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                 general relativity, quantum gravity, quantum 
                  mechanics, vacuum decay, Israel junction conditions, relativistic 
                  shells, WKB (semiclassical) approximation, quantum tunneling. 
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                 Project goals: 
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                 to give an effective Lagrangian description 
                  for the dynamics of spherically symmetric shells in general 
                  relativity that recovers the description in terms of Israel's 
                  junction conditions; to apply the above formalism to the problem 
                  of vacuum decay. 
                
                
                
                
                
                
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                 Project results: 
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                 determination of the dynamical quantities for 
                  a Lagrangian description of vacuum bubbles; computation of the 
                  limit of vanishing gravitational constant and of two cases of 
                  gravitational vacuum decay. 
                
                
                
                
                
                
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                 Short Description. 
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                  We propose an effective Lagrangian description for 
                    the dynamics of spherically symmetric shells in general 
                    relativity. The description is effective in the sense 
                    that it reproduces Israel's junction conditions in the spherically 
                    symmetric case. As shown in more detail elsewhere, 
                    the only remaining junction condition in the spherically symmetric 
                    case can be related with the superhamiltonian constraint of 
                    the system. 
                  To test the above formulation we apply it to three specific 
                    cases. In particular: 
                 
                
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we compute the flat spacetime limit,   , 
                      and show that we can reproduce the false vacuum decay amplitude 
                      in ordinary quantum field theory;  
                   
                  - we analyse the simplest example of gravitational vacuum 
                    fluctuation, computing the probability for the spontaneous 
                    nucleation in Minkowski spacetime;
 
                  - we compute a more complex example of gravitational vacuum 
                    fluctuation, namely the amplitude for inflationary bubble 
                    nucleation.
 
                 
                In our formalism and under the WKB approximation, all the above 
                  results can be obtained as the integral of the Euclidean momentum 
                  describing a tunneling process through an effective potential 
                  barrier that links two alllowed classical configurations. 
                As shown in all examples, the results obtained with our method 
                  are consistent with those obtained by other procedures in the 
                  literature. 
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