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The effectiveness of selection in a species affects the direction of amino acid frequency evolution. 物种选择的有效性会影响氨基酸频率的进化方向。
4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-06-22 DOI: 10.1101/2023.02.01.526552
Hanon McShea, Catherine Weibel, Sawsan Wehbi, Peter Goodman, Jennifer E James, Andrew L Wheeler, Joanna Masel

Nearly neutral theory predicts that species with higher effective population size (N e ) are better able to purge slightly deleterious mutations. We compare evolution in high-N e vs. low-N e vertebrates to reveal which amino acid frequencies are subject to subtle selective preferences. We take three complementary approaches, two measuring flux and one measuring outcomes. First, we fit non-stationary substitution models of amino acid flux using maximum likelihood, comparing the high-N e clade of rodents and lagomorphs to its low-N e sister clade of primates and colugos. Second, we compare evolutionary outcomes across a wider range of vertebrates, via correlations between amino acid frequencies and N e . Third, we dissect the details of flux in human, chimpanzee, mouse, and rat, as scored by parsimony - this also enables comparison to a historical paper. All three methods agree on which amino acids are preferred under more effective selection. Preferred amino acids tend to be smaller, less costly to synthesize, and to promote intrinsic structural disorder. Parsimony-induced bias in the historical study produces an apparent reduction in structural disorder, perhaps driven by slightly deleterious substitutions. Within highly exchangeable pairs of amino acids, arginine is strongly preferred over lysine, and valine over isoleucine, consistent with more effective selection preferring a marginally larger free energy of folding. These two preferences match differences between thermophiles and mesophilic relatives. These results reveal the biophysical consequences of mutation-selection-drift balance, and demonstrate the utility of nearly neutral theory for understanding protein evolution.

近中性理论预测,有效种群规模(N e)较高的物种能够更好地清除轻微的有害突变。我们比较了高 N e 与低 N e 脊椎动物的进化,以揭示哪些氨基酸频率受到微妙的选择性偏好的影响。我们采用了三种互补的方法,其中两种测量通量,一种测量结果。首先,我们使用最大似然法拟合氨基酸通量的非稳态替代模型,将啮齿类和蜥脚类的高N e支系与灵长类和疣鼻类动物的低N e姊妹支系进行比较。其次,我们通过氨基酸频率与 N e 之间的相关性,比较了更多脊椎动物的进化结果。第三,我们通过解析法对人类、黑猩猩、小鼠和大鼠的通量细节进行剖析--这也可以与历史文献进行比较。所有三种方法都一致认为,在更有效的选择下,哪些氨基酸更受青睐。优先选择的氨基酸往往体积较小,合成成本较低,而且会导致内在结构紊乱。在历史研究中,由解析偏差引起的结构紊乱明显减少,这可能是由轻微的有害替代引起的。在高度可交换的氨基酸对中,精氨酸比赖氨酸更受青睐,缬氨酸比异亮氨酸更受青睐,这与更有效的选择更青睐折叠自由能稍大的氨基酸是一致的。这两种偏好与嗜热菌和中嗜热菌之间的差异相吻合。这些结果揭示了突变-选择-漂移平衡的生物物理后果,并证明了近中性理论在理解蛋白质进化方面的实用性:根据分子进化的近中性理论,在种群规模较小的物种中,选择区分相似等位基因的能力较弱。我们确定了哪些氨基酸会受到这种弱偏好的影响--这些氨基酸往往较小、制造成本较低、会促进蛋白质结构的紊乱,而且相对于中嗜热菌而言,嗜热菌更富含这些氨基酸。后者与变异-选择-漂移平衡下蛋白质边际稳定性的理论相吻合。
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引用次数: 0
Superluminal geometrodynamics of braneworld hyperdrive via brane–bulk interaction 通过 "桥块 "相互作用的支链世界超驱动超光速几何动力学
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-31 DOI: 10.1142/s0217732324500329
Anuar Alias, Azman Jalar

Alcubierre’s warp-drive was the first to introduce superluminal travel from different approaches. Instead of creating a shortcut through spacetime via a wormhole, geometrodynamics of simultaneously contracting and expanding spacetime were conjectured. However, both methods require exotic matter that violates energy conditions. In this paper, we employ the concept of braneworld that naturally influences spacetime geometrodynamics. Starting from defining and developing the spacetime metric of the braneworld warp bubble, the expression for energy densities as a function of relevant parameters which contributes to the braneworld approach of superluminal travel by hyperspace-drive was derived.

