Effects of the Electronic Structure, Phase Transition and Localized Dynamics of Atoms in the Formation of Tiny Particles of Gold

In addition to the self-governing properties, tiny metallic colloids are the building blocks of larger particles. This topic has been a subject of many studies. Tiny particles of different sizes developed under three different experiments are discussed in this work. The development of a tiny-sized particle depends on the attained dynamics of atoms. When atoms of the compact monolayer assembly bind by a nanoenergy packet, the developed tiny-sized particle elongates atoms of arrays into the structures of smooth elements at the solution surface. The impinging electron streams at a fixed angle can elongate the already elongated atoms of arrays. Travelling photons along the interface influence the modified atoms. Gold atoms can also develop different tiny particles inside the solution. In addition to the dynamics of atoms, miscellaneous factors can contribute in the development of such tiny particles. Atoms in the form of tiny clusters can also amalgamate to develop a tiny-sized particle. In the third kind of tiny particle, amalgamated atoms can bind by executing electron dynamics. However, not all of the atoms can bind by the electron dynamics. This study very concisely highlights the fundamental process of developing a variety of tiny particles in which electronic structure, phase transition and localized dynamics of gold atoms influence the structure. The study targets the specific discussion that how atoms of tiny-sized particles bind, and how travelling photons along the air-solution interface influence their structure. Several possibilities may be opened through pulse-based process to develop engineered materials

Finslerian dipolar modulation of the CMB power spectra at scales 2<l<6002<l<600

A common explanation for the CMB power asymmetry is to introduce a dipolar modulation at the stage of inflation, where the primordial power spectrum is spatially varying. If the universe in the stage of inflation is Finslerian, and if the Finsler spacetime is non-reversible under parity flip, $x\rightarrow-x$, then a three dimensional spectrum which is the function of wave vector and direction is valid. In this paper, a three dimensional primordial power spectrum with preferred direction is derived in the framework of Finsler spacetime. It is found that the amplitude of dipolar modulation is related to the Finslerian parameter, which in turn is a function of wave vector. The angular correlation coefficients are presented, and the numerical results for the anisotropic correlation coefficients over the multipole range $2<l<600$ are given.Comment: 13 pages, 1 figure, accepted by EPJ

The electromagnetic decays of the charmed and bottom baryons in chiral perturbation theory

We have investigated the electromagnetic decays of the antitriplet and sextet charmed baryon systems with $J^P= \frac{1}{2}^+, \frac{3}{2}^+$ in the framework of the heavy baryon chiral perturbation theory. We first construct the chiral Lagrangians at $O(p^2)$ and $O(p^3)$. Then we calculate the electromagnetic (EM) decay amplitudes of the charmed baryon systems up to $O(p^3)$. With the help of the quark model, we estimate the low energy constants. The numerical results of the EM decay widths show good convergence of the chiral expansion. We notice that the two neutral EM decay processes $\Xi_c'^0\rightarrow\gamma+\Xi_c^0$ and ${\Xi_c^*}'^0\rightarrow\gamma+\Xi_c^0$ are strongly suppressed by the SU(3) U-spin flavor symmetry. With the same formalism, we also estimate the EM decay widths of the bottomed baryons. The EM decay widths of the heavy baryons may be measured at facilities such as LHCb and JPARC. The explicit chiral structures of the heavy baryon decay amplitudes derived in this work may be useful to the possible chiral extrapolations of the future lattice simulations of these EM decay amplitudes