I show that cosmological bubble walls in the thin wall approximation are unstable to the creation of “barnacles ” – loci of different wall tension adjacent to regions filled with a third vacuum. Barnacle formation leads to the same observational consequences as the extensively studied bubble collision scenario, but occurs exponentially more often. The process is described by a saddle point of the thin wall action with two negative modes. 1 a
We consider two spatially flat Friedmann-Robertson-Walker spacetimes divided by a timelike thin shel...
We study collisions between pairs of bubbles nucleated in an ambient false vacuum. For the first ti...
This science report is based on a cooperative study with T. Mishima (Nihon University) and N. Yoshin...
We develop a theory of static Bogomol’nyi-Prasad-Sommerfield (BPS) domain walls in stringy landscape...
Bubble collisions and defect formation in a damping environment (Melfo, Alejandra; Ferrera, Antonio...
We develop a theory of static BPS domain walls in stringy landscape and present a large family of BP...
We assess the effects of a collision between two vacuum bubbles in the thin-wall limit. After descri...
We study the dynamics of cosmological phase transitions in the case of small velocities of bubble wa...
This paper examines the evolution of spherical bubbles in a vacuum for all possible values of the co...
The interior of a vacuum bubble in de Sitter space may give an open universe with sufficient homogen...
[[abstract]]Motivated by the discovery of a plenitude of metastable vacua in a string landscape and ...
INTRODUCTION In this work, we consider bubble dynamics in the context of cosmological phase transiti...
We comprehensively study the effects of bubble wall thickness and speed on the gravitational wave em...
We comprehensively study the effects of bubble wall thickness and speed on the gravitational wave em...
The rate and manner of vacuum decay are calculated in an explicit flux compactifica-tion, including ...
We consider two spatially flat Friedmann-Robertson-Walker spacetimes divided by a timelike thin shel...
We study collisions between pairs of bubbles nucleated in an ambient false vacuum. For the first ti...
This science report is based on a cooperative study with T. Mishima (Nihon University) and N. Yoshin...
We develop a theory of static Bogomol’nyi-Prasad-Sommerfield (BPS) domain walls in stringy landscape...
Bubble collisions and defect formation in a damping environment (Melfo, Alejandra; Ferrera, Antonio...
We develop a theory of static BPS domain walls in stringy landscape and present a large family of BP...
We assess the effects of a collision between two vacuum bubbles in the thin-wall limit. After descri...
We study the dynamics of cosmological phase transitions in the case of small velocities of bubble wa...
This paper examines the evolution of spherical bubbles in a vacuum for all possible values of the co...
The interior of a vacuum bubble in de Sitter space may give an open universe with sufficient homogen...
[[abstract]]Motivated by the discovery of a plenitude of metastable vacua in a string landscape and ...
INTRODUCTION In this work, we consider bubble dynamics in the context of cosmological phase transiti...
We comprehensively study the effects of bubble wall thickness and speed on the gravitational wave em...
We comprehensively study the effects of bubble wall thickness and speed on the gravitational wave em...
The rate and manner of vacuum decay are calculated in an explicit flux compactifica-tion, including ...
We consider two spatially flat Friedmann-Robertson-Walker spacetimes divided by a timelike thin shel...
We study collisions between pairs of bubbles nucleated in an ambient false vacuum. For the first ti...
This science report is based on a cooperative study with T. Mishima (Nihon University) and N. Yoshin...