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Study of Dark Matter with Directionality Approach Using ZnWO4 Crystal Scintillators 用ZnWO4晶体闪烁体定向研究暗物质
Q2 Physics and Astronomy Pub Date : 2022-01-01 DOI: 10.31526/lhep.2022.348
A. Leoncini, L. A. Afanasieva, P. Belli, R. Bernabei, Yu. A. Borovlev, F. Cappella, V. Caracciolo, R. Cerulli, N. Cherubini, F. A. Danevich, V. Ya. Degoda, A. Incicchitti, D. V. Kasperovych, Ya. P. Kogut, V. Merlo, G. P. Podust, O. G. Polischuk, A. G. Postupaeva, V. N. Shlegel, V. I. Tretyak
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引用次数: 0
On the Question of the Analysis ofJ/ψ→ρπ→π+π−π0 j /ψ→ρπ→π+π−π0的分析问题
Q2 Physics and Astronomy Pub Date : 2022-01-01 DOI: 10.31526/lhep.2022.329
K. Yu. Todyshev
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引用次数: 0
Review on Dark Energy Problem and Modified Gravity Theories 暗能量问题与修正引力理论综述
Q2 Physics and Astronomy Pub Date : 2022-01-01 DOI: 10.31526/lhep.2022.352
K. Bamba
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引用次数: 1
Neutrino Portal to Freeze-in Dark Matter 中微子传送门到冻结的暗物质
Q2 Physics and Astronomy Pub Date : 2022-01-01 DOI: 10.31526/lhep.2022.356
P. Bhupal Dev
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引用次数: 0
Using Embedding Theorems to Account for the Extreme Properties of Traversable Wormholes 用嵌入定理解释可穿越虫洞的极端性质
Q2 Physics and Astronomy Pub Date : 2022-01-01 DOI: 10.31526/lhep.2022.244
Peter K. F. Kuhfittig
Embedding theorems, which have a long history in the general theory of relativity, are used in this paper to account for two of the more troubling aspects of Morris-Thorne wormholes: (1) the origin of exotic matter and the amount needed to sustain a wormhole, and (2) the enormous radial tension that is characteristic of wormholes with moderately sized throats. Attributing the latter to exotic matter ignores the fact that exotic matter was introduced for a completely different reason and is usually present in only small quantities.
嵌入定理在广义相对论中有着悠久的历史,在本文中使用它来解释莫里斯-索恩虫洞的两个更令人不安的方面:(1)外来物质的起源和维持虫洞所需的量,以及(2)具有中等大小喉道的虫洞所特有的巨大径向张力。将后者归因于外来物质忽略了一个事实,即外来物质是出于完全不同的原因引入的,而且通常只以少量存在。
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引用次数: 3
String (In)Stability Issues with Broken Supersymmetry 破缺超对称的弦稳定性问题
Q2 Physics and Astronomy Pub Date : 2021-07-08 DOI: 10.31526/lhep.2021.219
J. Mourad, A. Sagnotti
We review the main results of our investigations motivated by the tadpole potentials of ten–dimensional strings with broken supersymmetry. While these are at best partial indications, it is hard to resist the feeling that they do capture some lessons of String Theory. For example, these very tadpole potentials lead to weak-string-coupling cosmologies that appear to provide clues on the onset of the inflation from an initial fast roll. The transition, if accessible to us, would offer a natural explanation for the lack of power manifested by the CMB at large angular scales. In addition, the same tadpole potentials can drive spontaneous compactifications to lower–dimensional Minkowski spaces at corresponding length scales. Furthermore, the cosmological solutions exhibit an intriguing “instability of isotropy” that, if taken at face value, would point to an accidental origin of compactification. Finally, symmetric static AdS× S solutions driven by the tadpole potentials also exist, but they are unstable due to mixings induced by their internal fluxes. On the other hand, the original Dudas–Mourad solution is perturbatively stable, and we have gathered some detailed evidence that instabilities induced by internal fluxes can be held under control in a similar class of weak–coupling type–I IB compactifications to Minkowski space. Invited contribution to the special issue of Letters in High Energy Physics (LHEP) on “Swampland and String Theory Landscape”, edited by I. Antoniadis, K. Benakli and E. Dudas
