Dark Matter /ness/ en Possible Interaction between Baryons and Dark-matter Particles Revealed by the First Stars /ness/2018/03/01/possible-interaction-between-baryons-and-dark-matter-particles-revealed-first-stars <span>Possible Interaction between Baryons and Dark-matter Particles Revealed by the First Stars</span> <span><span>Anonymous (not verified)</span></span> <span><time datetime="2018-03-01T08:41:21-07:00" title="Thursday, March 1, 2018 - 08:41">Thu, 03/01/2018 - 08:41</time> </span> <div> <div class="imageMediaStyle focal_image_wide"> <img loading="lazy" src="/ness/sites/default/files/styles/focal_image_wide/public/article-thumbnail/nature_6.jpg?h=14961dfa&amp;itok=f_IppdVn" width="1200" height="600" alt="Nature logo"> </div> </div> <div role="contentinfo" class="container ucb-article-categories" itemprop="about"> <span class="visually-hidden">Categories:</span> <div class="ucb-article-category-icon" aria-hidden="true"> <i class="fa-solid fa-folder-open"></i> </div> <a href="/ness/taxonomy/term/6"> News </a> </div> <div role="contentinfo" class="container ucb-article-tags" itemprop="keywords"> <span class="visually-hidden">Tags:</span> <div class="ucb-article-tag-icon" aria-hidden="true"> <i class="fa-solid fa-tags"></i> </div> <a href="/ness/taxonomy/term/350" hreflang="en">Baryonic matter</a> <a href="/ness/taxonomy/term/348" hreflang="en">Cosmic radio-frequency spectrum</a> <a href="/ness/taxonomy/term/352" hreflang="en">Dark Matter</a> </div> <span>Rennan Barkana</span> <div class="ucb-article-content ucb-striped-content"> <div class="container"> <div class="paragraph paragraph--type--article-content paragraph--view-mode--default"> <div class="ucb-article-content-media ucb-article-content-media-above"> <div> <div class="paragraph paragraph--type--media paragraph--view-mode--default"> <div> <div class="imageMediaStyle large_image_style"> <img loading="lazy" src="/ness/sites/default/files/styles/large_image_style/public/article-image/nature.jpg?itok=zgez0fY0" width="1500" height="1150" alt="Nature logo"> </div> </div> </div> </div> </div> <div class="ucb-article-text d-flex align-items-center" itemprop="articleBody"> <div><p><strong>From Nature:</strong>&nbsp;The cosmic radio-frequency spectrum is expected to show a strong absorption signal corresponding to the 21-centimetre-wavelength transition of atomic hydrogen around redshift 20, which arises from Lyman-α radiation from some of the earliest stars. By observing this 21-centimetre signal—either its sky-averaged spectrum&nbsp;or maps of its fluctuations, obtained using radio interferometers - we can obtain information about cosmic dawn, the era when the first astrophysical sources of light were formed. The recent detection of the global 21-centimetre spectrum&nbsp;reveals a stronger absorption than the maximum predicted by existing models, at a confidence level of 3.8 standard deviations. Here we report that this absorption can be explained by the combination of radiation from the first stars and excess cooling of the cosmic gas induced by its interaction with dark matter. Our analysis indicates that the spatial fluctuations of the 21-centimetre signal at cosmic dawn could be an order of magnitude larger than previously expected and that the dark-matter particle is no heavier than several proton masses, well below the commonly predicted mass of weakly interacting massive particles. Our analysis also confirms that dark matter is highly non-relativistic and at least moderately cold, and primordial velocities predicted by models of warm dark matter are potentially detectable. These results indicate that 21-centimetre cosmology can be used as a dark-matter probe. <a href="https://www.nature.com/articles/nature25791" rel="nofollow">Read more...</a></p></div> </div> </div> </div> </div> <h2> <div class="paragraph paragraph--type--ucb-related-articles-block paragraph--view-mode--default"> <div>Off</div> </div> </h2> <div>Traditional</div> <div>0</div> <div>On</div> <div>White</div> Thu, 01 Mar 2018 15:41:21 +0000 Anonymous 554 at /ness