阿尔库比耶尔的曲速飞行器首次从不同角度引入了超光速旅行。与通过虫洞创造穿越时空的捷径不同,人们猜想了同时收缩和膨胀时空的几何力学。然而,这两种方法都需要违反能量条件的奇异物质。在本文中,我们采用了自然影响时空几何动力学的支链世界概念。从定义和发展支链世界翘曲气泡的时空度量开始,推导出了能量密度作为相关参数函数的表达式,这有助于支链世界超空间驱动器的超光速旅行方法。
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引用次数: 0
A review on correlations among the multiplicities of charge particles at SPS, RHIC and LHC energies 关于 SPS、RHIC 和大型强子对撞机能量下电荷粒子倍率之间相关性的综述
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-31 DOI: 10.1142/s0217732324300039
Shreya Bhattacharjee, Prabir Kr. Haldar

Correlation study among the charge particle multiplicities plays an important role to analyze the heavy-ion interactions. Different observables like charged particle multiplicities, azimuthal anisotropy among the multiplicity of charge particles, transverse momentum of the multiplicities, etc. can correlate and these help to comprehend the various phases of heavy-ion collisions. We have reviewed two- and three-particle correlations, azimuthal correlations and Bose–Einstein correlations among the multiplicities of charge particles. We have also studied the forward-backward correlation technique to investigate the correlations among the charged multiplicities. Here, we have discussed various kinds of correlations at SPS energy, RHIC energy and LHC energy.

电荷粒子多重性之间的相关性研究在分析重离子相互作用方面发挥着重要作用。带电粒子倍率、带电粒子倍率的方位角各向异性、倍率的横向动量等不同观测值之间存在相关性,这有助于理解重离子碰撞的各个阶段。我们回顾了电荷粒子倍率之间的两粒子和三粒子相关性、方位相关性和玻色-爱因斯坦相关性。我们还研究了前向后相关技术,以研究带电粒子倍率之间的相关性。在这里,我们讨论了在 SPS 能量、RHIC 能量和 LHC 能量下的各种相关性。
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引用次数: 0
Addendum — Inertia modified by electromagnetic Abelian gauge transformations 增编--通过电磁阿贝尔规规变换修正惯性
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-31 DOI: 10.1142/s0217732324910012
Alcides Garat

In this paper, we will analyze the relationship between both potentials in vacuum electrodynamics and their local gauge transformations.

本文将分析真空电动力学中这两种势之间的关系及其局部规规变换。
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引用次数: 0
Kaluza–Klein cosmological model with strange-quark-matter in f(R,T) theory of gravity f(R,T) 引力理论中具有奇异夸克物质的卡卢扎-克莱因宇宙学模型
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-31 DOI: 10.1142/s0217732324500561
Y. S. Solanke, T. D. Nakade, D. D. Pawar, V. J. Dagwal

This work deals with the Kaluza–Klein cosmological model with strange-quark-matter in f(R,T) theory of gravity, where R is the Ricci scalar and T is the trace of the energy–momentum tensor. To determine the solution of the field equation, we have assumed that scalar expansion θ is proportional to shear scalar σ2 which leads to R=Am, where R and A are metric potentials and m is constant. The cosmological parameters are investigated with the help of the equation of state strange-quark-matter (SQM) is p=ρ4Bc3, where Bc is Bag constant. We have concentrated on the distances of cosmology such as the look-back time, proper distance, luminosity distance, angular-diameter distance and distance modulus which are presented graphically by using suitable data of H0. The physical and geometrical properties of models are also discussed.

