Bautista, Teresa Dabholkar, Atish Erbin, Harold

A proper definition of the path integral of quantum gravity has been a long-standing puzzle because the Weyl factor of the Euclidean metric has a wrong-sign kinetic term. We propose a definition of two-dimensional Liouville quantum gravity with cosmological constant using conformal bootstrap for the timelike Liouville theory coupled to supercritica...

Paulos, Miguel F. Zan, Bernardo

We apply recently constructed functional bases to the numerical conformal bootstrap for 1D CFTs. We argue and show that numerical results in this basis converge much faster than the traditional derivative basis. In particular, truncations of the crossing equation with even a handful of components can lead to extremely accurate results, in oppositio...

Paulos, Miguel F. Zan, Bernardo

We apply recently constructed functional bases to the numerical conformal bootstrap for 1D CFTs. We argue and show that numerical results in this basis converge much faster than the traditional derivative basis. In particular, truncations of the crossing equation with even a handful of components can lead to extremely accurate results, in oppositio...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...

Abbar, Sajad Duan, Huaiyu Sumiyoshi, Kohsuke Takiwaki, Tomoya Volpe, Maria Cristina

The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations. It is believed that fast neutrino flavor transformation occurs in the region where the angular distributions of $\nu_e$ and $\bar\nu_e$ cross ea...