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In this study, we investigate the contribution of millisecond pulsars (MSPs) to the gamma-ray excess observed in the Galactic Center by analyzing data from high-resolution direct N-body simulations of six globular clusters (GCs) that experience close encounters with the nuclear star cluster. Using the φ-GPU code, we tracked the orbits of individual neutron stars (NSs) formed during the simulations, assuming a fraction of these NSs evolve into MSPs. Our model includes state-of-the-art single stellar evolution code including prescription for neutron star formation. We estimated the gamma-ray flux from these MSPs, considering known values for their gamma-ray emission. Our results show that MSPs originating from the six modeled GCs contribute a small but non-negligible fraction of the observed gamma-ray flux. This finding suggests that the actual gamma-ray flux from MSPs could be much higher when considering the entire population of GCs, potentially significantly contributing to the gamma-ray excess. This study highlights the importance of considering MSPs in the Galactic Center, originating from nearby globular clusters, as a potential source of the observed gamma-ray excess. Future work will involve more sophisticated simulations incorporating binary stellar evolution and comparing the fraction of MSPs in observed GCs to refine our models and improve the accuracy of our estimates. [ABSTRACT FROM AUTHOR]

Based on the recent association of IceCube TeV and PeV neutrino events with gamma-ray bursts (GRBs) by considering the Lorentz violation of neutrinos, we provide a new estimate on the GRB neutrino flux with a more significant result compared to the previous constraint by the IceCube Collaboration. Among these 24 neutrino "shower" events above 60 TeV, 12 events are associated with GRBs. Such a result is compatible with the prediction from GRB fireball models. Analysis of track events provides a consistent result with the shower events to associate high energy cosmic neutrinos with GRBs under the same Lorentz violation features of neutrinos. We also make a background estimation and reveal GRBs as a significant source for the ultra-high energy IceCube neutrino events. Our work supports the Lorentz violation and CPT -violation of neutrinos, indicating new physics beyond relativity. [ABSTRACT FROM AUTHOR]

Through comprehensively applying geological and geophysical data, as well as core and thin section observation, the characteristics of reservoirs and fractures in the second member of the Xujiahe Formation (hereinafter referred to as Xu2 Member) in the Yuanba area, northern Sichuan Basin, were studied. Combined with the analysis of the main controlling factors of production capacity, the types and characteristics of the sweet spots in the tight sandstone gas reservoir were determined. The evaluation standards and geological models of the sweet spots were established. The results are as follows: (1) There are bedding-parallel fracture-, fault-induced fracture-, and pore-dominated sweet spots in the tight sandstone gas reservoirs of the Xu2 Member. (2) The bedding parallel fracture-dominated sweet spots have developed in quartz sandstones with well-developed horizontal fractures and micro-fractures. They are characterized by high permeability and high gas output during production tests. This kind of sweet spots is thin and shows a limited distribution. Their logging responses show extremely low gamma-ray (GR) values and medium-high AC values. Moreover, the bedding parallel fracture-dominated sweet spots can be mapped using seismic methods. (3) The fault-induced fracture-dominated sweet spots have welldeveloped medium- and high-angle shear fractures. Their logging responses show an increase in peaks of AC values and total hydrocarbon content and a decrease in resistivity. Seismically, the areas with welldeveloped fault-induced fracture-dominated sweet spots can be effectively mapped using the properties such as seismic entropy and maximum likelihood. (4) The pore-dominated sweet spots are developed in medium-grained feldspathic litharenites with good reservoir properties. They are thick and widely distributed. (5) These three types of sweet spots are mainly determined by sedimentation, diagenesis, and tectonism. The bedding parallel fracture-dominated sweet spots are distributed in beachbar quartz sandstones on the top of the 1st sand layer group in the Xu2 Member, which develops in a shore-shallow lake environment. The fault-induced fracture-dominated sweet spots mainly occur near faults. They are increasingly developed in areas closer to faults. The pore-dominated sweet spots are primarily distributed in the 2nd and 3rd sand layer groups, which lie in the development areas of distributary channels near provenances at western Yuanba area. Based on the geological and seismic data, a comprehensive evaluation standard for these three types of sweet spots of the tight sandstone reservoirs in the Xu2 Member has been established, which, on the one hand, lays the foundation for the development and evaluation of the gas reservoir, and on the other hand, deepens the understanding of sweet spot in the tight sandstone gas reservoirs. [ABSTRACT FROM AUTHOR]