Abstract
A four-dimensional induced Einstein-Kalb-Ramond theory with a conformally coupled Kalb-Ramond term is discussed. It is argued that the Kalb-Ramond field is difficult to interpret as an axion field from a dynamical point of view, and hence tends to be unstable. One can, however, apply Routh’s method to extract an effective action for the axion field. It is found that the Kalb-Ramond hair will turn the event horizon into a naked singularity. Such an exact solution is found and analyzed carefully.
| Original language | English |
|---|---|
| Pages (from-to) | 2244-2247 |
| Number of pages | 4 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 53 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 1996 Jan 1 |
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All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)
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Induced Einstein-Kalb-Ramond theory and the black hole. / Kao, W. F.; Dai, W. B.; Wang, Shang Yung; Chyi, Tzuu Kang; Lin, Shih-Yuin.
In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 53, No. 4, 01.01.1996, p. 2244-2247.Research output: Contribution to journal › Article
TY - JOUR
T1 - Induced Einstein-Kalb-Ramond theory and the black hole
AU - Kao, W. F.
AU - Dai, W. B.
AU - Wang, Shang Yung
AU - Chyi, Tzuu Kang
AU - Lin, Shih-Yuin
PY - 1996/1/1
Y1 - 1996/1/1
N2 - A four-dimensional induced Einstein-Kalb-Ramond theory with a conformally coupled Kalb-Ramond term is discussed. It is argued that the Kalb-Ramond field is difficult to interpret as an axion field from a dynamical point of view, and hence tends to be unstable. One can, however, apply Routh’s method to extract an effective action for the axion field. It is found that the Kalb-Ramond hair will turn the event horizon into a naked singularity. Such an exact solution is found and analyzed carefully.
AB - A four-dimensional induced Einstein-Kalb-Ramond theory with a conformally coupled Kalb-Ramond term is discussed. It is argued that the Kalb-Ramond field is difficult to interpret as an axion field from a dynamical point of view, and hence tends to be unstable. One can, however, apply Routh’s method to extract an effective action for the axion field. It is found that the Kalb-Ramond hair will turn the event horizon into a naked singularity. Such an exact solution is found and analyzed carefully.
UR - http://www.scopus.com/inward/record.url?scp=0000307924&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0000307924&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.53.2244
DO - 10.1103/PhysRevD.53.2244
M3 - Article
AN - SCOPUS:0000307924
VL - 53
SP - 2244
EP - 2247
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
SN - 1550-7998
IS - 4
ER -