BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//sebbo.net//ical-generator//EN
NAME:Berkeley Public Library
X-WR-CALNAME:Berkeley Public Library
BEGIN:VEVENT
UID:122a9e0f-1cd6-4d81-875f-1b987644c76a
SEQUENCE:0
DTSTAMP:20260821T235410Z
DTSTART;TZID=America/Los_Angeles:20260915T173000
DTEND;TZID=America/Los_Angeles:20260915T190000
SUMMARY:Popping the Science Bubble @Central
LOCATION:Central Library\nCentral Library
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Central Library;X-APPLE-RA
 DIUS=10;X-TITLE=Central Library:geo:37.8681967,-122.2684903
GEO:37.8681967;-122.2684903
DESCRIPTION:A UC Berkeley seminar series.\nhttps://berkeleypubliclibrary.l
 ibnet.info/event/17261973
X-ALT-DESC;FMTTYPE=text/html:<p>Learn about cutting-edge research happenin
 g at UC Berkeley\, directly from the scientists themselves. Join Popping t
 he Science Bubble on Tuesday\, September 15th at 5:30 pm at the Central Li
 brary in the second floor Mystery Room or join us virtually on Zoom: http:
 //bit.ly/PtSBBerkeley (register at the link).</p>\n<p>This month's present
 ations will be:</p>\n<p><strong>Searching for Dark Matter: Axions!</strong
 > &mdash\; Shreya Puranam\, <em>Physics</em></p>\n<p>Only 15% of the matte
 r in the universe is the matter that makes us up (baryonic matter). We ref
 er to the other 85% as dark matter. While we have known about the existenc
 e of dark matter through observations of galaxy motion since the mid 1900'
 s\, we have yet to directly detect and determine what makes it up. One com
 pelling candidate that I search for is a particle called the axion. During
  this talk\, I will show why we know dark matter must exist\, why the axio
 n is a good candidate\, and how we actually search for it.</p>\n<p><strong
 >Where Did All the Antimatter Go?</strong> &mdash\; Charlie Hultquist\, <e
 m>Physics</em></p>\n<p>We're used to regular matter -- a positively charge
 d nucleus surrounded by negatively charged electrons. Antimatter is the re
 verse -- a negative nucleus surrounded by positive electrons (positrons). 
 We believe that just after the Big Bang\, equal amounts of matter and anti
 matter were present in the universe. In contrast\, today's universe is fil
 led with an abundance of matter. To understand where all this antimatter w
 ent\, we use particle accelerators to recreate conditions in the early uni
 verse and look for matter-antimatter asymmetric processes.</p>\n<p>Learn m
 ore at the <a href="https://poppingthesciencebubble.wordpress.com/">Scienc
 e Bubble website</a>.</p>\n<p>Watch past talks on <a href="https://www.you
 tube.com/@PtSBBerkeley/videos">YouTube</a>.</p>\nhttps://berkeleypubliclib
 rary.libnet.info/event/17261973
URL;VALUE=URI:https://berkeleypubliclibrary.libnet.info/event/17261973
ATTACH:https://static.libnet.info/images/events/berkeleypubliclibrary/Sept
 ember_Science_Bubble_for_Communico.png
END:VEVENT
END:VCALENDAR