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相关论文: Anomalous Isotopes In Dark Atoms models

200 篇论文

Direct searches for dark matter lead to serious problems for simple models with stable neutral Weakly Interacting Massive Particles (WIMPs) as candidates for dark matter. A possibility is discussed that new stable quarks and charged leptons…

宇宙学与河外天体物理 · 物理学 2011-12-06 Maxim Yu. Khlopov

We produce giant helium dimers by photoassociation of metastable helium atoms in a magnetically trapped, ultracold cloud. The photoassociation laser is detuned red of the atomic $2^3S_1 - 2^3P_0 $ line and produces strong heating of the…

凝聚态物理 · 物理学 2009-11-10 J. Leonard , M. Walhout , A. P. Mosk , T. Mueller , M. Leduc , C. Cohen-Tannoudji

A cosmological model with anisotropic dark energy is analyzed. The amount of deviation from isotropy of the equation of state of dark energy, the skewness \delta, generates an anisotropization of the large-scale geometry of the Universe,…

宇宙学与河外天体物理 · 物理学 2011-06-28 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco

The MiniBooNE low-energy excess stands as an unexplained anomaly in short-baseline neutrino oscillation experiments. It has been shown that it can be explained in the context of dark sector models. Here, we provide an overview of the…

高能物理 - 唯象学 · 物理学 2025-01-31 Asli M. Abdullahi , Jaime Hoefken Zink , Matheus Hostert , Daniele Massaro , Silvia Pascoli

We present a study of inhomogeneous big bang nucleosynthesis with emphasis on transport phenomena. We combine a hydrodynamic treatment to a nuclear reaction network and compute the light element abundances for a range of inhomogeneity…

天体物理学 · 物理学 2016-08-30 Elina Keihanen

Positive results of dark matter searches in experiments DAMA/NaI and DAMA/LIBRA taken together with negative results of other groups can imply nontrivial particle physics solutions for cosmological dark matter. Stable particles with charge…

宇宙学与河外天体物理 · 物理学 2009-12-01 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeniy Yu. Soldatov

We study perturbations of black holes absorbing dark energy. Due to the accretion of dark energy, the black hole mass changes. We observe distinct perturbation behaviors for absorption of different forms of dark energy into the black holes.…

广义相对论与量子宇宙学 · 物理学 2009-03-19 Xi He , Bin Wang , Shao-Feng Wu , Chi-Yong Lin

In several processes of stellar nucleosynthesis, like the astrophysical gamma-process, nuclear reactions involving alpha particles play an important role. The description of these reactions necessitates the knowledge of the alpha-nucleus…

核实验 · 物理学 2024-06-04 Zs. Mátyus , Gy. Gyürky , P. Mohr , A. Angyal , Z. Halász , G. G. Kiss , Á Tóth , T. Szücs , Zs. Fülöp

The prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. We calculate direct neutron capture on the even-even isotopes $^{124-145}$Sn and $^{208-238}$Pb with energy levels, masses, and…

核理论 · 物理学 2008-11-26 T. Rauscher , R. Bieber , H. Oberhummer , K. -L. Kratz , J. Dobaczewski , P. Moller , M. M. Sharma

In the Coulomb field of nucleus cut off on it size, besides usual atomic states, there are additional ones. These anomalous states are deep (in the range of $10\,MeV$) in the Dirac sea and can exist solely during a macroscopic acceleration…

综合物理 · 物理学 2024-01-18 B. Ivlev

There has been renewed interest in the possibility that dark matter exists in the form of atoms, analogous to those of the visible world. An important input for understanding the cosmological consequences of dark atoms is their…

高能物理 - 唯象学 · 物理学 2014-02-26 James M. Cline , Zuowei Liu , Guy D. Moore , Wei Xue

We consider Big Bang Nucleosynthesis (BBN) with long lived charged massive particles. Before decaying, the long lived charged particle recombines with a light element to form a bound state like a hydrogen atom. This effect modifies the…

高能物理 - 唯象学 · 物理学 2008-11-26 Kazunori Kohri , Fumihiro Takayama

It is believed that there may have been a large number of black holes formed in the very early universe. These would have quantised masses. A charged ``elementary black hole'' (with the minimum possible mass) can capture electrons, protons…

广义相对论与量子宇宙学 · 物理学 2009-08-18 V. V. Flambaum , J. C. Berengut

We find constraints on heavy, stable, strongly interacting massive particles (X) from searches for anomalous nuclei containing them, formed during primordial nucleosynthesis. Using existing data, we obtain a limit on the abundance ratio…

高能物理 - 唯象学 · 物理学 2009-10-31 Rabindra N. Mohapatra , Vigdor L. Teplitz

High-energy nuclear collisions create an energy density similar to that of the universe microseconds after the Big Bang, and in both cases, matter and antimatter are formed with comparable abundance. However, the relatively short-lived…

核实验 · 物理学 2015-03-19 STAR Collaboration

Ultralight dark matter is a compelling dark matter candidate. In this work, we examine the impact of quadratically-coupled ultralight dark matter on the predictions of Big Bang Nucleosynthesis. The presence of ultralight dark matter can…

高能物理 - 唯象学 · 物理学 2023-03-30 Thomas Bouley , Philip Sørensen , Tien-Tien Yu

The abundances of the isotopes of the elements C, N and O are mainly affected by the cold CNO cycles in non-explosive stellar situations, or by the hot CNO chains that can develop in certain explosive sites, like classical novae. Helium…

天体物理学 · 物理学 2007-05-23 M. Arnould , L. Siess , S. Goriely

Scalar dark matter can interact with Standard Model (SM) particles, altering the fundamental constants of Nature in the process. Changes in the fundamental constants during and prior to Big Bang nucleosynthesis (BBN) produce changes in the…

宇宙学与河外天体物理 · 物理学 2015-04-14 Y. V. Stadnik , V. V. Flambaum

Measurements of the helium-cluster breakup and neutron removal cross sections for neutron-rich Be isotopes A=10-12,14 are presented. These have been studied in the 30 to 42 MeV/u energy range where reaction measurements are proposed to be…

核实验 · 物理学 2015-06-26 N. I. Ashwood , M. Freer

The results of the study of unstable states in relativistic dissociation of isotopes $^{9,7}$Be, $^{10}$B, $^{12,11,10}$C, $^{14}$N and $^{16}$O in nuclear emulsion have been summarized. Their decays are identified in distributions by…