Localized bound states of fermions interacting via massive vector bosons

1990 ◽  
Vol 31 (3) ◽  
pp. 763-770 ◽  
Author(s):  
D. C. Ionescu ◽  
J. Reinhardt ◽  
B. Müller ◽  
W. Greiner ◽  
G. Soff
1999 ◽  
Vol 1999 (10) ◽  
pp. 012-012
Author(s):  
Peter H Fisher ◽  
Yoshi Uchida
Keyword(s):  

2018 ◽  
Vol 2018 ◽  
pp. 1-8
Author(s):  
Ganim Gecim ◽  
Yusuf Sucu

In this study, the Generalized Uncertainty Principle (GUP) effect on the Hawking radiation formed by tunneling of a massive vector boson particle from the 2+1 dimensional new-type black hole was investigated. We used modified massive vector boson equation based on the GUP. Then, the Hamilton-Jacobi quantum tunneling approach was used to work out the tunneling probability of the massive vector boson particle and Hawking temperature of the black hole. Due to the GUP effect, the modified Hawking temperature was found to depend on the black hole properties, on the AdS3 radius, and on the energy, mass, and total angular momentum of the tunneling massive vector boson. In the light of these results, we also observed that modified Hawking temperature increases by the total angular momentum of the particle while it decreases by the energy and mass of the particle and the graviton mass. Also, in the context of the GUP, we see that the Hawking temperature due to the tunneling massive vector boson is completely different from both that of the spin-0 scalar and that of the spin-1/2 Dirac particles obtained in the previous study. We also calculate the heat capacity of the black hole using the modified Hawking temperature and then discuss influence of the GUP on the stability of the black hole.


1984 ◽  
Vol 139 (4) ◽  
pp. 307-309 ◽  
Author(s):  
M. Veltman
Keyword(s):  

2012 ◽  
Vol 03 (07) ◽  
pp. 619-624
Author(s):  
Takehisa Fujita ◽  
Naohiro Kanda ◽  
Kazuhiro Tsuda

2021 ◽  
Vol 67 (3 May-Jun) ◽  
pp. 415
Author(s):  
R. Guerrero ◽  
R. Omar Rodríguez ◽  
F. Carreras

To confine vector bosons in the four dimensional sector of a domain wall spacetime, we propose a mechanism in which the interaction among vectors is propagated via the self-interaction of the scalar wall.  In the process, the vector acquires an asymptotic mass, defined by the bulk cosmological constant, and it ends up coupled to the wall by the tension of the brane. The mechanism is applied on the Randall Sundrum scenario and regular versions of it, and on singular domain walls. In any case, the  electrostatic potential between two charged particles is defined by both the vector state attached to the wall and a continuous tower of massive vector states that propagate freely along the scenario's extra dimension.


1988 ◽  
Vol 37 (2) ◽  
pp. 560-562 ◽  
Author(s):  
Marcela Carena ◽  
Carlos Wagner ◽  
Luis Masperi

1986 ◽  
Vol 91 (4) ◽  
pp. 398-409 ◽  
Author(s):  
R. M. Doria ◽  
A. W. Smith ◽  
J. A. Helayël-Neto ◽  
S. Pugnetti
Keyword(s):  

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