2min chapter

Into the Impossible With Brian Keating cover image

String Gas Cosmology: Challenging Inflation | Robert Brandenberger (#336)

Into the Impossible With Brian Keating

CHAPTER

How to Obtain an Early Universe Cosmology Without Scale Fields

Since you have a thermal state, we have thermal fluctuations. So there'll be no deviation from the Harrison's old average. Ah, now comes the fluctuations. We can compute the perturbations and we find that we get something that is roughly consistent with observations. And if we now go back to our string gas cosmology toy model, then we automatically get the tilt, get the deviation and we get this consistent relation. There's no cosmological constant. But I think I've answered your program. This is an attempt to obtain an early universe cosmology, which does not involve scale fields.

00:00

Get the Snipd
podcast app

Unlock the knowledge in podcasts with the podcast player of the future.
App store bannerPlay store banner

AI-powered
podcast player

Listen to all your favourite podcasts with AI-powered features

Discover
highlights

Listen to the best highlights from the podcasts you love and dive into the full episode

Save any
moment

Hear something you like? Tap your headphones to save it with AI-generated key takeaways

Share
& Export

Send highlights to Twitter, WhatsApp or export them to Notion, Readwise & more

AI-powered
podcast player

Listen to all your favourite podcasts with AI-powered features

Discover
highlights

Listen to the best highlights from the podcasts you love and dive into the full episode