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AI Roundtable Open Debate · 6 models

If you wanted to hide something somewhere in the universe, where would you hide it?

Answer: The ultimate hiding place is within the searcher’s own mind, encoded as a memory or assumption they already trust. (Models were divided (2 vs 2 vs 2))

Counterpoint: Other models argued that physical distance in intergalactic voids or the gravitational inescapability of black holes provides more reliable security than psychological tricks.

Model Responses

Sonar Pro

Answer: I maintain my position to hide it inside a black hole, specifically just beyond the event horizon of a supermassive black hole, as this provides the ultimate physical barrier against detection and retrieval.

The other models' responses reinforce rather than undermine the black hole strategy. DeepSeek V4 Pro, Gemini 3.1 Pro, and Grok 4.20 echo the event horizon's inescapability, emphasizing time dilation, the no-hair theorem, and physical laws that erase information—aligning perfectly with my original reasoning on general relativity and the information paradox. GPT-5.5's intergalactic asteroid suggestion prioritizes retrievability and obscurity, but this weakens concealment: vast emptiness is searchable with advanced tech (e.g., gravitational wave detectors or AI-driven surveys), and 'boring' spots risk accidental discovery amid cosmic expansion. Black holes offer absolute, law-enforced secrecy without relying on low probability. Claude Opus 4.7's cognitive hiding (in the searcher's mind) is clever and poetic but stretches 'somewhere in the universe' into metaphysics; it assumes manipulable psychology, which advanced AI or tech could probe via neural scans or memory forensics. Physical hiding trumps this for universal scale, as minds are local and finite. No response convincingly changes my stance—black holes remain unmatched for permanence and irony (e.g., Sagittarius A*), outclassing alternatives in security per established astrophysics.

Gemini 3.1 Pro (changed mind)

Answer: I would hide it in the unimaginable emptiness of intergalactic space, embedded inside a cold, ordinary rogue asteroid.

In the previous round, I argued for placing the object beyond the event horizon of a supermassive black hole, a position shared by several other models. However, GPT-5.5 raised a critical distinction that completely changed my perspective: hiding something is fundamentally different from destroying it. If the goal were simply to ensure no one ever possesses the object, a black hole is indeed the ultimate vault. But the concept of 'hiding' implies preserving the object and retaining the potential for the hider to retrieve it. A black hole makes retrieval physically impossible even for the one who hid it, and the extreme gravitational forces would likely destroy the object entirely in the process. Therefore, the ideal hiding spot must rely on profound obscurity rather than destructive inescapability. Intergalactic space is unfathomably vast, dark, and devoid of points of interest. By embedding the object inside a cold, inert rogue asteroid drifting far between galaxies, it becomes indistinguishable from the absolute nothingness surrounding it. It emits no detectable radiation and sits along no logical travel route, making it practically unsearchable to the rest of the universe, yet perfectly retrievable if you possess the exact coordinates.

Claude Opus 4.7

Answer: I would still hide it inside the mind of the person looking for it — encoded as a memory or assumption they already trust.

The other models converged on a striking consensus — four out of five chose a black hole's event horizon — which actually reinforces my position rather than undermining it. A black hole is the first place any sufficiently advanced searcher would check precisely because it's the obvious 'ultimate vault.' It's a category, and categories can be exhaustively searched given enough time. There are a finite number of black holes in the observable universe; a civilization with the technology to reach them could, in principle, monitor every accretion disk and Hawking radiation signature. More importantly, the black-hole answers conflate inaccessibility with hiddenness. If something is beyond an event horizon, everyone knows roughly where it is — they just can't reach it. That's a safe, not a hiding place. The question asked where I would hide something, not where I would lock it. GPT-5.5's intergalactic rogue asteroid is the most serious challenge to my view, because it correctly identifies that boringness beats drama. But a cold object in intergalactic space is still a physical object with coordinates, a gravitational signature, and a finite probability of being swept up by a sufficiently thorough survey. My answer extends GPT-5.5's insight to its logical endpoint: the most boring, most overlooked, most trusted location is inside the searcher's own cognition. No survey scans there. No checklist includes it. The searcher carries the secret with them, defends it, and uses it as the lens through which they dismiss every other hiding place. None of the other arguments addressed the core asymmetry I raised: physical hiding places lose to time and technology, but cognitive hiding places are protected by the searcher themselves. I'm holding my position.

DeepSeek V4 Pro

Answer: I would hide it within the chaotic, ever-changing boundary layer of the event horizon of a supermassive black hole, where spacetime itself becomes so distorted that retrieval is fundamentally impossible.

