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相关论文: Primordial black holes as dark matter and gravitat…

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We investigate a new mechanism to create large curvature perturbations on small scales due to parameter resonance in a single-field inflationary model with a small periodic structure upon the potential. After reentering the horizon, the…

宇宙学与河外天体物理 · 物理学 2020-06-17 Rong-Gen Cai , Zong-Kuan Guo , Jing Liu , Lang Liu , Xing-Yu Yang

We devise a novel mechanism and for the first time demonstrate that the Higgs model in particle physics can drive the inflation to satisfy the cosmic microwave background observations and simultaneously enhance the curvature perturbations…

广义相对论与量子宇宙学 · 物理学 2021-04-07 Zhu Yi , Yungui Gong , Bin Wang , Zong-hong Zhu

We show that resonant processes during multi-field inflation can generate a large curvature perturbation on small scales. This perturbation naturally leads to the formation of primordial black holes that may constitute dark matter, as well…

宇宙学与河外天体物理 · 物理学 2025-12-05 Yuma S. Furuta , Mindaugas Karčiauskas , Kazunori Kohri , Alejandro Sáez

Primordial black holes as dark matter may be generated in single-field models of inflation thanks to the enhancement at small scales of the comoving curvature perturbation. This mechanism requires leaving the slow-roll phase to enter a…

宇宙学与河外天体物理 · 物理学 2018-07-26 Matteo Biagetti , Gabriele Franciolini , Alex Kehagias , Antonio Riotto

We study the formation of primordial black holes and the generation of gravitational waves in a class of cosmological models that are direct supersymmetric analogs of the observationally favored nonminimally coupled Higgs inflation model.…

宇宙学与河外天体物理 · 物理学 2023-03-01 Shinsuke Kawai , Jinsu Kim

We present a novel model-independent generic mechanism for primordial black hole formation within the context of non-singular matter bouncing cosmology. In particular, considering a short duration transition from the matter contracting…

广义相对论与量子宇宙学 · 物理学 2024-06-21 Theodoros Papanikolaou , Shreya Banerjee , Yi-Fu Cai , Salvatore Capozziello , Emmanuel N. Saridakis

The possibility that dark matter could be primordial black holes is discussed with an emphasis on the most commonly studied inflationary dynamics that could have produced them.

宇宙学与河外天体物理 · 物理学 2025-02-20 Guillermo Ballesteros

Primordial black holes can be produced by a long range attractive fifth force stronger than gravity, mediated by a light scalar field interacting with nonrelativistic "heavy" particles. As soon as the energy fraction of heavy particles…

宇宙学与河外天体物理 · 物理学 2018-04-25 Luca Amendola , Javier Rubio , Christof Wetterich

We propose that the totality of dark matter in the universe might ascribe its origin to one of the key properties of cosmological inflation, that it may be eternal: regions that at the end of the primordial accelerated expansion of the…

宇宙学与河外天体物理 · 物理学 2026-02-10 G. Franciolini , M. Peloso , A. Riotto

With the direct discovery of gravitational waves, black holes have regain interest in the recent years. In particular primordial black holes (PBHs), which originate from the very early Universe, may constitute (at least in part) dark…

广义相对论与量子宇宙学 · 物理学 2024-05-15 Alexandre Arbey

The next generation of space-borne gravitational wave detectors may detect gravitational waves from extreme mass-ratio inspirals with primordial black holes. To produce primordial black holes which contribute a non-negligible abundance of…

宇宙学与河外天体物理 · 物理学 2018-07-04 Haoran Di , Yungui Gong

We show that primordial black holes - in the observationally allowed mass window with $f_{\rm pbh}=1$ - formed from late nucleating patches in a first order phase transition imply upcoming gravitational wave interferometers will see a large…

高能物理 - 唯象学 · 物理学 2024-01-26 Iason Baldes , María Olalla Olea-Romacho

The local primordial density fluctuations caused by quantum vacuum fluctuations during inflation grow into stars and galaxies in the late universe and, if they are large enough, also produce primordial black holes. We study the formation of…

广义相对论与量子宇宙学 · 物理学 2025-12-22 Neven Bilić , Dragoljub D. Dimitrijević , Goran S. Djordjevic , Milan Milošević , Marko Stojanović

We show that fragmentation of the inflaton into long-lived spatially localized oscillon configurations can lead to copious production of black holes. In a single-field inflation model primordial black holes of sublunar mass can form, and…

宇宙学与河外天体物理 · 物理学 2018-10-12 Eric Cotner , Alexander Kusenko , Volodymyr Takhistov

We investigate a possibility of primordial black hole (PBH) formation with a hierarchical mass spectrum in multiple phases of inflation. As an example, we find that one can simultaneously realize a mass spectrum which has recently attracted…

宇宙学与河外天体物理 · 物理学 2019-08-13 Yuichiro Tada , Shuichiro Yokoyama

Primordial black holes are a unique probe of the early Universe and offer a potential link between inflationary dynamics and dark matter. In a recent work \cite{Inui:2024fgk}, we analyse PBH formation and the associated stochastic…

宇宙学与河外天体物理 · 物理学 2025-04-28 Cristian Joana

The gravitational waves measured at LIGO are presumed here to come from merging primordial black holes. We ask how these primordial black holes could arise through inflationary models while not conflicting with current experiments. Among…

宇宙学与河外天体物理 · 物理学 2017-04-11 Nicholas Orlofsky , Aaron Pierce , James D. Wells

Primordial black holes are produced in a minimal UV extension to the Higgs inflation with an included $R^2$ term. We show that for parameters consistent with Standard Model measurements and Planck observation results lead to $M_{\rm PBH}…

高能物理 - 唯象学 · 物理学 2021-02-03 Dhong Yeon Cheong , Sung Mook Lee , Seong Chan Park

Primordial black holes (PBHs) are supposed to form from the collapse of over-densed regions generated by large scalar curvature perturbations in the radiation dominated era. Despite decades of various independent observations, the nature of…

星系天体物理 · 物理学 2021-08-31 Chen Yuan , Qing-Guo Huang

The NANOGrav Collaboration has recently published a strong evidence for a stochastic common-spectrum process that may be interpreted as a stochastic gravitational wave background. We show that such a signal can be explained by second-order…

宇宙学与河外天体物理 · 物理学 2021-02-03 V. De Luca , G. Franciolini , A. Riotto
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