我们回顾了由破缺超对称十维弦的蝌蚪势所激发的主要研究结果。虽然这些充其量只是部分迹象,但很难不让人觉得它们确实抓住了弦理论的一些教训。例如,这些蝌蚪势导致了弱弦耦合宇宙学,它似乎提供了从最初的快速滚动开始的暴胀的线索。如果我们能观测到这种转变,就能很自然地解释宇宙微波背景在大角度尺度上表现出的能量不足。此外,相同的蝌蚪电位可以驱动相应长度尺度下的低维闵可夫斯基空间的自发紧化。此外,宇宙学解表现出一种有趣的“各向同性不稳定性”,如果从表面上看,这将指向紧化的偶然起源。最后,也存在由蝌蚪电位驱动的对称静态adsxs溶液,但由于其内部通量引起的混合而不稳定。另一方面,原始的Dudas-Mourad解是微扰稳定的,并且我们已经收集了一些详细的证据,证明由内通量引起的不稳定性可以在类似Minkowski空间的一类弱耦合i型IB紧化中被控制。应邀为《高能物理快报》(LHEP)关于“沼泽和弦理论景观”的特刊撰稿,由I. Antoniadis, K. Benakli和E. Dudas编辑
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引用次数: 8
Higgs Portal Vector Dark Matter Interpretation: Review of EffectiveField Theory Approach and Ultraviolet Complete Models 希格斯入口向量暗物质解释:对有效场理论方法和紫外线完全模型的回顾
Q2 Physics and Astronomy Pub Date : 2021-07-02 DOI: 10.31526/lhep.2022.270
M. Zaazoua, L. Truong, K. Assamagan, F. Fassi
A review of the Higgs portal-vector dark matter interpretation of the spin-independent darkmatter nucleon elastic scattering cross section is presented, where the invisible Higgs decay width measured at the LHC is used. Effective Field Theory and ultraviolet complete models are discussed. LHC interpretations show only the scalar and Majorana dark-matter scenarios; we propose to include interpretation for vector dark matter in the EFT and UV completions theoretical framework. In addition, our studies suggest an extension of the LHC dark matter interpretations to the sub-GeV regime.
综述了对自旋无关暗物质核子弹性散射截面的希格斯门矢量暗物质解释,其中使用了在LHC测量的不可见希格斯衰变宽度。讨论了有效场论和紫外完全模型。LHC的解释只显示了标量和马略拉纳暗物质的场景;我们建议在EFT和UV完成理论框架中包括对矢量暗物质的解释。此外,我们的研究表明,LHC暗物质的解释扩展到了亚GeV状态。
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引用次数: 8
Quantum Newtonian Cosmology Revisited 量子牛顿宇宙学重访
Q2 Physics and Astronomy Pub Date : 2021-04-12 DOI: 10.31526/LHEP.2022.321
L. Gouba
We formulate the Lagrangian of the Newtonian cosmology where the cosmological constant is also introduced. Following the affine quantization procedure, the Hamiltonian operator is derived. The wave functions of the Newtonian universe and the corresponding eigenvalues for the case of matter dominated by a negative cosmological constant are given.
我们建立了牛顿宇宙学的拉格朗日量,其中还引入了宇宙学常数。根据有效的量子化过程,导出了哈密顿算子。给出了牛顿宇宙的波函数和负宇宙学常数支配物质情况下的相应特征值。
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引用次数: 0
Formal Solutions of Any-Order Mass, Angular-Momentum, andDipole Perturbations on the Schwarzschild Background Spacetime Schwarzschild背景时空上任意阶质量、角动量和偶极扰动的形式解
Q2 Physics and Astronomy Pub Date : 2021-01-31 DOI: 10.31526/lhep.2021.215
Kouji Nakamura
Formal solutions of any-order mass, angular-momentum, dipole perturbations on the Schwarzschild background spacetime are derived in a gauge-invariant manner. Once we accept the proposal in [K. Nakamura, Class. Quantum Grav. {bf 38} (2021), 145010.], we can extend the gauge-invariant linear perturbation theory on the Schwarzschild background spacetime including the monopole ($l=0$) and dipole ($l=1$) modes to any-order perturbations of the same background spacetime through the arguments in [K. Nakamura, Class. Quantum Grav. {bf 31} (2014), 135013.]. As a result of this resolution, we reached to a simple derivation of the above formal solutions of any order.
以规范不变的方式导出了Schwarzschild背景时空上任意阶质量、角动量、偶极扰动的形式解。一旦我们接受了[K.Nakamura,Class.Quantum Grav.{bf 38}(2021),145010.]中的提议,我们可以通过[K.Nakamura,Class.Quantum Grav.{bf 31}(2014),135013.]中的自变量,将包括单极($l=0$)和偶极($l=1$)模式的Schwarzschild背景时空上的规范不变线性微扰理论扩展到相同背景时空的任何阶微扰,我们得到了上述任意阶形式解的一个简单推导。
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引用次数: 4
Explaining the Results of EDGES Observation of 21 cm Line with Dark Matter-Dark Energy and Dark Matter-Baryon Interactions 用暗物质-暗能量和暗物质-重子相互作用解释21厘米线EDGES观测结果
Q2 Physics and Astronomy Pub Date : 2021-01-31 DOI: 10.31526/lhep.2021.208
Upala Mukhopadhyay, D. Majumdar, Kanan K. Datta
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引用次数: 0
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Letters in High Energy Physics
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