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The EDGES collaboration's observation of an anomalously strong 21 cm absorption feature around the cosmic dawn era has energised the cosmological community by suggesting a novel signature of dark matter in the cooling of cosmic hydrogen. In…

高能物理 - 唯象学 · 物理学 2021-03-16 Chuang Li , Nick Houston , Tianjun Li , Qiaoli Yang , Xin Zhang

Recently the EDGES collaboration reported an anomalous absorption signal in the sky-averaged 21-cm spectrum around $z=17$. Such a signal may be understood as an indication for an unexpected cooling of the hydrogen gas during or prior to the…

高能物理 - 唯象学 · 物理学 2018-11-14 Rennan Barkana , Nadav Joseph Outmezguine , Diego Redigolo , Tomer Volansky

The recently claimed anomaly in the measurement of the 21 cm hydrogen absorption signal by EDGES at $z\sim 17$, if cosmological, requires the existence of new physics. The possible attempts to resolve the anomaly rely on either (i) cooling…

Recently the EDGES experiment reported an enhanced 21cm absorption signal in the radio wave observation, which may be interpreted as either anomalous cooling of baryons or heating of cosmic microwave background photons. In this paper, we…

高能物理 - 唯象学 · 物理学 2018-07-10 Takeo Moroi , Kazunori Nakayama , Yong Tang

A hypothetical particle known as the axion holds the potential to resolve both the cosmic dark matter riddle and particle physics' long-standing, strong CP dilemma. An unusually strong 21-cm absorption feature associated with the initial…

高能物理 - 唯象学 · 物理学 2025-10-17 C. R. Das

Any particle dark matter (DM) scenario featuring a suppressed power spectrum of astrophysical relevance results in a delay of galaxy formation. As a consequence, such scenarios can be constrained using the global 21-cm absorption signal…

宇宙学与河外天体物理 · 物理学 2018-10-03 Aurel Schneider

We argue that dark matter in the form of macroscopically large nuggets of standard model quarks and antiquarks can help to alleviate the tension between standard model cosmology and the recent EDGES observation of a stronger than…

高能物理 - 唯象学 · 物理学 2019-03-19 K. Lawson , A. R. Zhitnitsky

The EDGES Collaboration has recently reported the detection of a stronger-than-expected absorption feature in the global 21-cm spectrum, centered at a frequency corresponding to a redshift of z ~ 17. This observation has been interpreted as…

高能物理 - 唯象学 · 物理学 2018-07-11 Asher Berlin , Dan Hooper , Gordan Krnjaic , Samuel D. McDermott

In the standard cosmology, it is believed that there are two relatively weak and distinct band-limited absorption features, with the first absorption minima near 20 MHz ($z\sim70$) and the other minima at higher frequencies between 50-110…

宇宙学与河外天体物理 · 物理学 2023-06-08 Mansi Dhuria , Viraj Karambelkar , Vikram Rentala , Priyanka Sarmah

It was shown in ref. [1] that cold dark matter axions reach thermal contact with baryons, and therefore cool them, shortly after the axions thermalize among themselves and form a Bose-Einstein condensate. The recent observation by the EDGES…

宇宙学与河外天体物理 · 物理学 2018-08-02 Pierre Sikivie

The EDGES Collaboration has recently announced the detection of the 21-cm spectrum with an absorption profile centred at $78$ megahertz, of which the depth is deeper than that expected by the standard cosmological paradigm. To enrich the…

宇宙学与河外天体物理 · 物理学 2018-12-03 Chunlong Li , Yi-Fu Cai

The EDGES experiment has detected the global absorption signal of 21 cm line at $z\sim17$ in cosmic dawn era and reported its amplitude larger than the standard cosmological prediction. One of the possible explanation requires that the…

宇宙学与河外天体物理 · 物理学 2019-10-02 Jitesh R. Bhatt , Arvind Kumar Mishra , Alekha C. Nayak

Recently the EDGES experiment has claimed the detection of an absorption feature centered at 78 MHz. When interpreted as a signature of cosmic dawn, this feature appears at the correct wavelength (corresponding to a redshift range of…

高能天体物理现象 · 物理学 2018-08-15 Prateek Sharma

We are approaching a new era to probe the 21-cm neutral hydrogen signal from the period of cosmic dawn. This signal offers a unique window to the virgin Universe, e.g., to study dark matter models with different small-scale behaviours. The…

宇宙学与河外天体物理 · 物理学 2021-06-21 Venno Vipp , Andi Hektor , Gert Hütsi

The recent observation of the 21-cm absorption signal by the EDGES experiment provides a new observational window into the dynamics of the young Universe. Based on this result, we constrain the properties of ALPs and excited dark matter via…

高能物理 - 唯象学 · 物理学 2018-09-12 Andi Hektor , Gert Hütsi , Luca Marzola , Ville Vaskonen

The EDGES collaboration has recently reported the detection of an unexpectedly stronger absorption signal in the global 21-cm spectrum around cosmic red-shift z = 17, resulting in the significant cooling of the primordial gas. The cooling…

高能物理 - 唯象学 · 物理学 2019-11-20 Mansi Dhuria

Measurements of the temperature of the baryons at the end of the cosmic dark ages can potentially set very precise constraints on energy injection from exotic sources, such as annihilation or decay of the dark matter. However, additional…

宇宙学与河外天体物理 · 物理学 2018-07-11 Hongwan Liu , Tracy R. Slatyer

The EDGES experiment has observed an absorption feature in the global 21 cm spectrum with a surprisingly large amplitude. These results can be explained by decreasing the kinetic temperature of baryons, which could be achieved through the…

宇宙学与河外天体物理 · 物理学 2018-12-07 Yupeng Yang

Observations of the redshifted 21-cm signal (in absorption or emission) allow us to peek into the epoch of "dark ages" and the onset of reionization. These data can provide a novel way to learn about the nature of dark matter, in particular…

宇宙学与河外天体物理 · 物理学 2019-12-11 Alexey Boyarsky , Dmytro Iakubovskyi , Oleg Ruchayskiy , Anton Rudakovskyi , Wessel Valkenburg

The recently announced result by EDGES points an unexpected excess in the 21 cm global brightness temperature from cosmic dawn at $z\sim 17$, potentially indicating new phenomena beyond the $\Lambda$CDM model. A generic cosmological model…

宇宙学与河外天体物理 · 物理学 2019-02-06 Linfeng Xiao , Rui An , Le Zhang , Bin Yue , Yidong Xu , Bin Wang
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