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Related papers: Classical Decay Rates of Oscillons

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The heavy and superheavy elements of the periodic table predominately disintegrate by {\alpha}-decay, facilitating transitions mainly between ground states and occasionally involving isomeric states. This study focuses on estimating the…

Nuclear Theory · Physics 2025-09-19 A. Jain , M. Imran , G. Saxena

Cosmological issues of the gravitino production by the decay of a heavy scalar field $X$ are examined, assuming that the damped coherent oscillation of the scalar once dominates the energy of the universe. The coupling of the scalar field…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takehiko Asaka , Shuntaro Nakamura , Masahiro Yamaguchi

In Class. Quantum Grav. 26 (2009) 175006 (arXiv:0812.4333v3) Bizon et al discuss the power-law tail in the long-time evolution of a spherically symmetric self-gravitating massless scalar field in odd spatial dimensions. They derive explicit…

General Relativity and Quantum Cosmology · Physics 2010-04-30 Nikodem Szpak

Decay spectroscopy of the long-lived states in $^{186}$Tl has been performed at the ISOLDE Decay Station at ISOLDE, CERN. The $\alpha$ decay from the low-spin $(2^-)$ state in $^{186}$Tl was observed for the first time and a half-life of…

The fluctuation properties of nuclear giant resonance spectra are studied in the presence of continuum decay. The subspace of quasi-bound states is specified by one-particle one-hole and two-particle two-hole excitations and the continuum…

Nuclear Theory · Physics 2009-01-23 S. Drożdż , A. Trellakis , J. Wambach

Decay of a scalar condensate via interactions with (quasi-)particles is of interest to many fields in physics, including cosmology. In cosmology, the decay of an inflaton condensate leads to the production of daughter particles and…

High Energy Physics - Phenomenology · Physics 2026-04-03 Ayuki Kamada , Kodai Sakurai

In the analysis of highly-oscillatory evolution problems, it is commonly assumed that a single frequency is present and that it is either constant or, at least, bounded from below by a strictly positive constant uniformly in time. Allowing…

Numerical Analysis · Mathematics 2018-07-23 Philippe Chartier , Mohammed Lemou , Florian Méhats , Gilles Vilmart

We explain simple semi-classical rules to estimate the lifetime of any given highly-excited quantum state of the string spectrum in flat spacetime. We discuss both the decays by splitting into two massive states and by massless emission. As…

High Energy Physics - Theory · Physics 2024-05-21 Roberto Iengo , Jorge G. Russo

The exact decay rate for emission of massless minimally coupled scalar fields by a non-extremal black hole in 2+1 dimensions is obtained. At low energy, the decay rate into scalars with zero angular momentum is correctly reproduced within…

High Energy Physics - Theory · Physics 2009-10-30 D. Birmingham , I. Sachs , S. Sen

We obtain the precise decay rates of traveling wave for a class of nonlocal evolution equations arising in the theory of phase transitions. We also investigate the spectrum of the operator obtained by linearizing at such a traveling wave.…

Classical Analysis and ODEs · Mathematics 2011-05-23 Guangyu Zhao , Shigui Ruan

In contrast to the complex $\phi^4$ model, vortex-antivortex collisions in the complex $\phi^6$ theory reveal a resonant structure due to the existence of a remarkably stable, long-lived, large amplitude oscillon in the broken vacuum.…

High Energy Physics - Theory · Physics 2026-03-31 D. Canillas Martínez , A. González-Parra , D. Miguélez-Caballero , A. Wereszczynski

We study the stabilization and the wellposedness of solutions of the wave equation with subcritical semilinearities and locally distributed nonlinear dissipation. The novelty of this paper is that we deal with the difficulty that the main…

Chiral cosmic string loop tends to the stationary (vorton) configuration due to the energy loss into the gravitational and electromagnetic radiation. We describe the asymptotic behaviour of near stationary chiral loops and their fading to…

High Energy Physics - Phenomenology · Physics 2009-11-07 Eugeny Babichev , Vyacheslav Dokuchaev

We explore the fate of the universe given the possibility that the density associated with `dark energy' may decay slowly with time. Decaying dark energy is modeled by a homogeneous scalar field which couples minimally to gravity and whose…

Astrophysics · Physics 2009-11-07 Ujjaini Alam , Varun Sahni , A. A. Starobinsky

We show that axion stars formed from axions with nearly Planck-scale decay constants $f$ are unstable to decay, and are unlikely to have phenomenological consequences. More generally, we show how results at smaller $f$ cannot be naively…

High Energy Physics - Phenomenology · Physics 2021-06-23 Joshua Eby , Lauren Street , Peter Suranyi , L. C. R. Wijewardhana

Long-lived heavy particles present during the big bang could have a decay channel opened by gravitons. Such decays can produce gravitational waves with large enough abundance to be detectable, and a peculiar narrow spectrum peaked today…

High Energy Physics - Phenomenology · Physics 2025-03-20 Giacomo Landini , Alessandro Strumia

We report the phenomenon of coherent super decay, where a linear sum of several damped oscillators can collectively decay much faster than the individual ones in the first stage, followed by stagnating ones after more than 90 percent of the…

Applied Physics · Physics 2018-12-04 Ka Yan Au Yeung , Brian Yang , Liang Sun , Kehang Bai , Z. Yang

We study a rapidly-oscillating scalar field with potential $V(\phi) = k|\phi|^n$ nonminally coupled to the Ricci scalar $R$ via a term of the form $(1- 8 \pi G_0 \xi \phi^2) R$ in the action. In the weak coupling limit, we calculate the…

General Relativity and Quantum Cosmology · Physics 2018-01-31 Dan Li , Shi Pi , Robert J. Scherrer

We investigate the asymptotic tail behavior of massive scalar fields in Schwarzschild background. It is shown that the oscillatory tail of the scalar field has the decay rate of $t^{-5/6}$ at asymptotically late times, and the oscillation…

General Relativity and Quantum Cosmology · Physics 2007-10-02 Hiroko Koyama , Akira Tomimatsu

We numerically evolve spherically symmetric solutions to the linear wave equation on some expanding Friedmann-Lema\^itre-Robertson-Walker (FLRW) spacetimes and study the respective asymptotics for large times. We find a quantitative…

General Relativity and Quantum Cosmology · Physics 2026-02-17 Flavio Rossetti , Alex Vañó-Viñuales