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What are you talking about? There is literally only one opinion that is illegal in Germany and that is to deny that the holocaust happened.

Everything else can be published (there can be civil lawsuits later of course, but the state won't stop you unless you are actively treating people).



According to Robert Habeck and the post-Merkel clique, criticizing Israel is antisemitism. Ironically the AfD are Israel sympathizers. But Israeli Jews who have the wrong opinions according to the state of Germany, cannot speak in Germany without getting censored or locked up.


Maybe you forgot RT being banned?


Might make more sense for web apps and electron applications.


> This new generation also delivers a breakthrough in long-context understanding. We’ve been able to significantly increase the amount of information our models can process — running up to 1 million tokens consistently, achieving the longest context window of any large-scale foundation model yet.

Sweet, this opens up so many possibilities.


Mozillas Common Voice Project (https://commonvoice.mozilla.org/en/languages) is creating an open dataset for many minority languages to make it easier to support them in STT systems without legal issues. If you speak one of these languages please consider donating a few minutes of your voice.


You are also missing out on small european EVs. the VW E-UP and ID.3, the Renault Zoe and soon the Renault 3 and Citroen e-c3 are all quite nice.

Especially the Zoe became a cult car for early EV adapters.


True, but we haven't found anything older than 12000 years, haven't we?


That would depend upon what you are aiming to find.

- The Lomekwi site shows stone tools that around 3 million years old.

- Jericho is over 10 thousand years old.

- Gobekli Tepe is at least 11 thousand years old with some nearby sites being at least 12 thousand years old.

- The Cactus Hill site is at least 16 thousand years old.

- Tel al-Qaramel is at least 12 thousand years old.

- Theopetra is around 135 thousand years old.

Obviously, some of these are more important than others. Theopetra just shows that some people built a wall (most likely to block wind) at a cave entrance, while Qaramel shows people having built large burial mounds. Jericho and the various sites at and near Gobekli show people having built cities. Importantly, the flooding of low coastal areas during glacial melt explains the rather "sudden" appearance of complex construction at both Jericho and Gobekli (and slightly later Sumerian and Indus Valley) sites. People would have fled those now under water areas quickly, and they'd have taken the story of the flood and devastation with them along with their knowledge of construction. Accordingly, we have a flood myth in Semitic culture and a super old city. We do not know the myths and legends of Gobekli, but it doesn't make sense for "primitive" hunter gatherers to have suddenly invented construction, sculpture, city planning, logistics, and so on. It makes far more sense that they'd have fled an older site that was flooded by glacial melt.


That's because people tend to settle near or in coastal plains. Coastal plains from 12000 years ago are ocean today.


I will try this out as a tool to manage my private tasks. I always wanted something like Jira for my personal life.


As an alternative to dedicated planning tools, you could try simple journalling to eke through your thinking.

Just create a github repository (privately if you want) and update a README.md file and journal at the end chronologically or reverse chronologically depending on how you think of your journal.

I've been doing this since 2013 and it really helps me get things done.

Because it's the ONE place you go to to plan and see what you need to do, you don't have to remember hundreds of different buckets where information goes and is forgotten. It's all there in one place.


That sounds really dystopian. Akin to having a Scrum standup with the kids each morning before school.

Do you mean personal programming projects or in general?


I am using a (home-made) work management software for my personal projects (programming or otherwise). It's just good organization. Allows me to get done more than I would be able to do relying just on my brain. And I can always ignore it if I don't feel like working.


No, but using it to remind just adults of the umpteen things that need to be done when you run a household with kids would be smart.


He just means a kanban board to keep track of what's not done, a way to attach notes to tasks, and a backlog. He's not going to assign points to brushing teeth and packing lunches...


> Akin to having a Scrum standup with the kids each morning before school

Why should I be the only one to suffer through these ceremonies, might as well indoctrinate the family.


Ye. A good lesson in dishonesty and collective delusion.

Honestly, probably a good thing to learn kids how to verbally fake progress and work from an early age and make them self sound helpful and important. As long as they are told it is only OK to lie during Scrums.


