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相关论文: Catastrogenesis: DM, GWs, and PBHs from ALP string…

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We propose a new scenario for the formation of asteroid-mass primordial black holes (PBHs). Our mechanism is based on the annihilation of the string-wall network associated with the breaking of a $U(1)$ global symmetry into a discrete $Z_N$…

高能物理 - 唯象学 · 物理学 2023-07-04 Graciela B. Gelmini , Jonah Hyman , Anna Simpson , Edoardo Vitagliano

Axion-like particles (ALPs) are a compelling candidate for dark matter (DM), whose production is associated with the formation of a string-wall network. If walls bounded by strings persist, which requires the potential to have multiple…

高能物理 - 唯象学 · 物理学 2021-09-29 Graciela B. Gelmini , Anna Simpson , Edoardo Vitagliano

In post-inflation axion-like particle (ALP) models, a stable domain wall network forms if the model's potential has multiple minima. This system must annihilate before dominating the Universe's energy density, producing ALPs and…

高能物理 - 唯象学 · 物理学 2023-11-30 Graciela B. Gelmini , Jonah Hyman

The global $U_{PQ}(1)$ Peccei-Quinn (PQ) symmetry, proposed to resolve the strong CP problem, predicts the existence of the axion, a pseudo Nambu-Goldstone boson and a leading dark matter candidate. The spontaneous breaking of this symmetry…

高能物理 - 唯象学 · 物理学 2026-04-16 Ishan Swamy , Deobrat Singh

We study the formation of primordial black holes (PBHs) from density fluctuations due to supercooled phase transitions (PTs) triggered in an axion-like particle (ALP) model. We find that the mass of the PBHs is inversely correlated with the…

宇宙学与河外天体物理 · 物理学 2025-10-02 Angela Conaci , Luigi Delle Rose , P. S. Bhupal Dev , Anish Ghoshal

The primordial black holes (PBHs) play as a novel source to radiate light elementary particles of energies in the region of a few hundred MeV. We explore the possibility that the axion-like particles (ALPs) with mass less than 1 MeV are…

高能物理 - 唯象学 · 物理学 2022-12-07 Tong Li , Rui-Jia Zhang

We investigate the possibility that primordial black holes (PBHs) can be formed from large curvature perturbations generated during the waterfall phase transition in a hybrid inflation model driven by an axion-like particle (ALP) $\phi$.…

宇宙学与河外天体物理 · 物理学 2025-09-08 Waqas Ahmed , Anish Ghoshal , Umer Zubair

LIGO-Virgo collaboration has found black holes as heavy as $M \sim 30M_\odot$ through the detections of the gravitational waves emitted during their mergers. Primordial black holes (PBHs) produced by inflation could be an origin of such…

宇宙学与河外天体物理 · 物理学 2018-01-08 Keisuke Inomata , Masahiro Kawasaki , Kyohei Mukaida , Yuichiro Tada , Tsutomu T. Yanagida

Axion-like particles (ALPs) are pseudo Nambu-Goldstone bosons associated with spontaneously broken global symmetries incorporated in the Standard Model (SM) Lagrangian in many models beyond the SM. The existence of a light ALP is plausible…

高能物理 - 唯象学 · 物理学 2025-06-11 Shirin Chenarani , Mojtaba Mohammadi Najafabadi

We propose a mechanism to generate Primordial Black Holes (PBHs) which is independent of cosmological inflation and occurs slightly below the QCD phase transition. Our setup relies on the collapse of long-lived string-domain wall networks…

高能物理 - 唯象学 · 物理学 2019-03-27 Francesc Ferrer , Eduard Masso , Giuliano Panico , Oriol Pujolas , Fabrizio Rompineve

Primordial black holes (PBHs) can be produced in the very early Universe due to the large density fluctuations. The cosmic background of axion-like particles (ALPs) could be non-thermally generated by PBHs. In this paper, we investigate the…

宇宙学与河外天体物理 · 物理学 2026-01-27 Hai-Jun Li

The QCD axion can solve the Strong CP Problem and be the dark matter of our universe. If the PQ symmetry breaking scale associated with the axion is below the inflationary reheating temperature, axion strings and domain walls populate the…

高能物理 - 唯象学 · 物理学 2024-07-04 David I. Dunsky , Marius Kongsore

Axion like particles (ALPs), the pseudo Nambu-Goldstone bosons associated to the spontaneous breaking of global symmetry, have emerged as promising dark matter candidates. Conventionally, in the context of misalignment mechanism, the…

高能物理 - 唯象学 · 物理学 2024-05-07 Soumen Kumar Manna , Arunansu Sil

Primordial black holes (PBHs) are of fundamental interest in cosmology and astrophysics, and have received much attention as a dark matter candidate and as a potential source of gravitational waves. One possible PBH formation mechanism is…

宇宙学与河外天体物理 · 物理学 2020-08-13 Alexander C. Jenkins , Mairi Sakellariadou

We present a new mechanism for the primordial black hole (PBH) production within the QCD axion framework. We take the case where the Peccei-Quinn symmetry breaks during inflation, resulting in a $N_{\rm DW}=1$ string-wall network that…

高能物理 - 唯象学 · 物理学 2024-06-25 Shuailiang Ge , Jinhui Guo , Jia Liu

Primordial black holes (PBHs) are very appealing dark matter (DM) candidates. It is highly plausible though, should they exist, that they would not make up all of the DM. Several studies showed that if the rest of DM is made of thermal…

高能天体物理现象 · 物理学 2025-11-24 Julien Lavalle , Pierre Salati

Light primordial black holes (LPBHs) with masses in the range $10$~g~$\leq M_{\rm BH} \leq 10^9$~g, although they evaporate before Big Bang Nucleosynthesis, can play a significant role in the production of both dark matter and dark…

宇宙学与河外天体物理 · 物理学 2025-07-08 Marco Manno , Daniele Montanino

Models that produce Axion-Like-Particles (ALP) after cosmological inflation due to spontaneous $U(1)$ symmetry breaking also produce cosmic string networks. Those axionic strings lose energy through gravitational wave emission during the…

高能物理 - 唯象学 · 物理学 2023-12-21 Géraldine Servant , Peera Simakachorn

Non-perturbative gravitational effects induce explicit global symmetry breaking terms within axion models. These exponentially suppressed terms in the potential give a mass contribution to the axion-like particles (ALPs). In this work we…

高能物理 - 唯象学 · 物理学 2025-03-05 Dhong Yeon Cheong , Koichi Hamaguchi , Yoshiki Kanazawa , Sung Mook Lee , Natsumi Nagata , Seong Chan Park

If primordial black holes (PBHs) formed at the quark-hadron epoch, their mass must be close to the Chandrasekhar limit, this also being the characteristic mass of stars. If they provide the dark matter (DM), the collapse fraction must be of…

宇宙学与河外天体物理 · 物理学 2020-12-16 Bernard Carr , Sebastien Clesse , Juan García-Bellido
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