rah

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[–] rah@hilariouschaos.com 2 points 1 week ago (1 children)

On reflection, I realised my flippant joke may not have been well received. I apologise. I've deleted the comment.

[–] rah@hilariouschaos.com 2 points 1 week ago

British police aren't right wing.

LOL

[–] rah@hilariouschaos.com 1 points 1 week ago

poor, defenseless, innocent women

Not doing yourself any favours with this kind of sarcastic comment.

Anyone who advocates for the disenfranchisement of trans people

I've never seen anybody argue that trans people should be denied the right to vote. Including in this article.

[–] rah@hilariouschaos.com 1 points 1 week ago

Yup

What's the name of the package? I couldn't find anything.

[–] rah@hilariouschaos.com 2 points 2 weeks ago (1 children)

You are saying that Christianity actively opposes the virtues of Christianity, right.

No. You're saying that followers of Christianity do not display Christian virtues. I'm saying therefore Christianity is having a negative impact on the spread of Christian virtues and so if your goal is to promote Christian virtues then promoting Christianity is working against your goals.

[–] rah@hilariouschaos.com -4 points 2 weeks ago* (last edited 2 weeks ago)

Did you read it?

Yes. Did you?

She doesn’t think Trans people, a part of the LGBT community, exist.

The article makes no mention of whether she views trans people as existing. Again, you're jumping to conclusions. And to be frank, you're being ridiculous.

[–] rah@hilariouschaos.com 1 points 2 weeks ago (2 children)

Is there a client for Signal in Debian?

[–] rah@hilariouschaos.com 2 points 2 weeks ago

Paper abstract:

We propose a novel scenario in which scalar perturbations, which seed the large-scale structure of the universe, are generated without relying on a scalar field (the inflaton). In this framework, inflation is driven by a de Sitter space time, where tensor metric fluctuations (i.e., gravitational waves) naturally arise from quantum vacuum oscillations, and scalar fluctuations are generated via second-order tensor effects. We compute the power spectrum of such scalar fluctuations and show it to be consistent with near scale invariance. We derive the necessary conditions under which scalar perturbations become significant and much larger than the tensor modes, and we identify a natural mechanism to end inflation via a transition to a radiation-dominated phase. Our proposed mechanism could remove the need for a model-dependent scenario: the choice of a scalar field, as the inflaton, to drive inflation.

https://dx.doi.org/10.1103/vfny-pgc2

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