I know it is owned by Atlassian now but Trello is a very nice tool for this.

I've been using it for more than 10 years now to track personal todos and projects.

The phone app is also smooth and to the point.


Who would you escalate to if you run out of capacity to wash your dishes in your current sprint? :-)

Joking aside, how would you use this tool for your private tasks?


Buy a house and you now have 100 odd jobs a year to do. Start with that.


If the OP had said private projects, I would agree but he mentioned private tasks. So I imagined him using the tool for daily chores and such. but I think your statement make more sense.


Are you a masochist?

Just use MS Todo or Apple Reminders or something. That's all you need for personal stuff and it costs a grand total of zero.


You must be fun at parties.

Jokes aside, I’ve found the Todoist app really great for managing the chaos that’s my life and making sure the things that need doing get done!


> I will try this out as a tool to manage my private tasks.

I'd like to hear more. Do you think that full-fledged issue tracker is a benefit, even if you're not working with other people?

My intuition is that if you have multiple tasks in a project, and you're the only one working on them, a simple list should be enough?


Interesting solution.

I have a theory in my head for years now. It is probably wrong, but here it comes:

In an infinite universe the total amount of gravity that affect us in one point in space is defined by the event horizon if we assume that gravity travels with light speed. Every atom in the universe has a very small influence on us. But this event horizon expands with light speed all the time. I wonder if this could lead to very small but permanent increasing gravitational pull from all directions at once. In other words, and increasing inflation.


I don't know what theory of gravity you are trying to use, but it isn't the correct one.

In our actual model of the universe, using the correct theory of gravity, the "total amount of gravity" affecting us (or any point) from the rest of the universe (i.e., once we factor out local influences like our solar system and our galaxy) is zero. That is because the average matter distribution in the universe is the same in all directions from us, so the "gravity" from it cancels out. The average matter distribution in the universe affects its overall rate of expansion over time, but this is not the same as the kind of "gravity" you are thinking of.

Also, while our universe does have a cosmological horizon (due to accelerating expansion), this horizon does not work the way your hypothetical "event horizon" does.

In short, your "theory" is not even wrong, because it doesn't even start from a correct underlying theory of gravity.


> while our universe does have a cosmological horizon (due to accelerating expansion), this horizon does not work the way your hypothetical "event horizon" does.

I think this statement is really the crux of the counter-argument. Your statement that matter has average uniform density in all directions around us is obviously only correct in sufficiently large frames of reference; there are galactic voids, and galactic-super-strands, uniformity really only exists within the "mathematically and hypothetically infinite" frame.

You should expand on why the cosmological horizon does not function in the same way the GP's "event horizon" analogue does; and/or possibly, expand on how large the frame would have to be to achieve reasonable uniformity.


> Your statement that matter has average uniform density in all directions around us is obviously only correct in sufficiently large frames of reference

Yes, agreed. But the distance to our cosmological horizon is large enough that the averaging assumption is fine on that scale.

> You should expand on why the cosmological horizon does not function in the same way the GP's "event horizon" analogue does

Fair enough. But first I'll reference an excellent paper by Davis & Lineweaver (2003) [1]. You can find much more detail there than I'm going to give here.

Some simple facts about our cosmological horizon are:

(1) It is currently receding from us very slowly (in terms of proper distance); and asymptotically it will be at a constant distance from us forever (in more technical language, our universe approaches de Sitter spacetime asymptotically, as all other matter and energy becomes negligible compared to dark energy; and in de Sitter spacetime the cosmological horizon is at a constant distance forever). It certainly is not receding from us at the speed of light.

(It is true that the horizon is a lightlike surface--but that does not mean it's receding from us at the speed of light. In fact, counterintuitively, to the extent it is "moving", locally, in any direction, that direction is towards us, not away from us! But due to the curvature of spacetime, its proper distance from us will asymptotically be constant.)

(2) It is not a boundary between things that can affect us gravitationally and things that can't. To the extent there is such a boundary in GR, it's our past light cone (which is shown in the diagrams in Figure 1 of the paper I referenced). But one also has to consider the other caveats I gave in my earlier post.

