## Just Accepted

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Published:
, doi: 10.1088/1674-1137/ac945b

**Abstract:**

The cosmic distance duality relation (DDR) is constrained from the combination of type-Ia supernovae (SNe Ia) and strong gravitational lensing (SGL) systems using deep learning method. To make use of the full SGL data, we reconstruct the luminosity distance from SNe Ia up to the highest redshift of SGL using deep learning, then it is compared with the angular diameter distance obtained from SGL. Considering the influence of lens mass profile, we constrain the possible violation of DDR in three lens mass models. Results show that in the SIS model and EPL model, DDR is violated at high confidence level, with the violation parameter

*σ*confidence level, with the violation parameter

Published:
, doi: 10.1088/1674-1137/ac93ed

**Abstract:**

In this work, we systematically investigate the two-pseudoscalar meson systems with the Bethe-Salpeter equation in the ladder and instantaneous approximations. By solving the Bethe-Salpeter equation numerically with the kernel containing the one-particle exchange diagrams, we find that the

Published:
, doi: 10.1088/1674-1137/ac936b

**Abstract:**

We study the deep inelastic scattering (DIS) of a proton-targeted lepton in the presence of gluon condensation using gauge/gravity duality. We use a modified

*c*corresponds to the gluon condensation in the boundary theory. Firstly, when examining the electromagnetic field, we find that non-zero

*c*can increase the magnitude of the field. Our goal is to find the acceptable value of

*c*for this scattering and our method is based on setting the mass of the proton as an eigenvalue of the baryonic state equations of the DIS to find the acceptable value of the parameter

*c*on the other side of the equations. Therefore in the second step, we calculate wave function equations for the baryonic states where the mass of the proton target requires a value contribution of

*c*as

*x*and

*q*, which are Björken variables and the lepton momentum transfers, respectively. Comparing the Jlab Hall C data with our theoretical calculations, our results are acceptable.

Published:

**Abstract:**

We study a double covering of modular

*χ*square numerical analysis, we find that both scenarios have some predictions in case of normal hierarchy reproducing neutrino oscillation data. But, we would not find any solutions to satisfy the neutrino oscillation data in case of radiative seesaw of inverted hierarchy.

Published:

**Abstract:**

We study the dependence of the transverse mass distribution of the charged lepton and the missing energy on the parton distributions (PDFs) adapted to the

*W*boson mass measurements at the CDF and ATLAS experiments. We compare the shape variations of the distribution induced by different PDFs, and find that spread of predictions from different PDF sets can be much larger than the PDF uncertainty predicted by a specific PDF set. We suggest analyzing the experimental data using up-to-date PDFs for better understanding of the PDF uncertainties in the

*W*boson mass measurements. We further carry out a series of Lagrange multiplier scans to identify the constraints on the transverse mass distribution imposed by individual data sets in the CT18 global analysis. In the case of CDF measurement, the distribution is mostly sensitive to the

*d*-quark PDFs at intermediate

*x*region that are largely constrained by the DIS and Drell-Yan data on deuteron target, as well as the Tevatron lepton charge asymmetry data.

Published:

**Abstract:**

A partial wave scattering matrix for the total effective complex potential of nucleus nucleus collisions is used to handily analyze the angular variations of elastic scattering and fusion cross-sections simultaneously with a unique potential. The expectation value of the imaginary part of the potential calculated using the distorted waves from the full potential in the elastic channel accounts for

Published:

**Abstract:**

We make a detailed study on the properties of the total decay width of Higgs decay channel

Published:
, doi: 10.1088/1674-1137/ac945c

**Abstract:**

The cross sections of

*σ*, denoted as

Published:

**Abstract:**

In this work, we observe that in the presence of the string cloud parameter

*a*and the quintessence parameter

*γ*, with the equation of state parameter

*a*and

*γ*. Further, we see the effects of the parameters

*a*and

*γ*on the rate of emission energy for the Schwarzschild black hole. We notice that the rate of emission energy is higher in the presence of clouds of string and quintessence. Moreover, we study the weak deflection angle using the Gauss-Bonnet theorem. We show the influence of the cloud of string parameter

*a*and the quintessential parameter

*γ*on the weak deflection angle. We notice that both the parameters

*a*and

*γ*increase the deflection angle

*α*.

