异常微波发射功率的估计

Kristopher T. Pickens, G. Scarel
{"title":"异常微波发射功率的估计","authors":"Kristopher T. Pickens, G. Scarel","doi":"10.4236/wjcmp.2020.103007","DOIUrl":null,"url":null,"abstract":"Context \nand Background: The product of the electromagnetic (EM) wave’s \npower P times its period τ, i.e. Pτ, is the amount of energy conserved \nin EM wave’s absorption in matter. Whether Pτ is the amount of energy conserved in the emission of EM waves from matter is \nnot assessed. Motivation: In this research, \nwe perform a computational study to explore the ability of Pτ to represent the \namount of energy conserved in EM wave’s emission from matter. Hypothesis: Since the magnitude of the power P of \nemitted EM waves computed through Larmor’s formula for a rotating dipole is \nexcessively small, we alternatively hypothesize that Pτ and the law of conservation of energy can lead to a realistic \nestimation of P. Methods: We \nestimate the power PAME of \nthe anomalous microwave emission (AME), a well-characterized radiation \ngenerated in the interstellar medium (ISM) by spinning dust grains, and one possible source of contamination of the cosmic \nmicrowave background (CMB). For our estimation of PAME, we assume the AME to be generated in a molecular \ncloud mostly populated by spinning silicate nanoparticles (SSNs) or polycyclic \naromatic hydrocarbon (PAH) spinning dust grains. Indeed, SSNs and PAHs are \nlisted among the most probable sources of AME, and their characteristics are \nwell-known. We discriminate between realistic and non-realistic values of PAME based upon the magnitude \nof two parameters that depend on PAME: \nthe significant distance z, and the \ntime of photon production T. The \nparameter z is the space interval from the spinning dust grain within which the \nspinning dust grain’s electric field is effective. Results: Using the \ninformation available for AME, SSNs and PAHs, we estimate the power PAME using both Larmor’s \nformula and Pτ. We compare and \ncomment the results obtained for z and T. Conclusions: Our study \nhighlights the effectiveness of Pτ over \nLarmor’s formula in providing a realistic value of PAME. This finding might have consequences in quantum \ntechnology of single photon detection and production.","PeriodicalId":308307,"journal":{"name":"World Journal of Condensed Matter Physics","volume":"104 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-06-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Estimation of the Power of the Anomalous Microwave Emission\",\"authors\":\"Kristopher T. Pickens, G. Scarel\",\"doi\":\"10.4236/wjcmp.2020.103007\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Context \\nand Background: The product of the electromagnetic (EM) wave’s \\npower P times its period τ, i.e. Pτ, is the amount of energy conserved \\nin EM wave’s absorption in matter. Whether Pτ is the amount of energy conserved in the emission of EM waves from matter is \\nnot assessed. Motivation: In this research, \\nwe perform a computational study to explore the ability of Pτ to represent the \\namount of energy conserved in EM wave’s emission from matter. Hypothesis: Since the magnitude of the power P of \\nemitted EM waves computed through Larmor’s formula for a rotating dipole is \\nexcessively small, we alternatively hypothesize that Pτ and the law of conservation of energy can lead to a realistic \\nestimation of P. Methods: We \\nestimate the power PAME of \\nthe anomalous microwave emission (AME), a well-characterized radiation \\ngenerated in the interstellar medium (ISM) by spinning dust grains, and one possible source of contamination of the cosmic \\nmicrowave background (CMB). For our estimation of PAME, we assume the AME to be generated in a molecular \\ncloud mostly populated by spinning silicate nanoparticles (SSNs) or polycyclic \\naromatic hydrocarbon (PAH) spinning dust grains. Indeed, SSNs and PAHs are \\nlisted among the most probable sources of AME, and their characteristics are \\nwell-known. We discriminate between realistic and