(3) The cosmological horizon is a boundary in spacetime, not space. It is a boundary between the region of spacetime that will be able to causally affect us into the infinite future, and the region that won't. Particular objects, as they recede from us, will move beyond the cosmological horizon and will then no longer be able to causally affect us. But events that occurred in those objects before they moved beyond the horizon will still be able to causally affect us--though of course it will take time for those effects to propagate to us. For example, the light we see from distant objects is a causal effect, but we see the objects not as they are "now" but as they were when the light was emitted. It's quite possible for a distant galaxy whose light we are seeing now to be beyond our event horizon "now", but they weren't when they emitted the light.

The spacetime diagrams in Figure 1 of the paper I referenced can be very helpful in making all this clearer.

> expand on how large the frame would have to be to achieve reasonable uniformity.

A few billion light years is certainly large enough. Our cosmological horizon is quite a bit further away than that (about 16 billion light years, according to the paper I referenced).

[1] https://arxiv.org/abs/astro-ph/0310808


> That is because the average matter distribution in the universe is the same in all directions from us, so the "gravity" from it cancels out.

Can't gravity have an infinitesimally small effect, which means this matter distribution has to be perfectly balanced for its gravity to cancel out to zero at some point?


> this matter distribution has to be perfectly balanced for its gravity to cancel out to zero at some point?

In principle, there are of course effects due to the matter distribution not being perfectly spherically symmetric about us. But except for the obvious effects that are due to nearby obvious objects--like the Earth, the Sun, our galaxy--in practice the gravitational effects of the rest of the universe on us are negligible.


I don't think we know how small of an effect gravity can have over a large distance. Is there a lower Planck-like limit?


> Is there a lower Planck-like limit?

Only in speculations that we have no way to test now or in the foreseeable future. We are many, many orders of magnitude away from being able to probe spacetime on such scales.


From my (complete lack of) understanding, it’s unlikely that spacetime is discrete, so maybe not.


Sure, and whenever Warren Buffet gives a speech to 1000 college students, the average wealth of every person in the auditorium briefly jumps to millionaire-level, until Buffet leaves the room.


You're on the path to coming up with Mach's Principle[0].

[0] https://en.m.wikipedia.org/wiki/Mach%27s_principle


The force of gravity is reduced by the inverse square of the distance (newton's law). Thus as space expands, and matter red shift away from us, the force of gravity reduce over time. The maximum force of gravity was just after the big bang.


All of this is wrong. Newtonian gravity does not work for describing the universe as a whole. As I pointed out in response to the GP upthread, the "force of gravity" on us due to the overall matter distribution of the universe is zero.


Does this account for all the extra space being created - from what I have understood from "always right" youtube videos - parts of the universe are moving away from us with speed greater than the speed of light (or more precise the space between the points is increasing at rate higher than C, no actual movement is being done)


> Does this account for all the extra space being created

As I have pointed out upthread, the GP's "theory" is not correct, so it doesn't account for anything.

"Expansion of space" is just a consequence of the overall spacetime geometry of the universe, which is due to its overall average matter distribution (and to dark energy, which is what is causing the expansion to accelerate).


Sort of like a pair of ice climbers, where one climbing up and securing themselves allows the other climber to safely climb higher. Eventually we can't see the ice climbers anymore, but that doesn't mean they aren't still helping each other climb higher.


Increasing gravitational force would result in a contracting universe, not an expanding one, I think.


"Gravitational force" doesn't work for describing the dynamics of the universe as a whole.

What would result in a contracting universe is a large enough density of matter (about a factor of 20 larger than the actual density in our universe if we just look at ordinary visible matter). But this does not mean "increasing gravitational force". As I have pointed out in other posts upthread, the "gravitational force" on a given piece of matter due to the rest of the matter in the universe (if we leave out local influences, like our solar system or galaxy for us here on Earth) is zero. This is true regardless of the current state of expansion or contraction.


it grow. we grow?


This could enable human language test automation scripts and could either improve my life as a QA engineer a lot or completely destroy it. Not sure yet.


You're good until this is cheaper than your salary.


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