Gravitational shine of dark domain walls

نویسندگان

چکیده

Cosmic domain walls are harmless, provided that their tension decreases with expansion of the Universe. This setup can be realized, if scale spontaneous symmetry breaking is induced dynamically through interaction hot primordial plasma. In case, wall attain large values in early Universe without any conflict observations. Owing to initial tension, these topological defects may serve as a powerful source gravitational waves. We make preliminary estimate wave spectrum and argue it distinct from produced by other sources, particular constant tension. The resulting signal range accessible Einstein Telescope, DECIGO, TianQin, LISA, IPTA, or SKA, field constituting very feebly coupled plasma has tiny self-interactions. particular, one consider this for role Dark Matter. discuss various Matter production mechanisms properties emitted waves associated them. find conventional freeze-out freeze-in lead perhaps unobservable frequency However, also possible at second order phase transition leading formation inverse transition, when get dissolved eventually. both cases, there essentially no lower bound on

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Interaction of gravitational waves with domain walls

We study the gravitational perturbations of thick domain walls. The refraction index and spin properties of the solutions interior to the wall are analyzed in detail. It is shown that the gravitational waves suffer a refraction process by domain walls. The reflection and transmission coefficients are derived in the thin wall limit. In relation to the spin content, it is shown that the ‘×’ helic...

متن کامل

Gravitational domain walls and p - brane distributions ∗

We review the main algebraic aspects that characterize and determine the domain wall solutions of maximal gauged supergravity in various spacetime dimensions by considering consistent truncations that retain a number of components in the diagonal of the coset space scalar manifold of the theory. Starting from the algebraic classification of domain walls in D = 4 gauged supergravity, we also der...

متن کامل

Interaction between gravitational waves and domain walls

We study the gravitational perturbations of thick domain walls. The refraction index and spin properties of the solutions interior to the wall are analyzed in detail. It is shown that the gravitational waves suffer a refraction process by domain walls. The reflection and transmission coefficients are derived in the thin wall limit. In relation to the spin content, it is shown that the “×” helic...

متن کامل

A Review of Gravitational Waves from Cosmic Domain Walls

In this contribution, we discuss the cosmological scenario where unstable domain walls are formed in the early universe and their late-time annihilation produces a significant amount of gravitational waves. After describing cosmological constraints on long-lived domain walls, we estimate the typical amplitude and frequency of gravitational waves observed today. We also review possible extension...

متن کامل

Evolution of light domain walls interacting with dark matter.

In this paper we discuss the evolution of domain walls generated in the early Universe considering, unlike the previous studies, an interaction between the walls and a major gaseous component of the dark matter. It is assumed that the walls can reflect the particles elastically and with a reAection coe%cient of unity. We discuss a toy Lagrangian that could give rise to such a phenomenon. In the...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Journal of Cosmology and Astroparticle Physics

سال: 2022

ISSN: ['1475-7516', '1475-7508']

DOI: https://doi.org/10.1088/1475-7516/2022/04/028