本研究涉及引力 f(R,T)理论中的奇异夸克物质的卡卢扎-克莱因宇宙学模型,其中 R 是利玛窦标量,T 是能动张量的迹。为了确定场方程的解,我们假定标量膨胀θ与剪切标量σ2成正比,从而得出 R=Am,其中 R 和 A 是度量势,m 是常数。借助奇异夸克物质(SQM)的状态方程 p=ρ-4Bc3(其中 Bc 是 Bag 常量)来研究宇宙学参数。我们集中研究了宇宙学中的距离,如回望时间、适当距离、光度距离、角直径距离和距离模量,并利用适当的 H0 数据以图表的形式展示出来。我们还讨论了模型的物理和几何特性。
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引用次数: 0
Effect of polarized colliding beam on Higgs boson production at the lepton collider 偏振对撞光束对轻子对撞机产生希格斯玻色子的影响
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-08 DOI: 10.1142/s0217732324500470
Ijaz Ahmed, Mashal Shakar, M. U. Ashraf, Jamil Muhammad, Taimoor Khurshid

Different production processes involving the Higgs boson, such as annihilation and W/Z boson fusion, will be observed in the International Linear Collider (ILC). The ILC operates at a center-of-mass (CM) energy of s=200–1000GeV. The study reveals that the production cross-section can either be enhanced or reduced depending on the CM energy and the specific combination used, which has implications for selecting appropriate production processes. Additionally, this investigation highlights that by polarizing beams, the number of measurable observables increases. These observables, such as left–right asymmetry, detailed effective polarization, and adequate effective luminosity, are crucial to ascertain contemporary physical parameters in physics models absurdly the Standard Model (SM).

