Below the Schwinger critical magnetic field value, quantum vacuum and gamma-ray bursts delay

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2025-02-01 Epub Date: 2025-01-16 DOI:10.1016/j.physletb.2025.139272
Iver H. Brevik , Moshe M. Chaichian , Anca Tureanu
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Abstract

A magnetic field above the Schwinger critical value Bcrit=109 Tesla is much higher than any magnetic field known by now in the interstellar bulk except in the vicinity of observed magnetars having magnetic fields between 109 and 1011 Tesla. Above the critical magnetic field limit, calculated by Schwinger in the lowest order perturbation in quantum electrodynamics (QED), one reaches the threshold for electron-positron pair creation (through the intermediate electric field, as known also from standard electrodynamics), which has interesting consequences. Therefore, finding out whether one could encounter some consequences of interest also for the values of the magnetic field below the Schwinger critical point, we invoke the next higher-order effect in QED, which is emerging from the Quantum Vacuum Effect. The latter is equivalent to the use of the Euler-Heisenberg effective theory in nonlinear electrodynamics, where the Lagrangian has now a term with a higher power, B4. In this case, in the region B<Bcrit, we show that interesting effects appear, among them the Cherenkov radiation and the reduction in the speed of light. The latter effects appear due to the quantum vacuum mimicking a medium. We also present quantitative arguments for such a close analogy. As a rough estimate, we show that the time delay τ of gamma-ray bursts (GRB) having traveled through the entire cosmological distances in an average strong magnetic field such as 106 Tesla, reaches an experimentally considerable value of τ=2.4 hours. Of course in the vicinity of magnetars, the magnetic field is much stronger, of the order of 1091011 Tesla. However, in this case the linear scale of GRB trajectory through such regions would be much smaller. For the latter, we also give a corresponding estimate for the number of the magnetars along the trajectory and also for the delay. Finally, we shall dwell on the recently raised issue in the literature, namely the Lorentz invariance violation (LIV).
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在施温格临界磁场值以下,量子真空和伽马射线爆发延迟
超过Schwinger临界值Bcrit=109特斯拉的磁场比目前已知的星际体中的任何磁场都要高得多,除了在观测到的磁场在109到1011特斯拉之间的磁星附近。在由Schwinger在量子电动力学(QED)的最低阶扰动中计算的临界磁场极限之上,人们达到了电子-正电子对产生的阈值(通过中间电场,也从标准电动力学中知道),这有有趣的后果。因此,为了找出在施温格临界点以下的磁场值是否也会遇到一些有趣的结果,我们调用了QED中的下一个高阶效应,它是从量子真空效应中出现的。后者相当于在非线性电动力学中使用欧拉-海森堡有效理论,其中拉格朗日量现在有一个更高幂的项,B4。在这种情况下,在区域B<;Bcrit中,我们展示了有趣的效应,其中包括切伦科夫辐射和光速的降低。后一种效应的出现是由于量子真空模拟了一种介质。我们也为这种相近的类比提出了定量论证。粗略估计,伽玛射线暴(GRB)在106特斯拉等平均强磁场中穿越整个宇宙距离的时间延迟τ在实验上达到相当可观的τ=2.4小时。当然,在磁星附近,磁场要强得多,约为109−1011特斯拉。然而,在这种情况下,GRB轨迹通过这些区域的线性尺度会小得多。对于后者,我们也给出了沿轨迹的磁星数和延迟的相应估计。最后,我们将详细讨论最近在文献中提出的问题,即洛伦兹不变性违反(LIV)。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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