Published:
, doi: 10.1088/1674-1137/ac8cd5

**Abstract:**

The

*W*mass determination at the Tevatron CDF experiment reported a deviation from the SM expectation at 7

*σ*level. We discuss a few possible interpretations and their collider implications. We perform electroweak global fits under various frameworks and assumptions. We consider three types of electroweak global fits in the effective-field-theory framework: the

*S*-

*T*, the

*S*-

*T*-

Published:

**Abstract:**

In this paper, we investigate the influence of the angular momentum of a charged particle around non-extremal and extremal Einstein-Maxwell-Dilaton-Axion black holes on the Lyapunov exponent. The angular momentum's ranges and spatial regions where the bound of the exponent is violated are found for certain values of the rotation parameter and dilatonic constant of the black holes. This violation always exists when the rotation parameter is large enough and the rotation directions of the particle is opposite to those of the black holes. The spatial regions outside the extermal black hole for the violation is relatively large. In the near-horizon regions of the extremal black holes, the violation depends on the rotation directions of the black holes and particle, and does not depend on the value of the angular momentum.

Published:

**Abstract:**

In this work, the microstructure of charged AdS black holes under minimal length effects is investigated. We study the thermodynamics of black holes in the extended phase space, where the cosmological constant is regarded as the thermodynamic pressure. The modified Hawking temperature and phase transition are obtained based on the generalized uncertainty principle (GUP). Then, using thermodynamic geometry, the microstructure of black holes can be determined by the ratio of GUP parameter to charge. For a small ratio, the black hole exhibits the typical RN-AdS microstructure with van der Waals phase transition and repulsive/attractive interactions. As the ratio increases, the reentrant phase transition takes place, and both the repulsion-attraction coexisted black hole and the attraction dominated black hole can be found in this case. For a large ratio, the black hole behaves like a Schwarzchild-AdS black hole in which neither phase transition nor repulsive interaction exists. These results suggest that the GUP effect will reduce the repulsive interaction presented by the charged AdS black hole.

Published:
, doi: 10.1088/1674-1137/ac8c22

**Abstract:**

In this paper, we consider an open system from the thermodynamic perspective for an adiabatic FRW universe model in which particle creation occurs within the system. In that case, the modified continuity equation is obtained and then we correspond it to the continuity equation of

*T*is the torsion scalar. We consider the contents of the universe to be dark matter and dark energy and consider an interaction term between them. The interesting point of this study is that we make equivalent the modified continuity equation resulting from the particle creation with the matter continuity equation resulting from

Published:

**Abstract:**

In this work we study the quasi-two-body decays

Published:

**Abstract:**

We investigate generalized Jackiw-Teitelboim gravity, coupling the dilaton field with two scalar matter fields. We obtain the equations of motion of the fields and investigate the linear perturbation of the solutions in general. We study two specific situations that allow analytic solutions with topological behavior and check how the dilaton field, the warp factor and Ricci scalar behave. In particular, we have shown how the parameters can de used to modify the structure of the solutions. Moreover, the perturbations are in general described by intricate coupled differential equations, but in some specific cases we could construct the corresponding zero modes analytically.

Published:

**Abstract:**

A three Higgs-doublet model admitting an

*soft*

Published:

**Abstract:**

The dibaryon concept for the nuclear force is presented, assuming that the main attraction between the nucleons at medium distances is determined by the

*s*-channel exchange of an intermediate six-quark (dibaryon) state. To construct the respective

*NN*interaction model, a microscopic six-quark description of the

*NN*system is used, in which symmetry aspects play a special role. It is shown that the

*NN*interaction in all important partial waves can be described properly by a superposition of the long-range

*t*-channel one-pion exchange and the

*s*-channel exchange by an intermediate dibaryon. The developed model gives a good description of both elastic phase shifts and inelasticities of

*NN*scattering in all

*S*,

*P*,

*D*and

*F*partial waves at energies from zero to 600–800 MeV and even higher. The parameters of the intermediate six-quark states corresponding to the best fit of

*NN*scattering data are found to be consistent with the parameters of the known dibaryon resonances in those

*NN*partial configurations where their existence has been experimentally confirmed. Predictions for new dibaryon states are given as well.

**ISSN** 1674-1137 **CN** 11-5641/O4

Original research articles, Ietters and reviews Covering theory and experiments in the fieids of

- Particle physics
- Nuclear physics
- Particle and nuclear astrophysics
- Cosmology

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