国际直线对撞机(ILC)将观测涉及希格斯玻色子的不同生产过程,如湮灭和W/Z玻色子融合。国际直线对撞机的质心能量为 s=200-1000GeV。研究显示,根据 CM 能量和所使用的特定组合,生产截面可以增强或减小,这对选择适当的生产过程具有影响。此外,这项研究还强调,通过对光束进行极化,可测量的观测值数量也会增加。这些观测指标,如左右不对称、详细的有效偏振和足够的有效光度,对于确定荒谬的标准模型(SM)物理模型中的当代物理参数至关重要。
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引用次数: 0
Further prediction on the possible double-peak structure of the X17 particle 对 X17 粒子可能的双峰结构的进一步预测
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-08 DOI: 10.1142/s0217732324500573
Hua-Xing Chen
<p>The <span><math altimg="eq-00003.gif" display="inline" overflow="scroll"><mi>X</mi><mn>1</mn><mn>7</mn></math></span><span></span> particle, discovered by [A. J. Krasznahorkay <i>et al.</i>, <i>Phys. Rev. Lett.</i><b>116</b>, 042501 (2016), doi:10.1103/PhysRevLett.116.042501] at ATOMKI, was recently confirmed in the <span><math altimg="eq-00004.gif" display="inline" overflow="scroll"><mi>γ</mi><mi>γ</mi></math></span><span></span> invariant mass spectra by [K. U. Abraamyan, C. Austin, M. I. Baznat, K. K. Gudima, M. A. Kozhin, S. G. Reznikov and A. S. Sorin, arXiv:2311.18632] at JINR. We notice with surprise and interest that the <span><math altimg="eq-00005.gif" display="inline" overflow="scroll"><mi>X</mi><mn>1</mn><mn>7</mn></math></span><span></span> seems to have a double-peak structure. This is in a possible coincidence with our QCD sum rule study of [H.-X. Chen, arXiv:2006.01018], where we interpreted the <span><math altimg="eq-00006.gif" display="inline" overflow="scroll"><mi>X</mi><mn>1</mn><mn>7</mn></math></span><span></span> as a tetraquark state composed of four bare quarks (<span><math altimg="eq-00007.gif" display="inline" overflow="scroll"><mi>u</mi><mi>ū</mi><mi>d</mi><mover accent="true"><mrow><mi>d</mi></mrow><mo>̄</mo></mover></math></span><span></span>), and claimed that “A unique feature of this tetraquark assignment is that we predict two almost degenerate states with significantly different widths”. These two different tetraquark states are described by two different chiral tetraquark currents <span><math altimg="eq-00008.gif" display="inline" overflow="scroll"><msub><mrow><mi>ū</mi></mrow><mrow><mi>L</mi></mrow></msub><msub><mrow><mi>γ</mi></mrow><mrow><mi>μ</mi></mrow></msub><msub><mrow><mi>d</mi></mrow><mrow><mi>L</mi></mrow></msub><mspace width="0.35em"></mspace><msub><mrow><mover accent="true"><mrow><mi>d</mi></mrow><mo>̄</mo></mover></mrow><mrow><mi>L</mi></mrow></msub><msup><mrow><mi>γ</mi></mrow><mrow><mi>μ</mi></mrow></msup><msub><mrow><mi>u</mi></mrow><mrow><mi>L</mi></mrow></msub></math></span><span></span> and <span><math altimg="eq-00009.gif" display="inline" overflow="scroll"><msub><mrow><mi>ū</mi></mrow><mrow><mi>L</mi></mrow></msub><msub><mrow><mi>γ</mi></mrow><mrow><mi>μ</mi></mrow></msub><msub><mrow><mi>d</mi></mrow><mrow><mi>L</mi></mrow></msub><mspace width="0.35em"></mspace><msub><mrow><mover accent="true"><mrow><mi>d</mi></mrow><mo>̄</mo></mover></mrow><mrow><mi>R</mi></mrow></msub><msup><mrow><mi>γ</mi></mrow><mrow><mi>μ</mi></mrow></msup><msub><mrow><mi>u</mi></mrow><mrow><mi>R</mi></mrow></msub></math></span><span></span>. To verify whether the tetraquark assignment is correct or not, we replace the up and down quarks by the strange quarks, and apply the QCD sum rule method to study the other four chiral tetraquark currents <span><math altimg="eq-00010.gif" display="inline" overflow="scroll"><msub><mrow><mi>ū</mi></mrow><mrow><mi>L</mi></mrow></msub><msub><mrow><mi>γ</mi></mrow><mrow><mi>μ</mi></
由[A. J. Krasznahorkay 等人,Phys.J. Krasznahorkay 等人,Phys. Rev. Lett.116,042501 (2016),doi:10.1103/PhysRevLett.116.042501] 在 ATOMKI 发现的 X17 粒子,最近被 [K. U. Abraamyan、C. Austin、M. I. Baznat、K. K. Gudima、M. A. Kozhin、S. G. G. Baznat、K.U. Abraamyan、C. Austin、M. I. Baznat、K. K. Gudima、M. A. Kozhin、S. G. Reznikov 和 A. S. Sorin, arXiv:2311.18632]在日本核研院证实。我们惊讶并感兴趣地注意到,X17 似乎具有双峰结构。这可能与我们的 QCD 和则研究[H.-X. Chen, arXiv:2006.01018]不谋而合,当时我们把 X17 解释为由四个裸夸克(uūd̄)组成的四夸克态,并声称 "这种四夸克赋值的一个独特特征是,我们预测了两个宽度明显不同的几乎退化的态"。这两种不同的四夸克态由两种不同的手性四夸克电流 ūLγμdLd̄LγμuL 和 ūLγμdLd̄RγμuR 描述。为了验证四夸克的赋值是否正确,我们用奇异夸克来代替上夸克和下夸克、并应用 QCD 和则方法研究另外四种手性四夸克电流 ūLγμsLs̄LγμuL、ūLγμsLs̄RγμuR、d̄LγμsLs̄LγμdL 和 d̄LγμsLs̄RγμdR。我们计算了它们的相关函数,发现非微扰 QCD 效应对它们的贡献不大。我们的结果表明,可能存在质量约为236∼296MeV的四个几乎退化的四夸克态。每个态都由四个裸夸克(uūss̄或 dd̄ss̄)组成。
