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cosmic microwave background

cosmic microwave background

Search complete. 135 mentions across 25 episodes found for "cosmic microwave background".

Oct 29, 2026

Matt O'DowdHOST
0:59
This episode is supported by 23andMe.
Matt O'DowdHOST
1:02
If you study a map of the Cosmic Microwave Background, or CMB, you may notice a large deep blue splotch on the lower right.
Matt O'DowdHOST
1:10
This is the cold spot.
Matt O'DowdHOST
1:13
Is this feature a statistical fluke, the signature of vast supervoids, or even the imprint of another universe? Is that giant cold spot in the cosmic microwave background really evidence of a collision with another universe? That's what all the media hype is saying, which means it's time for another space time journal club to sort it out.
Matt O'DowdHOST
1:42
Today we're going to talk about a fascinating new publication by Mackenzie et al.
Matt O'DowdHOST
1:46
2017 titled Evidence Against a Super Void Causing the CMB Cold Spot.
Matt O'DowdHOST
1:53
First, the name.
Matt O'DowdHOST
1:55
Evidence against a supervoid.
Matt O'DowdHOST
16:05
In the last episode, we did a Space Time Journal Club on a new paper investigating whether the cold spot in the cosmic microwave background was due to supervoids or a collision with another universe.
Matt O'DowdHOST
16:18
Let's discuss.
Matt O'DowdHOST
16:20
A few people point out that there are lots of cold spots in the CMB map and that some look larger than the actual cold spot.
Matt O'DowdHOST
16:28
Well, first, let me point out that the cold spot wasn't identified by the, ooh, that bit looks a bit bluer than the rest method.
Matt O'DowdHOST
16:36
Detailed statistical analysis of the entire Planck CMB map pointed to that region as being a significant outlier.
Matt O'DowdHOST
16:44
It's the size of the consistently low temperature region that's unusual.
Matt O'DowdHOST
16:49
There are smaller, cooler regions that are consistent with random fluctuations.
PeterHOST
32:53
It was an event so big that we can detect the echo of all this energy all around us even 14 billion years later.
PeterHOST
33:04
It's called the Cosmic Microwave Background, the CMB.
PeterHOST
33:08
But it's not actually a leftover of the Big Bang.
PeterHOST
33:13
The CMB is the imprint of an event 380,000 years after the Big Bang.

27 MINS LATER

PeterHOST
60:14
It would have nowhere to go.
PeterHOST
60:17
Temperatures would rise as the pressure increased.
PeterHOST
60:21
Same cosmic microwave background energy, but a much smaller box.
PeterHOST
60:26
The heat would go up.
Cool Worlds

Cool Worlds

A MILLION MPH

Oct 29 · 11 Mentions

David KippingHOST
21:10
After all, when you walk down the carriage of a 50mph train, are you moving at 3mph or 53mph? Both are right, it just depends what you're comparing to.
David KippingHOST
21:22
But one example might at first seem to defy this, the Cosmic Microwave Background or the CMB.
David KippingHOST
21:30
This is the radiation that was produced by the hot primordial soup of the early universe just 380,000 years after the big bang.
David KippingHOST
21:40
That time corresponds to the epoch when the universe became transparent to light for the first time.
David KippingHOST
21:45
Because before that it was largely ionized, creating a kind of thick fog that prevented light from traversing space.
David KippingHOST
21:52
The CMB radiation is all around us.
David KippingHOST
21:55
We are bathed in its light.
David KippingHOST
21:58
It comes from every direction.
David KippingHOST
15:31
After all, the entire universe was filled with this ionized plasma.
David KippingHOST
15:35
This light is known as the Cosmic Microwave Background or CMB and it encodes the temperature of the universe at this time.
David KippingHOST
15:43
Any patch of the CMB more than two degrees away from another patch is simply too far away to have had time for light to have traveled between them, at least given the age of the universe at the time, just 380,000 years old.
David KippingHOST
15:58
So if we see a particular pattern or ripple repeated in the CMB that is separated by more than two degrees, well, that implies that space somehow wraps around on itself.
Michelle CollinsHOST
13:17
And so you normally, by assuming this sort of, we assume in this, you have a flat lambda cold dark matter model, and then you get a value for H naught for that model.
Michelle CollinsHOST
13:24
If you were to change the model, you would get a slightly different value of H naught, but the CMB supports this sort of flat lambda CDM cosmology.
Michelle CollinsHOST
13:30
So they use that.
Michelle CollinsHOST
13:31
Now the problem is that these two values are now measured very precisely, but they don't agree at a fairly high significance level.

