Zobrazeno 1 - 10
of 195
pro vyhledávání: '"Casalderrey-Solana Jorge"'
Relativistic, charged, superheated bubbles may play an important role in neutron star mergers if first-order phase transitions are present in the phase diagram of Quantum Chromodynamics. We describe the properties of these bubbles in the hydrodynamic
Externí odkaz:
http://arxiv.org/abs/2406.14450
General Relativity predicts that the spacetime near a cosmological singularity undergoes an infinite number of chaotic oscillations between different Kasner epochs with rapid transitions between them. This so-called BKL behaviour persists in the pres
Externí odkaz:
http://arxiv.org/abs/2312.11643
Autor:
Attems Maximilian, Bea Yago, Casalderrey-Solana Jorge, Mateos David, Santos-Oliván Daniel, Sopuerta Carlos F., Triana Miquel, Zilhão Miguel
Publikováno v:
EPJ Web of Conferences, Vol 175, p 07030 (2018)
Ever since fast hydrodynamization has been observed in heavy ion collisions the understanding of the hot early out-of-equilibrium stage of such collisions has been a topic of intense research. We use the gauge/gravity duality to model the creation of
Externí odkaz:
https://doaj.org/article/0f8d8f402c33443188d68c044d4f784d
Neutron star mergers provide a unique laboratory for the study of strong-field gravity coupled to Quantum Chromodynamics in extreme conditions. The frequencies and amplitudes of the resulting gravitational waves encode invaluable information about th
Externí odkaz:
http://arxiv.org/abs/2210.03171
Gradient jet tomography in high-energy heavy-ion collisions utilizes the asymmetric transverse momentum broadening of a propagating parton in an inhomogeneous medium. Such broadening is studied within a path integral description of the evolution of t
Externí odkaz:
http://arxiv.org/abs/2204.05323
Autor:
Bea, Yago, Casalderrey-Solana, Jorge, Giannakopoulos, Thanasis, Jansen, Aron, Mateos, David, Sanchez-Garitaonandia, Mikel, Zilhão, Miguel
Publikováno v:
JHEP09(2022)008
Cosmological phase transitions can proceed via the nucleation of bubbles that subsequently expand and collide. The resulting gravitational wave spectrum depends crucially on the properties of these bubbles. We extend our previous holographic work on
Externí odkaz:
http://arxiv.org/abs/2202.10503
Publikováno v:
JHEP 10 (2022) 049
We study the production of gravitational waves by a thermalized plasma of $\mathcal N$=4 Supersymmetric Yang Mills matter. We focus on the large number of colors limit, $N_c\rightarrow \infty$, and compute the spectrum of gravitational waves both for
Externí odkaz:
http://arxiv.org/abs/2202.05241