{"title":"Further prediction on the possible double-peak structure of the X17 particle","authors":"Hua-Xing Chen","doi":"10.1142/s0217732324500573","DOIUrl":"https://doi.org/10.1142/s0217732324500573","url":null,"abstract":"&lt;p&gt;The &lt;span&gt;&lt;math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;X&lt;/mi&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; particle, discovered by [A. J. Krasznahorkay &lt;i&gt;et al.&lt;/i&gt;, &lt;i&gt;Phys. Rev. Lett.&lt;/i&gt;&lt;b&gt;116&lt;/b&gt;, 042501 (2016), doi:10.1103/PhysRevLett.116.042501] at ATOMKI, was recently confirmed in the &lt;span&gt;&lt;math altimg=\"eq-00004.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; invariant mass spectra by [K. U. Abraamyan, C. Austin, M. I. Baznat, K. K. Gudima, M. A. Kozhin, S. G. Reznikov and A. S. Sorin, arXiv:2311.18632] at JINR. We notice with surprise and interest that the &lt;span&gt;&lt;math altimg=\"eq-00005.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;X&lt;/mi&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; seems to have a double-peak structure. This is in a possible coincidence with our QCD sum rule study of [H.-X. Chen, arXiv:2006.01018], where we interpreted the &lt;span&gt;&lt;math altimg=\"eq-00006.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;X&lt;/mi&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; as a tetraquark state composed of four bare quarks (&lt;span&gt;&lt;math altimg=\"eq-00007.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;u&lt;/mi&gt;&lt;mi&gt;ū&lt;/mi&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;mover accent=\"true\"&gt;&lt;mrow&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;mo&gt;̄&lt;/mo&gt;&lt;/mover&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;), and claimed that “A unique feature of this tetraquark assignment is that we predict two almost degenerate states with significantly different widths”. These two different tetraquark states are described by two different chiral tetraquark currents &lt;span&gt;&lt;math altimg=\"eq-00008.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;ū&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mspace width=\"0.35em\"&gt;&lt;/mspace&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mover accent=\"true\"&gt;&lt;mrow&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;mo&gt;̄&lt;/mo&gt;&lt;/mover&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;u&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; and &lt;span&gt;&lt;math altimg=\"eq-00009.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;ū&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mspace width=\"0.35em\"&gt;&lt;/mspace&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mover accent=\"true\"&gt;&lt;mrow&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;mo&gt;̄&lt;/mo&gt;&lt;/mover&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;R&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;u&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;R&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;. To verify whether the tetraquark assignment is correct or not, we replace the up and down quarks by the strange quarks, and apply the QCD sum rule method to study the other four chiral tetraquark currents &lt;span&gt;&lt;math altimg=\"eq-00010.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;ū&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;μ&lt;/mi&gt;&lt;/","PeriodicalId":18752,"journal":{"name":"Modern Physics Letters A","volume":"4 1","pages":""},"PeriodicalIF":1.4,"publicationDate":"2024-05-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140926997","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Degeneracy pressure in the presence of maximum length for non-interacting electrons 非相互作用电子存在最大长度时的去能压力
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-08 DOI: 10.1142/s0217732324500391
S. Parsamehr, N. Fatahi

