派博傳思國(guó)際中心

標(biāo)題: Titlebook: Cosmological Probes of Light Relics; Benjamin Wallisch Book 2019 The Editor(s) (if applicable) and The Author(s), under exclusive license [打印本頁]

作者: Tamoxifen    時(shí)間: 2025-3-21 20:00
書目名稱Cosmological Probes of Light Relics影響因子(影響力)




書目名稱Cosmological Probes of Light Relics影響因子(影響力)學(xué)科排名




書目名稱Cosmological Probes of Light Relics網(wǎng)絡(luò)公開度




書目名稱Cosmological Probes of Light Relics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Cosmological Probes of Light Relics被引頻次




書目名稱Cosmological Probes of Light Relics被引頻次學(xué)科排名




書目名稱Cosmological Probes of Light Relics年度引用




書目名稱Cosmological Probes of Light Relics年度引用學(xué)科排名




書目名稱Cosmological Probes of Light Relics讀者反饋




書目名稱Cosmological Probes of Light Relics讀者反饋學(xué)科排名





作者: 易于出錯(cuò)    時(shí)間: 2025-3-21 20:30

作者: ineffectual    時(shí)間: 2025-3-22 01:35

作者: 連詞    時(shí)間: 2025-3-22 05:44

作者: monogamy    時(shí)間: 2025-3-22 12:31
Searching for Light Relics with the CMB,s through the sensitivity to this effect that the recent CMB?data has provided a robust detection of free-streaming neutrinos. In this chapter, we revisit the phase shift of the CMB?anisotropy spectrum as a probe of new physics. The phase shift is particularly interesting because its physical origin
作者: Stagger    時(shí)間: 2025-3-22 13:28
Searching for Light Relics with LSS, constrained to be less than ten percent of the total energy density in radiation. Upcoming cosmic microwave background (CMB) experiments, however, have the potential to measure the radiation density at the one-percent level, which is close to well-motivated theoretical targets. In this chapter, we
作者: Stagger    時(shí)間: 2025-3-22 17:58
Measurement of Neutrinos in the BAO Spectrum, energy density in the early universe and, therefore, played an important role in the evolution of cosmological perturbations. In particular, fluctuations in the neutrino density produced a distinct shift in the temporal phase of sound waves in the primordial plasma. In this chapter, we report on th
作者: 行為    時(shí)間: 2025-3-22 21:54
Conclusions and Outlook,ot only become precise enough to answer questions about the universe at large, but also to start addressing puzzles in the microscopic description of Nature. Cosmological measurements are particularly well suited to study Standard Model neutrinos and to shed light on the possible existence of other
作者: crumble    時(shí)間: 2025-3-23 04:01
Light Species in Cosmology and Particle Physics,mates for the constraining power of astrophysical systems and cosmology, we introduce the particle physics aspects of this thesis, discuss the main cosmological parameter capturing neutrinos and any other light thermal relics, and examine the possible signatures of these particles in cosmological observables.
作者: 闖入    時(shí)間: 2025-3-23 09:36

作者: 載貨清單    時(shí)間: 2025-3-23 13:00
2190-5053 icle physics through analytic insights, numerical computatioThe wealth of recent cosmic microwave background and large-scale structure data has transformed the field of cosmology. These observations have not only become precise enough to answer questions about the universe on the largest scales, but
作者: 嘴唇可修剪    時(shí)間: 2025-3-23 16:05
Tabellen- und Abbildungsverzeichnis,mology. We consider in particular the basics underlying the standard model of cosmology, the thermal history of the universe and the fluctuations around the smooth universe. In addition, we review the main cosmological observables: the cosmic microwave background, the large-scale structure of the universe and the baryon acoustic oscillations.
作者: 無法取消    時(shí)間: 2025-3-23 21:52
Soziale Gerechtigkeit und Demokratie,Nature. Cosmological measurements are particularly well suited to study Standard Model neutrinos and to shed light on the possible existence of other light relics beyond the Standard Model. In this chapter, we summarize the main results of this thesis and make a few remarks on future directions.
作者: Anecdote    時(shí)間: 2025-3-23 23:10

作者: 深淵    時(shí)間: 2025-3-24 04:57
Conclusions and Outlook,Nature. Cosmological measurements are particularly well suited to study Standard Model neutrinos and to shed light on the possible existence of other light relics beyond the Standard Model. In this chapter, we summarize the main results of this thesis and make a few remarks on future directions.
作者: HAVOC    時(shí)間: 2025-3-24 08:46
Soziale Gerechtigkeit und Demokratie,mates for the constraining power of astrophysical systems and cosmology, we introduce the particle physics aspects of this thesis, discuss the main cosmological parameter capturing neutrinos and any other light thermal relics, and examine the possible signatures of these particles in cosmological observables.
作者: Gossamer    時(shí)間: 2025-3-24 11:21

作者: 有發(fā)明天才    時(shí)間: 2025-3-24 17:19
Alexander Bogner,Helge Torgersenpectrum can significantly improve on current and near-term CMB experiments. We also propose a modified analysis of BAO data and show that the phase shift induced by relic neutrinos in the BAO spectrum can be detected at high significance in future experiments.
作者: 蝕刻術(shù)    時(shí)間: 2025-3-24 22:41
Alexander Bogner,Helge Torgersenence for a non-zero phase shift at greater than 95simulations and forecasts. Besides providing a new measurement of the cosmic neutrino background, this work is the first application of the BAO feature beyond its application as a standard ruler and to early universe physics.
作者: BARK    時(shí)間: 2025-3-25 00:31

