Correction
Astronomy & Astrophysics
Nashwan Sabti, James Alvey, Miguel Escudero, Malcolm Fairbairn, Diego Blas
Summary: The new measurement of the d+p -> He-3+gamma reaction rate has important implications for predicting the primordial deuterium abundance during the time of BBN, but has little impact on constraints on dark sector parameters. Constraints on neutrino-like particles are not significantly affected, while constraints on electrophilic dark sector states may vary moderately. With updated results for light dark sector states, the combination of BBN and CMB observations can lead to some variation in bounds on electrophilic dark sectors.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Eunseok Hwang, Dukjae Jang, Kiwan Park, Motohiko Kusakabe, Toshitaka Kajino, A. Baha Balantekin, Tomoyuki Maruyama, Chang-Mo Ryu, Myung-Ki Cheoun
Summary: In this study, the dynamic screening effects of moving ions on big bang nucleosynthesis were explored, with findings indicating significant suppression of these effects during the BBN epoch due to the low density of background plasma components. The comparison with thermonuclear reaction rates for solar fusion was conducted to analyze the impact of dynamic screening effects, with discussions on potential expansion of the study to other astrophysical scenarios in the future.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Physics, Multidisciplinary
Latham Boyle, Kieran Finn, Neil Turok
Summary: We investigate the idea that the universe before the Big Bang is the CPT reflection of the universe after the bang to explain how the universe does not violate CPT symmetry. We show that CPT symmetry selects a preferred vacuum state for quantum fields on a CPT-invariant cosmological background spacetime. The theory also predicts a universe/anti-universe pair emerging into the radiation-dominated era and offers insights into dark matter and cosmological perturbations.
Article
Astronomy & Astrophysics
Alberto Salvio
Summary: The article investigates the general effective field theory describing the interactions of a massless dark photon with all Standard Model particles. The thermal production rate, cosmological yield, and contribution to the effective number of neutrinos of the dark photon are calculated. These predictions meet current observational bounds and will be tested in future measurements.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Simone Biondini, Jacopo Ghiglieri
Summary: In this study, the impact of the high-temperature regime on dark matter production rate is investigated. It is found that in such conditions, multiple soft scatterings and 2 -> 2 processes contribute significantly to the production rate.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Prolay Chanda, James Unwin
Summary: In this paper, the scenario in which Asymmetric Dark Matter (ADM) decouples from the Standard Model thermal bath during an early period of matter domination is explored. Model independent analysis and a specific example in the context of an elegant SO(10) implementation are presented and contrasted with conventional ADM models. The prospects for superheavy ADM in this setting are discussed in the concluding remarks.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Leo W. H. Fung, Lingfeng Li, Tao Liu, Hoang Nhan Luu, Yu-Cheng Qiu, S-H Henry Tye
Summary: Research suggests that introducing an axion model in the Higgs field can solve the Li-7 puzzle in the early universe and reconcile the late-universe measurements. The model alleviates tensions between different data sets by suppressing the matter power spectrum with the axion's matter density.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Paul Frederik Depta, Marco Hufnagel, Kai Schmidt-Hoberg
Summary: In this study, the model-independent constraints from Big Bang Nucleosynthesis on MeV-scale particles phi decaying into photons and/or electron-positron pairs are revised and updated, with the resulting bounds significantly strengthened, especially for small masses. The release of the public code ACROPOLIS for numerical solution of reaction networks allows for evaluating the impact of photodisintegration on final light element abundances, revealing potential solutions to problems like the lithium problem through processes like the photodisintegration of beryllium.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Sougata Ganguly, Sourov Roy, Ananya Tapadar
Summary: The lack of information before BBN allows for the presence of a new species 0 with a specific energy density redshift. This non-standard cosmological setup enables a larger coupling between the dark and visible sectors, even without thermal equilibrium. By considering the U(1)Lmu-LT 0 U(1)X gauge extension of the SM, different cosmological phases of the thermally decoupled dark sector are studied. It is shown that the dark matter relic density and muon (g - 2) anomaly can be reconciled within this scenario, satisfying various constraints.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Physics, Multidisciplinary
Cara Giovanetti, Mariangela Lisanti, Hongwan Liu, Joshua T. Ruderman
Summary: Dark sectors provide a theoretical framework for studying thermally-produced low-energy dark matter, and these sectors can be constrained by measuring cosmic background radiation and early universe elemental abundances.
PHYSICAL REVIEW LETTERS
(2022)
Article
Astronomy & Astrophysics
Ananya Tapadar, Sougata Ganguly, Sourov Roy
Summary: In this paper, the non-adiabatic evolution of dark sector is studied in the framework of a U(1)(L mu)-( L tau )circle times U(1)(x) extension of the standard model. The connection between the visible and dark sectors is established through a portal coupling. The temperature evolution and various non-equilibrium stages of the dark sector are analyzed. Constraints on the model parameters from laboratory and astrophysical searches are investigated. The parameter space for the non-adiabatic evolution of the dark sector is significantly constrained for certain values of mass and coupling, while other constraints depend on the mass ratio.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Physics, Multidisciplinary
Petr Jizba, Gaetano Lambiase
Summary: By employing Tsallis' non-additive delta-entropy, this paper formulates the thermodynamic laws for gravitating systems and applies them to cosmology. The results show that Tsallis cosmology can consistently describe the formation of cold dark matter particles and primordial light elements.
Article
Astronomy & Astrophysics
Takanori Sato, Fuminobu Takahashi, Masaki Yamada
Summary: This paper investigates the gravitational production of dark photon dark matter during inflation when dark photons acquire mass through the Higgs mechanism. The research reveals that the energy density spectrum of dark photons can have two peaks at intermediate and small scales. Dark photons can explain dark matter, but their current mass needs to fall within a specific range.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Logan Morrison, Stefano Profumo, Dean J. Robinson
Summary: The study discusses a dark QCD sector as a minimal extension of the Standard Model, which includes Dark Matter candidates without the need for additional interactions with the visible sector. Under specific conditions, this dark sector can generate Dark Matter candidates.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Yann Mambrini, Keith A. Olive, Jiaming Zheng
Summary: Dark matter may only interact with the visible sector at high energy scales. During the period of reheating, the dominant process of dark matter production is through the decay products of the inflaton. This process dominates for low reheating temperatures and can produce the required density of dark matter.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)