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A NEW INSIGHT INTO NEUTRINO ENERGY LOSS BY ELECTRON CAPTURE OF IRON GROUP NUCLEI IN MAGNETAR SURFACES

机译:铁原子团核的电子俘获对中微子能量损失的新认识

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摘要

Based on the relativistic mean-field effective interactions theory, and the Lai dong model, we discuss the influences of superstrong magnetic fields (SMFs) on electron Fermi energy, nuclear blinding energy, and single-particle level structure in magnetar surfaces. Using the Shell-Model Monte Carlo method and the Random Phase Approximation theory, we analyze the neutrino energy loss rates (NELRs) by electron capture for iron group nuclei in SMFs. First, when B-12 < 100, we find that the SMFs have a slight influence on the NELRs for most nuclides at relativistic low temperatures (e.g., T-9 = 0.233); nevertheless, the NELRs increase by more than four orders of magnitude at relativistic high temperatures (e.g., T-9 = 15.53). When B-12 > 100, the NELRs decrease by more than three orders of magnitude (e.g., at T-9 = 15.53 for Fe52-61, Co55-60, and Ni56-63). Second, for a certain value of magnetic field and temperature, the NELRs increase by more than four orders of magnitude when rho(7) <= 10(3), but as the density increases (i.e., when rho(7) > 10(3)), there is almost no influence on the density of NELRs. For the density around rho(7) = 10(2), there is an abrupt increase in NELRs when B-12 >= 10(3.)5. Such jumps are an indication that the underlying shell structure has changed due to single-particle behavior by SMFs. Finally, we compare our NELRs with those of Fuller et al. (FFN) and Nabi & Klapdor-Kleingrothaus (NKK). For the case without SMFs, one finds that our rates for certain nuclei are close to about five orders of magnitude lower than FFN and NKK at relativistic low temperatures (e.g., T-9 = 1). However, at a relativistic high temperature (e.g., T-9 = 3), our results are in good agreement with NKK, but about one order of magnitude lower than FFN. For the case with SMFs, our NELRs for some iron group nuclei can be about five orders of magnitude higher than those of FFN and NKK. (Note that B-12, T-9, and rho(7) are in units of 10(12) G, 10(9) K, and 10(7)g cm(-3), respectively.)
机译:基于相对论平均场有效相互作用理论和赖东模型,我们讨论了超强磁场(SMF)对磁表面电子费米能,核致盲能和单粒子能级结构的影响。使用壳模型蒙特卡洛方法和随机相位逼近理论,我们通过电子捕获分析了SMF中铁基核的中微子能量损失率(NELR)。首先,当B-12 <100时,我们发现相对论低温下大多数核素的SMF对NELR都有轻微影响(例如T-9 = 0.233);尽管如此,NELR在相对论高温下(例如T-9 = 15.53)会增加四个数量级以上。当B-12> 100时,NELR降低三个数量级以上(例如,对于Fe52-61,Co55-60和Ni56-63,T-9 = 15.53)。其次,对于一定的磁场和温度值,当rho(7)<= 10(3)时,NELR会增加四个数量级以上,但随着密度的增加(即rho(7)> 10( 3)),对NELR的密度几乎没有影响。对于rho(7)= 10(2)附近的密度,当B-12> = 10(3.)5时NELR会突然增加。这种跳跃表明,由于SMF的单粒子行为,底层的壳结构已发生变化。最后,我们将我们的NELR与Fuller等人的进行了比较。 (FFN)和Nabi&Klapdor-Kleingrothaus(NKK)。对于没有SMF的情况,人们发现在相对论低温下(例如T-9 = 1),我们对某些核的比率比FFN和NKK低大约五个数量级。但是,在相对论的高温下(例如T-9 = 3),我们的结果与NKK吻合良好,但比FFN低约一个数量级。就SMF而言,我们对某些铁族核的NELR可以比FFN和NKK高约5个数量级。 (请注意,B-12,T-9和rho(7)分别以10(12)G,10(9)K和10(7)g cm(-3)为单位。)

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