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Theoretical calculations based on the Dirac--Coulomb--Breit relativistic coupled cluster method have been carried out for the electron affinities and ionization potentials of the superheavy element nihonium (Nh) and its lighter homologues…

Atomic Physics · Physics 2022-07-13 Yangyang Guo , Anastasia Borschevsky , Ephraim Eliav , Lukáš F. Pašteka

We use the constraints arising from primordial nucleosynthesis to bound a putative electric charge density $|e|n_q$ of the universe. We find $|n_q/n_\gamma| \lesssim 10^{-43}$, four orders of magnitude more stringent than previous limits.…

Astrophysics · Physics 2009-11-07 Eduard Masso , Francesc Rota

There have been suggestions that the abundance of Extremely Metal-Poor (EMP) stars can be reproduced by Hypernovae (HNe), not by normal supernovae (SNe). However, recently it was also suggested that if the innermost neutron-rich or…

High Energy Astrophysical Phenomena · Physics 2010-08-10 Natsuko Izutani , Hideyuki Umeda

The theory of QED corrections to hyperfine structure in light hydrogenic atoms and ions has recently advanced to the point that the uncertainty of these corrections is much smaller than 1 part per million (ppm), while the experiments are…

Nuclear Theory · Physics 2014-11-18 J. L. Friar , G. L. Payne

Probabilties of formation of various hydrogenic species during the exothermic nuclear $(n,{}^3$He$;t,p)-$reaction of atomic helium-3 with slow neutrons are determined. In particular, we have found that the probability to form the tritium…

Nuclear Theory · Physics 2015-05-27 Alexei M. Frolov , David M. Wardlaw

The theoretical status of the neutrino-nucleon cross section is reviewed for incident neutrino energies up to E_nu=10^12 GeV, including different approaches to high energy extrapolations. Nonstandard model physics may play a role at…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. H. Reno

The $1s^2->1s2p(^1P)$ excitation in confined and compressed helium atoms in either the bulk material or encapsulated in a bubble is shifted to energies higher than that in the free atom. For bulk helium, the energy shifts predicted from…

Chemical Physics · Physics 2023-08-09 N. C. Pyper , A. J. W. Thom , Colm T. Whelan

We have derived a primordial helium abundance of Yp = 0.2477 +- 0.0029, based on new atomic physics computations of the recombination coefficients of He I and of the collisional excitation of the H I Balmer lines together with observations…

Astrophysics · Physics 2011-02-11 M. Peimbert , V. Luridiana , A. Peimbert

The mass estimates of active and sterile (right-handed) neutrinos are considered at the phenomenological level using the seesaw mechanism. It is assumed that the neutrino mass values depend on three characteristic scales, and the sum of the…

High Energy Physics - Phenomenology · Physics 2025-05-13 V. V. Khruschov , S. V. Fomichev

Observation of Ultra High Energy Cosmic Rays (UHECR) -whose energy exceeds $10^20$eV- is still a puzzle for modern astrophysics. The transfer of more than 16 Joules to a microscopic particle can hardly be achieved, even in the most powerful…

Astrophysics · Physics 2009-10-31 Antoine Letessier-Selvon

In Phys. Rev. Lett. 102, 197002 (2009) it was reported that the element Eu becomes superconducting in the pressure and temperature range [84-142GPa], [1.8-2.75K]. The claim was largely based on ac susceptibility measurements. Recently…

Superconductivity · Physics 2021-12-10 J. E. Hirsch

In recent years, ALICE has extensively studied the production of light (anti)(hyper)nuclei in different collision systems and center-of-mass energies. Nevertheless, the production mechanisms of light (hyper)nuclei is still unclear and under…

High Energy Physics - Experiment · Physics 2023-03-22 Chiara Pinto

We have investigated the partitioning of U between silicate melt and Fe liquid at pressures of 3.0 to14.5 GPa and temperatures of 1660 to 2500 oC. The solubility of U in liquid Fe is in the range of 0.6 to 800 ppm and increases with…

Astrophysics · Physics 2007-05-23 Xuezhao Bao , Richard A. Secco , Joel E. Gagnon , Brian J. Fryer

We revisit the constraints on the properties of right handed neutrinos from the requirement to explain the observed light neutrino oscillation data in the type-I seesaw model. We use well-known relations to show that there is in general no…

High Energy Physics - Phenomenology · Physics 2019-05-03 Marco Drewes

Currently there are two significantly different observational determinations of the primordial helium abundance, and, if only statistical errors in He4 abundance determinations are considered, the discrepancies between the observational…

Astrophysics · Physics 2009-09-15 Keith A. Olive , Evan D. Skillman

High pT hadrons produced in ultra-relativistic heavy-ion collisions at RHIC probe nuclear matter at extreme conditions of high energy density. Experimental measurements in Au+Au collisions at \sqrtsNN=130, 200 GeV establish the existence of…

High Energy Physics - Experiment · Physics 2017-08-23 K. Filimonov

The interaction of relativistically strong tailored laser pulses with an atomic system is considered. Due to a special tailoring of the laser pulse, the suppression of the relativistic drift of the ionized electron and a dramatic…

Atomic Physics · Physics 2007-05-23 M. Klaiber , K. Z. Hatsagortsyan , C. H. Keitel

We study low-energy consequences of supersymmetric $SO(10)$ models with Yukawa unification $h_t = h_N$ and $h_b = h_\tau$. We find that it is difficult to reproduce the observed $m_b/m_\tau$ ratio when the third-generation right-handed…

High Energy Physics - Phenomenology · Physics 2009-09-29 Andrea Brignole , Hitoshi Murayama , Riccardo Rattazzi

The recent demonstration of laser excitation of the $\approx 8$ eV isomeric state of Thorium-229 is a significant step towards a nuclear clock. The low excitation energy likely results from a cancellation between electromagnetic and strong…

High Energy Physics - Phenomenology · Physics 2025-09-16 Andrea Caputo , Doron Gazit , Hans-Werner Hammer , Joachim Kopp , Gil Paz , Gilad Perez , Konstantin Springmann

I consider the synthesis of 6Li due to the decay of relic particles, such as gravitinos or moduli, after the epoch of Big Bang Nucleosynthesis. The synthesized 6Li/H ratio may be compared to 6Li/H in metal-poor stars which, in the absence…

Astrophysics · Physics 2009-10-31 K. Jedamzik
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