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This post is an experiment in two ways that I explain in comments here and here. But you don't need to read those comments before reading this post.
1. Introduction
In What We Owe the Future I argued that even very severe non-extinction catastrophes are unlikely to permanently derail civilisation. Even if a catastrophe killed 99.9% of people (leaving 8 million survivors), I'd put the chance we eventually re-attain today's technological level at well over 95%.
On the usual longtermist picture, this means such catastrophes are extraordinarily bad for present people but don't rival full existential catastrophes in long-run importance. Either we go extinct (or lock into a permanently terrible trajectory), or we navigate the "time of perils" once and reach existential security.
In this article I'll describe a mechanism by which non-extinction global catastrophes would have existential-level importance. I'll define:
The mechanism is straightforward: if a catastrophic setback occurs [...]
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Outline:
(00:19) 1. Introduction
(02:59) 2. A Simple Model of Sisyphus Risk
(03:03) 2.1. One catastrophic setback
(04:40) 2.2. Ords numbers
(06:36) 3. What Forms Could Post-AGI Catastrophic Setbacks Take?
(06:47) 3.1. Engineered pandemics
(07:48) 3.2. Nuclear war and nuclear winter
(08:31) 3.3. AI-driven catastrophe
(09:01) 3.4. Butlerian backlash and fertility decline
(10:22) 4. Would a Post-Setback Society Retain Alignment Knowledge?
(11:08) 4.1. Digital fragility
(12:44) 4.2. Hardware and software compatibility
(13:43) 4.3. Tacit knowledge
(14:40) 5. Wont AGI make post-AGI catastrophes essentially irrelevant?
(16:02) 6. Implications and Strategic Upshots
(16:07) 6.1. The importance of non-AI risks, especially non-AI non-bio
(17:06) 6.2. When to donate
(18:05) 6.3. A modest argument for more unipolar futures
(19:25) 6.4. The value of knowledge preservation and civilisational kernels
(20:25) 7. Conclusion
(21:38) Appendix: Extensions
(21:43) A.1 Multiple cycles
(29:26) A.2 Higher or lower risk in the rerun
(31:14) A.3 Trajectory change
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First published:
Source:
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Narrated by TYPE III AUDIO.
By EA Forum TeamThis post is an experiment in two ways that I explain in comments here and here. But you don't need to read those comments before reading this post.
1. Introduction
In What We Owe the Future I argued that even very severe non-extinction catastrophes are unlikely to permanently derail civilisation. Even if a catastrophe killed 99.9% of people (leaving 8 million survivors), I'd put the chance we eventually re-attain today's technological level at well over 95%.
On the usual longtermist picture, this means such catastrophes are extraordinarily bad for present people but don't rival full existential catastrophes in long-run importance. Either we go extinct (or lock into a permanently terrible trajectory), or we navigate the "time of perils" once and reach existential security.
In this article I'll describe a mechanism by which non-extinction global catastrophes would have existential-level importance. I'll define:
The mechanism is straightforward: if a catastrophic setback occurs [...]
---
Outline:
(00:19) 1. Introduction
(02:59) 2. A Simple Model of Sisyphus Risk
(03:03) 2.1. One catastrophic setback
(04:40) 2.2. Ords numbers
(06:36) 3. What Forms Could Post-AGI Catastrophic Setbacks Take?
(06:47) 3.1. Engineered pandemics
(07:48) 3.2. Nuclear war and nuclear winter
(08:31) 3.3. AI-driven catastrophe
(09:01) 3.4. Butlerian backlash and fertility decline
(10:22) 4. Would a Post-Setback Society Retain Alignment Knowledge?
(11:08) 4.1. Digital fragility
(12:44) 4.2. Hardware and software compatibility
(13:43) 4.3. Tacit knowledge
(14:40) 5. Wont AGI make post-AGI catastrophes essentially irrelevant?
(16:02) 6. Implications and Strategic Upshots
(16:07) 6.1. The importance of non-AI risks, especially non-AI non-bio
(17:06) 6.2. When to donate
(18:05) 6.3. A modest argument for more unipolar futures
(19:25) 6.4. The value of knowledge preservation and civilisational kernels
(20:25) 7. Conclusion
(21:38) Appendix: Extensions
(21:43) A.1 Multiple cycles
(29:26) A.2 Higher or lower risk in the rerun
(31:14) A.3 Trajectory change
---
First published:
Source:
---
Narrated by TYPE III AUDIO.