Cauchy's problem and Huygens' principle for relativistic higher spin wave equations in an arbitrary curved space-time

1985 ◽  
Vol 17 (1) ◽  
pp. 15-38 ◽  
Author(s):  
Volkmar Wünsch
1973 ◽  
Vol 30 (3) ◽  
pp. 201-209 ◽  
Author(s):  
J. Madore ◽  
W. Tait

Symmetry ◽  
2019 ◽  
Vol 11 (1) ◽  
pp. 36 ◽  
Author(s):  
Valerio Faraoni

Fields of spin s ≥ 1 / 2 satisfying wave equations in a curved space obey the Huygens principle under certain conditions clarified by a known theorem. Here, this theorem is generalized to spin zero and applied to an inflaton field in de Sitter-like space, showing that tails of scalar radiation are an unavoidable physical feature. Requiring the absence of tails, on the contrary, necessarily implies an unnatural tuning between cosmological constant, scalar field mass, and coupling constant to the curvature.


1996 ◽  
Vol 37 (9) ◽  
pp. 4274-4291 ◽  
Author(s):  
Philippe Droz‐Vincent

1978 ◽  
Vol 9 (5) ◽  
pp. 387-392 ◽  
Author(s):  
A. P. Fordy

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