non-realistic values of PAME based upon the magnitude \\nof two parameters that depend on PAME: \\nthe significant distance z, and the \\ntime of photon production T. The \\nparameter z is the space interval from the spinning dust grain within which the \\nspinning dust grain’s electric field is effective. Results: Using the \\ninformation available for AME, SSNs and PAHs, we estimate the power PAME using both Larmor’s \\nformula and Pτ. We compare and \\ncomment the results obtained for z and T. Conclusions: Our study \\nhighlights the effectiveness of Pτ over \\nLarmor’s formula in providing a realistic value of PAME. This finding might have consequences in quantum \\ntechnology of single photon detection and production.\",\"PeriodicalId\":308307,\"journal\":{\"name\":\"World Journal of Condensed Matter Physics\",\"volume\":\"104 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-06-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"World Journal of Condensed Matter Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.4236/wjcmp.2020.103007\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"World Journal of Condensed Matter Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.4236/wjcmp.2020.103007","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

背景与背景:电磁波的功率P与其周期τ的乘积,即Pτ,是电磁波在物质中吸收所保留的能量。Pτ是否为物质发射电磁波时所保留的能量,尚未得到评估。动机:在本研究中,我们进行了一项计算研究,以探索Pτ表示物质电磁波发射中守恒能量的能力。假设:由于通过旋转偶极子的Larmor公式计算的发射电磁波的功率P的大小太小,我们可以假设Pτ和能量守恒定律可以导致P的现实估计。我们估计了异常微波发射(AME)的功率PAME,这是一种在星际介质(ISM)中由旋转尘埃颗粒产生的具有良好特征的辐射,也是宇宙微波背景(CMB)可能的污染源之一。对于PAME的估计,我们假设AME是在一个分子云中产生的,该分子云主要由旋转的硅酸盐纳米颗粒(SSNs)或多环芳烃(PAH)旋转的粉尘颗粒组成。事实上,ssn和PAHs被列为AME最可能的来源,它们的特征是众所周知的。我们根据与PAME相关的两个参数的大小来区分PAME的真实值和非真实值:有效距离z和光子产生时间t。参数z是旋转尘埃颗粒的空间间隔,在此范围内旋转尘埃颗粒的电场是有效的。结果:利用AME, ssn和PAHs的可用信息,我们使用Larmor公式和Pτ来估计PAME的功率。我们对z和t的结果进行了比较和评论。结论:我们的研究强调了Pτ比Larmor公式在提供PAME的实际值方面的有效性。这一发现可能对单光子探测和产生的量子技术产生影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Estimation of the Power of the Anomalous Microwave Emission
Context and Background: The product of the electromagnetic (EM) wave’s power P times its period τ, i.e. Pτ, is the amount of energy conserved in EM wave’s absorption in matter. Whether Pτ is the amount of energy conserved in the emission of EM waves from matter is not assessed. Motivation: In this research, we perform a computational study to explore the ability of Pτ to represent the amount of energy conserved in EM wave’s emission from matter. Hypothesis: Since the magnitude of the power P of emitted EM waves computed through Larmor’s formula for a rotating dipole is excessively small, we alternatively hypothesize that Pτ and the law of conservation of energy can lead to a realistic estimation of P. Methods: We estimate the power PAME of the anomalous microwave emission (AME), a well-characterized radiation generated in the interstellar medium (ISM) by spinning dust grains, and one possible source of contamination of the cosmic microwave background (CMB). For our estimation of PAME, we assume the AME to be generated in a molecular cloud mostly populated by spinning silicate nanoparticles (SSNs) or polycyclic aromatic hydrocarbon (PAH) spinning dust grains. Indeed, SSNs and PAHs are listed among the most probable sources of AME, and their characteristics are well-known. We discriminate between realistic and non-realistic values of PAME based upon the magnitude of two parameters that depend on PAME: the significant distance z, and the time of photon production T. The parameter z is the space interval from the spinning dust grain within which the spinning dust grain’s electric field is effective. Results: Using the information available for AME, SSNs and PAHs, we estimate the power PAME using both Larmor’s formula and Pτ. We compare and comment the results obtained for z and T. Conclusions: Our study highlights the effectiveness of Pτ over Larmor’s formula in providing a realistic value of PAME. This finding might have consequences in quantum technology of single photon detection and production.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信