hasConcept C158448853 @default.
- W2892768713 hasConcept C158622935 @default.
- W2892768713 hasConcept C17020691 @default.
- W2892768713 hasConcept C185592680 @default.
- W2892768713 hasConcept C37589322 @default.