8 MINS LATER

Payel DasHOST
21:31
actually it'd be nice to really see, could we ever constrain a kind of shape for it?
Michelle CollinsHOST
21:35
But this is, I guess, a way of checking the systematics on that local universe.
Michelle CollinsHOST
21:38
So, you know, then we have to say, okay, well, there's a reason that the CMB is not the same as the local universe.
Michelle CollinsHOST
21:43
And it isn't because the local universe measurement is wrong.
Dave FarinaHOST
33:45
More data has to be gathered.
Dave FarinaHOST
33:47
And once the CMB was understood, it was pretty resound like, like, yeah, okay, this looks to be this very, very, um, very, very precisely matches the expectation out of this, uh, out of this, uh, big bang cosmological model.
Dave FarinaHOST
34:04
We would expect to see, uh, this, this, uh, this artifact and it would be stretched to precisely this, uh, this temperature.
Dave FarinaHOST
34:11
So, uh, and the, the, uh, the, the, the, uh, the, and it's a tropic, uh, uh, aspect of it too.
Dave FarinaHOST
35:39
So they need this story.
Dave FarinaHOST
35:40
And they need the story so bad... that they try to tell the story from within the history of science, but they're lying every time when they do that.
Dave FarinaHOST
35:48
Once they got to CMB, okay, Big Bang cosmology is very, very clear.
Dave FarinaHOST
35:52
And again, none of it substantiates any of their propaganda.
Dave FarinaHOST
7:47
This can help us learn about the structure and composition of the universe.
Dave FarinaHOST
7:50
There is also a cosmic neutrino background, analogous to the cosmic microwave background, which would give us information about a much earlier universe than the CMB.
Dave FarinaHOST
8:00
An experiment called Ptolemy is building a demonstrator to prove that an experiment could look for this.
Dave FarinaHOST
8:06
It is extremely hard to detect, but would revolutionize cosmology in the same way that the CMB did.
Dave FarinaHOST
8:12
There are also theories about sterile neutrinos, which are hypothetical neutrinos that don't feel the weak force, yet they mix with the three active flavors and add extra oscillation frequencies.
Dave FarinaHOST
8:23
Certain anomalies have been spotted in reactor and accelerator experiments that possibly point towards extra sterile neutrino flavors, as well as some theoretical motivations that let them act as dark matter or CP-violating components of the early universe.

Unknown podcast

What Happened at Big Bang?

Oct 25 · 2 Mentions

speaker_0NARRATOR
20:43
This moment known as decoupling is a defining milestone releasing an immense flood of radiation that will travel across the cosmos for eternity.
speaker_0NARRATOR
20:51
These photons, unimpeded at last, form what we now observe as the Cosmic Microwave Background, or CMB, the universe's oldest light, a fossilized afterglow from 380,000 years after the Big Bang.
speaker_0NARRATOR
21:06
The CMB is our cosmic blueprint, an invaluable relic that carries the secrets of the early universe, revealing subtle temperature variations that would one day shape galaxies, stars, and clusters.
speaker_0NARRATOR
21:19
It stands as a testament to the universe's origins, helping scientists decode its age, composition, and even its fate.
speaker_0NARRATOR
21:31
By now, at around 380,000 years old, the universe has become transparent but not yet illuminated.
PBS Space Time

PBS Space Time

Dark Flow

Oct 24 · 14 Mentions

Top 5%
Matt O'DowdHOST
2:30
And yet, there is one frame of reference that in some ways is a little more preferred, or at least special, than all of the others.
Matt O'DowdHOST
2:39
It's the frame of reference of the cosmic microwave background radiation, the CMB.
Matt O'DowdHOST
2:44
The CMB is the leftover heat glow from the hot, dense early universe.
Matt O'DowdHOST
2:49
In all directions, it appears to be the same temperature, around 2.7 Kelvin, and hence, the same microwave wavelength.
Matt O'DowdHOST
2:57
Actually, when we look at the CMB from our moving platform of planet Earth, we don't see a perfectly even temperature.
Matt O'DowdHOST
3:05
This motion is due to the sun's orbit around the Milky Way and the Milky Way falling to the great attractor.
Matt O'DowdHOST
3:11
More on that last one soon.
Matt O'DowdHOST
3:13
That motion causes the CMB to be Doppler shifted.

15 more episodes mention cosmic microwave background.

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