作者: GENRE    時(shí)間: 2025-3-25 04:42
Measurement of Neutrinos in the BAO Spectrum,ence for a non-zero phase shift at greater than 95simulations and forecasts. Besides providing a new measurement of the cosmic neutrino background, this work is the first application of the BAO feature beyond its application as a standard ruler and to early universe physics.
作者: 粗語    時(shí)間: 2025-3-25 08:00
J?rg Faust,Hans-Joachim Lauth,Wolfgang Munodel. In this chapter, we give a concise introduction to the topic of this thesis, the search for these elusive particles by identifying and extracting their robust signatures in cosmological observables. Moreover, we outline the rest of the thesis and provide a collection of the employed notation and conventions.
作者: obsession    時(shí)間: 2025-3-25 11:41
Introduction,del. In this chapter, we give a concise introduction to the topic of this thesis, the search for these elusive particles by identifying and extracting their robust signatures in cosmological observables. Moreover, we outline the rest of the thesis and provide a collection of the employed notation and conventions.
作者: Acumen    時(shí)間: 2025-3-25 16:04
Book 2019ly become precise enough to answer questions about the universe on the largest scales, but also to address puzzles in the microscopic description of Nature. This thesis investigates new ways of probing the early universe, the properties of neutrinos and the possible existence of other light particle
作者: 項(xiàng)目    時(shí)間: 2025-3-25 22:51
2190-5053 icles thathave ever been in thermal equilibrium or imply strong bounds on their properties..? ? ? ? ? ? ? ? ? ? ? ? ? ? ?.978-3-030-31100-1978-3-030-31098-1Series ISSN 2190-5053 Series E-ISSN 2190-5061
作者: JEER    時(shí)間: 2025-3-26 01:34
Searching for Light Relics with the CMB,t simple models to illustrate each of these effects and provide observational constraints from the Planck temperature and polarization data on additional forms of radiation. We also estimate the capabilities of future CMB?Stage-4 experiments. Whenever possible, we give analytic interpretations and c
作者: EXALT    時(shí)間: 2025-3-26 05:11

作者: 串通    時(shí)間: 2025-3-26 09:06

作者: overwrought    時(shí)間: 2025-3-26 14:00
https://doi.org/10.1007/978-3-030-31098-1Cosmic Neutrinos/Cosmic Neutrino Background; Light Thermal Relics; Early Universe Cosmology; Cosmologic
作者: 破譯    時(shí)間: 2025-3-26 19:47

作者: 野蠻    時(shí)間: 2025-3-27 00:14

作者: 遠(yuǎn)足    時(shí)間: 2025-3-27 04:36

作者: forager    時(shí)間: 2025-3-27 07:41
Soziale Gerechtigkeit und Demokratie,e new degrees of freedom, many of which contain new light species that are efficiently produced in the early universe. In this chapter, we provide the connection between cosmological observables and these additional light relics predicted beyond the Standard Model. Apart from order-of-magnitude esti
作者: 法律的瑕疵    時(shí)間: 2025-3-27 13:03
Soziale Gerechtigkeit und Demokratie,he potential to explore a fundamentally new territory of physics beyond the Standard Model. Specifically, observations may become sensitive to any light relics that have ever been in thermal equilibrium with the Standard Model. In this chapter, we demonstrate that even the absence of a detection wou
作者: LAY    時(shí)間: 2025-3-27 17:07
Alexander Bogner,Helge Torgersens through the sensitivity to this effect that the recent CMB?data has provided a robust detection of free-streaming neutrinos. In this chapter, we revisit the phase shift of the CMB?anisotropy spectrum as a probe of new physics. The phase shift is particularly interesting because its physical origin
作者: AFFIX    時(shí)間: 2025-3-27 21:40
Alexander Bogner,Helge Torgersen constrained to be less than ten percent of the total energy density in radiation. Upcoming cosmic microwave background (CMB) experiments, however, have the potential to measure the radiation density at the one-percent level, which is close to well-motivated theoretical targets. In this chapter, we
作者: CIS    時(shí)間: 2025-3-28 00:16

作者: 鈍劍    時(shí)間: 2025-3-28 03:19

作者: Vital-Signs    時(shí)間: 2025-3-28 09:37
Cosmological Probes of Light Relics978-3-030-31098-1Series ISSN 2190-5053 Series E-ISSN 2190-5061
作者: Relinquish    時(shí)間: 2025-3-28 14:14





歡迎光臨 派博傳思國(guó)際中心 (http://www.yitongpaimai.cn/) Powered by Discuz! X3.5
开化县| 濉溪县| 黄大仙区| 巴青县| 梨树县| 漯河市| 桓台县| 察隅县| 衡阳县| 台州市| 沧州市| 韶山市| 东兴市| 兴隆县| 遵义市| 双鸭山市| 离岛区| 安乡县| 石嘴山市| 故城县| 马边| 金堂县| 白沙| 清镇市| 新巴尔虎左旗| 汕头市| 平阳县| 工布江达县| 靖西县| 清流县| 彩票| 龙川县| 监利县| 屏边| 天全县| 涿鹿县| 芮城县| 运城市| 老河口市| 朝阳县| 龙岩市|