Combining quantum theory with the fundamental principles of gravity results in the modification of the uncertainty principle. In this study, we employ the extended uncertainty principle (EUP) with the maximum length derived from the cosmological particle horizon. The impact of this specific kind of modification is examined in a non-interacting electron gas system. We analytically derive the generalized relations for the degeneracy pressure and the bulk modulus. An intriguing finding is that the degeneracy pressure is reduced, as confirmed by the observed size of white dwarfs, which is smaller than what is predicted by the standard theory. Nevertheless, it is still capable of providing support against gravitational collapse.

量子理论与引力基本原理的结合导致了对不确定性原理的修正。在这项研究中,我们采用了扩展不确定性原理(EUP),其最大长度来自宇宙学粒子视界。我们在一个非相互作用电子气体系统中研究了这种特定修改的影响。我们分析推导出了退化压力和体积模量的广义关系。一个有趣的发现是,退化压力减小了,这一点可以从观测到的白矮星的大小得到证实,它比标准理论预测的要小。尽管如此,它仍然能够为防止引力坍缩提供支持。
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引用次数: 0
Micro-cosmos model of a nucleon 核子的微宇宙模型
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-05-04 DOI: 10.1142/s0217732324500536
Michael Cramer Andersen

This study explores the age-old quest to construct a geometric model of a quantum particle. While static classical particle models have largely been dismissed, the focus has now shifted to intricate dynamic models that hold the promise of reconciling general relativity with quantum mechanics. We propose that matter particles can be described as radiation confined within dynamically curved spacetime regions, without the need for quantization of space and time, and using standard field equations and natural Planck units. Specifically, we investigate a cyclic or oscillating radiation-dominated micro-cosmos undergoing repeated bouncing. Our methodology employs integration, with carefully defined initial conditions. The results include several observable properties characteristic of quantum particles. We calculate the total mass, revealing a compelling inverse proportionality between mass and radius identical with the de Broglie relationship. Applying this model to protons, we discover a profound and surprisingly simple relationship between the proton’s radius and mass expressed in Planck units. This enables a definition of the proton radius that aligns remarkably well with the 2018 CODATA value. Furthermore, our analysis demonstrates that the radial density profile of the proton (or nucleon), averaged over a cycle time, increases toward the center. The problem of embedding the micro-cosmos within a background spacetime is also described. These results underscore the relevance of general relativity in the domain of nuclear physics. Moreover, the model offers a fresh perspective that can stimulate new ideas in the ongoing quest to unify general relativity with quantum physics.

本研究探讨了构建量子粒子几何模型的古老探索。尽管静态经典粒子模型在很大程度上已被否定,但现在的焦点已转移到复杂的动态模型上,这些模型有望调和广义相对论与量子力学。我们提出,物质粒子可以描述为限制在动态弯曲时空区域内的辐射,而无需量化空间和时间,并使用标准场方程和自然普朗克单位。具体来说,我们研究的是一个循环或振荡的辐射主导的微宇宙,它经历着反复的反弹。我们的研究方法采用积分法,并仔细定义了初始条件。研究结果包括量子粒子的几个可观测特性。我们计算了总质量,揭示了质量与半径之间令人信服的反比关系,与德布罗意关系相同。将这一模型应用于质子,我们发现质子的半径与以普朗克单位表示的质量之间存在着深刻而令人惊讶的简单关系。这使得质子半径的定义与 2018 年 CODATA 数值非常吻合。此外,我们的分析表明,质子(或核子)的径向密度剖面在一个周期时间内的平均值向中心增加。我们还描述了将微宇宙嵌入背景时空的问题。这些结果强调了广义相对论在核物理领域的相关性。此外,该模型还提供了一个崭新的视角,可以激发人们在不断寻求广义相对论与量子物理学统一的过程中产生新的想法。
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引用次数: 0
A novel quantum dialogue without information leakage based on single photons in both polarization and spatial-mode degrees of freedom 基于偏振和空间模式自由度单光子的无信息泄露新型量子对话
IF 1.4 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-04-26 DOI: 10.1142/s0217732324500354
Shen Rao

This paper puts forward a novel quantum dialogue (QD) protocol without information leakage based on single photons in both polarization and spatial-mode degrees of freedom. In this protocol, the receiver sends his private message to the sender in the way of quantum secure direct communication; and the receiver decodes out the private message of the sender with the help of auxiliary single photons in two degrees of freedom, double controlled-not (CNOT) operations and an auxiliary classical bit sequence sent from the sender. As a result, no information leakage takes place. Moreover, this protocol is proven to defeat the intercept-resend attack, the measure-resend attack, the entangle-measure attack and the Trojan horse attack from an outside eavesdropper. This protocol only employs single photons in two degrees of freedom as quantum resource and needs single-photon measurements. The qubit efficiency of this protocol is as high as 66.7%.

本文基于偏振和空间模式两个自由度的单光子,提出了一种无信息泄露的新型量子对话(QD)协议。在该协议中,接收方以量子安全直接通信的方式向发送方发送自己的私人信息;接收方则借助发送方发送的两个自由度的辅助单光子、双受控不(CNOT)操作和辅助经典比特序列解码出发送方的私人信息。因此,不会发生信息泄露。此外,该协议还被证明可以击败外部窃听者的拦截-发送攻击、测量-发送攻击、纠缠-测量攻击和木马攻击。该协议仅使用两个自由度的单光子作为量子资源,并需要单光子测量。该协议的量子比特效率高达 66.7%。
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引用次数: 0
期刊
Modern Physics Letters A
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