Behrends–Fronsdal Spin Projection Operator in Space-Time with Arbitrary Dimension

Author(s):  
A. P. Isaev ◽  
M. A. Podoinitsyn
2001 ◽  
Vol 16 (04n06) ◽  
pp. 251-260
Author(s):  
S. FERRARA

Superconformal algebras in space–time of arbitrary dimension and signature are considered and their relation to super-Poincaré algebras outlined.


1974 ◽  
Vol 68 (1) ◽  
pp. 203-213 ◽  
Author(s):  
R. Grimm ◽  
S. Mǎrculescu

1993 ◽  
Vol 08 (25) ◽  
pp. 2413-2426 ◽  
Author(s):  
R. R. METSAEV

Using the light-cone formulation of relativistic dynamics we present a wide class of cubic interaction vertices for higher spin fields of any symmetry in arbitrary dimension of space-time. The solution is obtained in terms of generating function for interaction vertices.


2017 ◽  
Vol 310 ◽  
pp. 19-31 ◽  
Author(s):  
Randolph E. Bank ◽  
Panayot S. Vassilevski ◽  
Ludmil T. Zikatanov

1993 ◽  
Vol 08 (35) ◽  
pp. 3345-3348
Author(s):  
V. V. BELOKUROV ◽  
M. Z. IOFA

Ultraviolet divergencies in gauge theories including those with higher powers of covariant derivatives are discussed in a space-time of an arbitrary dimension. In particular, it is noted that in the case d=5 all the one-loop graphs are finite, and theories with sufficiently high power of derivatives are finite in all orders.


2006 ◽  
Vol 03 (04) ◽  
pp. 691-700 ◽  
Author(s):  
PAUL ALLEN ◽  
LARS ANDERSSON ◽  
JAMES ISENBERG

We consider the timelike minimal surface problem in Minkowski spacetimes and show local and global existence of such surfaces having arbitrary dimension ≥ 2 and arbitrary co-dimension, provided they are initially close to a flat plane.


2002 ◽  
Vol 17 (30) ◽  
pp. 1979-1989 ◽  
Author(s):  
JE-AN GU ◽  
W.-Y. P. HWANG

We study the spontaneous symmetry breaking (SSB) induced by a scalar field and its non-minimal interaction with gravity in the space–time of an arbitrary dimension (D > 2), where the gravitational field is treated as a dynamical field. We explore mainly the possibility of implementing SSB after introducing the non-minimal coupling with such dynamical gravitational field.


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