Matches in SemOpenAlex for { <https://semopenalex.org/work/W4287577041> ?p ?o ?g. }
- W4287577041 endingPage "A139" @default.
- W4287577041 startingPage "A139" @default.
- W4287577041 abstract "This paper investigates the various spherically symmetric wormhole solutions in the presence of tidal forces and applies numerous methods, such as test particle orbital dynamics, ray-tracing and microlensing. We make the theoretical predictions on the test particle orbital motion around the tidal wormholes with the use of normalized by $mathcal{L}^2$ effective potential. In order to obtain the ray-tracing images (of both geometrically thin and thick accretion disks, relativistic jets), we properly modify the open source $texttt{GYOTO}$ code with python interface. We applied this techniques to probe the accretion flows nearby the Schwarzschild-like and charged Reissner-Nordstrom (RS) wormholes (we assumed both charged RS wormhole and special case with the vanishing electromagnetic charge, namely Damour-Solodukhin (DS) wormhole). It was shown that the photon sphere for Schwarzschild-like wormhole presents for both thin and thick accretion disks and even for the vanishing tidal forces. Moreover, it was observed that $r_{mathrm{ph}}toinfty$ as $alphatoinfty$, which constraints $alpha$ parameter to be sufficiently small and positive in order to respect the EHT observations. On the other hand, for the case of RS wormhole, photon sphere radius shrinks as $Lambdatoinfty$, as it was predicted by the effective potential. In addition to the accretion disks, we as well probe the relativistic jets around two wormhole solutions of our consideration. Finally, with the help of star bulb microlensing, we approximate the radius of the wormhole shadow and as we found out, for Schild WH, $R_{mathrm{Sh}}approx r_0$ for ZTF and grows linearly with $alpha$. On the contrary, shadow radius for charged wormholes slowly decreases with the growing trend of DS parameter $Lambda$." @default.
- W4287577041 created "2022-07-25" @default.
- W4287577041 creator A5015654075 @default.
- W4287577041 creator A5021642439 @default.
- W4287577041 creator A5056852306 @default.
- W4287577041 creator A5079238899 @default.
- W4287577041 date "2022-09-01" @default.
- W4287577041 modified "2023-10-06" @default.
- W4287577041 title "Accretion flows around exotic tidal wormholes" @default.
- W4287577041 cites W1990678913 @default.
- W4287577041 cites W2000764548 @default.
- W4287577041 cites W2003872523 @default.
- W4287577041 cites W2017010109 @default.
- W4287577041 cites W2061955368 @default.
- W4287577041 cites W2075161427 @default.
- W4287577041 cites W2083102574 @default.
- W4287577041 cites W2090749997 @default.
- W4287577041 cites W2091261428 @default.
- W4287577041 cites W2102038740 @default.
- W4287577041 cites W2106642021 @default.
- W4287577041 cites W2109112103 @default.
- W4287577041 cites W2150401567 @default.
- W4287577041 cites W2172203136 @default.
- W4287577041 cites W2219142959 @default.
- W4287577041 cites W2252795400 @default.
- W4287577041 cites W2273892807 @default.
- W4287577041 cites W2297596203 @default.
- W4287577041 cites W2400200941 @default.
- W4287577041 cites W2517332908 @default.
- W4287577041 cites W2767609769 @default.
- W4287577041 cites W2797437121 @default.
- W4287577041 cites W2807642113 @default.
- W4287577041 cites W2809838409 @default.
- W4287577041 cites W2896600995 @default.
- W4287577041 cites W2936095933 @default.
- W4287577041 cites W2936349953 @default.
- W4287577041 cites W2937056002 @default.
- W4287577041 cites W2938000962 @default.
- W4287577041 cites W2939024351 @default.
- W4287577041 cites W2944879418 @default.
- W4287577041 cites W2974043736 @default.
- W4287577041 cites W2984697394 @default.
- W4287577041 cites W2990825672 @default.
- W4287577041 cites W3008226156 @default.
- W4287577041 cites W3018127985 @default.
- W4287577041 cites W3025620969 @default.
- W4287577041 cites W3095914820 @default.
- W4287577041 cites W3098333541 @default.
- W4287577041 cites W3100393621 @default.
- W4287577041 cites W3104409174 @default.
- W4287577041 cites W3105230895 @default.
- W4287577041 cites W3105509586 @default.
- W4287577041 cites W3105555647 @default.
- W4287577041 cites W3105588560 @default.
- W4287577041 cites W3106368228 @default.
- W4287577041 cites W3107883104 @default.
- W4287577041 cites W3111363137 @default.
- W4287577041 cites W3122229992 @default.
- W4287577041 cites W3126400039 @default.
- W4287577041 cites W3155468695 @default.
- W4287577041 cites W3169003210 @default.
- W4287577041 cites W3172509636 @default.
- W4287577041 cites W3179834643 @default.
- W4287577041 cites W3203465452 @default.
- W4287577041 cites W3203740869 @default.
- W4287577041 cites W4210573398 @default.
- W4287577041 cites W4220912582 @default.
- W4287577041 cites W776457703 @default.
- W4287577041 doi "https://doi.org/10.1051/0004-6361/202244358" @default.
- W4287577041 hasPublicationYear "2022" @default.
- W4287577041 type Work @default.
- W4287577041 citedByCount "2" @default.
- W4287577041 countsByYear W42875770412022 @default.
- W4287577041 crossrefType "journal-article" @default.
- W4287577041 hasAuthorship W4287577041A5015654075 @default.
- W4287577041 hasAuthorship W4287577041A5021642439 @default.
- W4287577041 hasAuthorship W4287577041A5056852306 @default.
- W4287577041 hasAuthorship W4287577041A5079238899 @default.
- W4287577041 hasBestOaLocation W42875770411 @default.
- W4287577041 hasConcept C115304011 @default.
- W4287577041 hasConcept C121332964 @default.
- W4287577041 hasConcept C125125069 @default.
- W4287577041 hasConcept C136125196 @default.
- W4287577041 hasConcept C147452769 @default.
- W4287577041 hasConcept C150846664 @default.
- W4287577041 hasConcept C178635117 @default.
- W4287577041 hasConcept C2776401274 @default.
- W4287577041 hasConcept C29013271 @default.
- W4287577041 hasConcept C37914503 @default.
- W4287577041 hasConcept C38652104 @default.
- W4287577041 hasConcept C41008148 @default.
- W4287577041 hasConcept C44870925 @default.
- W4287577041 hasConcept C74650414 @default.
- W4287577041 hasConceptScore W4287577041C115304011 @default.
- W4287577041 hasConceptScore W4287577041C121332964 @default.
- W4287577041 hasConceptScore W4287577041C125125069 @default.
- W4287577041 hasConceptScore W4287577041C136125196 @default.
- W4287577041 hasConceptScore W4287577041C147452769 @default.