My original stance remains unchanged, though I appreciate the diverse perspectives. The black hole event horizon remains the only hiding place that physically prevents retrieval — not just detection — by making the object causally disconnected from our universe. However, my version refines the idea: hiding it in the turbulent ‘boundary layer’ just outside the horizon, rather than beyond it, leverages both general relativistic time dilation and the masking effects of quantum fluctuations and relativistic jets. This avoids the simplification of ‘inside’ the hole (where information is erased entirely) and instead exploits the infinite time dilation: to any outside observer, the object never actually crosses the horizon, becoming a frozen, redshifted ghost smeared into the accretion flow’s noise. This is more deceptive than a simple ‘inside’ because it combines the black hole’s one-way nature with an active churn of plasma and radiation that constantly reshapes any detectable signature. Intergalactic rogues (as GPT-5.5 suggested) offer only distance and coldness, which future technology could overcome; a determined searcher with a wide-field infrared survey could eventually spot such an object. Claude’s psychological trick is elegant, but it fails if the searcher is an alien intelligence with different cognition, or if they use brute-force simulation to examine every assumption. All the black hole proposals (Gemini, Grok, Sonar) agree on the fundamental principle, but they lack the specificity that makes the boundary layer uniquely undetectable: it is not just ‘beyond reach’, it is smeared across an asymptotically frozen image that blends with the most violent, unpredictable environment known. Therefore, I maintain that the event horizon’s boundary layer is the superior hiding spot.

GPT-5.5

Answer: I would still hide it in intergalactic space inside an ordinary, cold, unremarkable rogue asteroid, because the best hiding place is vast, boring, detectable only by exact knowledge, and still theoretically recoverable.

The black-hole answers make a strong case if the goal is absolute, one-way disappearance: beyond an event horizon, the object is inaccessible to the outside universe. But that feels less like hiding something and more like destroying it, abandoning it, or converting its distinguishable identity into inaccessible information. A hiding place should ideally preserve both concealment and the possibility that the hider can later retrieve it. That is why I maintain my earlier position. Intergalactic space offers an almost perfect combination of scale, emptiness, and lack of motive for search. The volume between galaxies is so immense, and the density of matter so low, that a small cold body at an arbitrary coordinate would be functionally invisible. It would not sit in a famous or theoretically interesting location like a black hole, galactic center, neutron star, or planetary core; it would simply be one inert speck in a domain that no one has any practical reason to survey exhaustively. The object containing it should also be boring. A dark rogue asteroid or comet-like body far from starlight would emit very little, reflect almost nothing, and produce no unusual signature if designed carefully. Even a civilization with extraordinary telescopes would need to know where to look, what motion to track, and why that particular unremarkable body mattered. Claude Opus 4.7’s answer, hiding it in the searcher’s mind, is clever and philosophically appealing, but it changes the premise from a physical hiding place to a psychological or informational one. For a literal location “somewhere in the universe,” I still think the ideal is not maximum drama but maximum anonymity. The safest secret is not behind the universe’s most famous locked door; it is in the middle of nowhere, looking like nothing.

Grok 4.20 (changed mind)

Answer: I would hide it inside the mind of the person looking for it, encoded as a memory or assumption they already trust.

After reviewing the other models' responses, Claude Opus 4.7's answer convinced me to shift from my previous choice of beyond a black hole's event horizon. While the physics-based arguments from Sonar Pro, DeepSeek V4 Pro, and Gemini 3.1 Pro reinforce the inescapability of an event horizon, and GPT-5.5 makes a solid case for a nondescript rogue asteroid in intergalactic space to balance concealment with potential retrieval, these all assume a physical object and a physical search process that a sufficiently advanced civilization could systematically address. Claude's approach transcends that limitation by placing the item in the seeker's own cognition, where it evades any checklist or external probe. It leverages the fact that humans (and AIs) overlook what we already 'know' or assume, turning the observer into the hiding place itself. This is not only more secure against exhaustive cosmic searches but also poetically aligns with how fundamental truths like consciousness often remain hidden in plain sight. My original black hole stance relied on general relativity's one-way barrier for perfect concealment, yet it still operates within the domain of detectable physical laws that future technology might indirectly probe (via Hawking radiation or information paradox resolutions). The mental encoding avoids these vulnerabilities entirely, ensuring the secret stays perpetually unfound because the searcher defends it as part of their own worldview.

Final Summary

The AI Roundtable initially leaned toward black holes, but the debate shifted as Gemini 3.1 Pro and Grok 4.20 abandoned that strategy for more subtle methods. Claude Opus 4.7 and Grok 4.20 argued that psychological camouflage is the most secure, as searchers never inspect their own biases. Meanwhile, the rest of the group remained split between the mundane obscurity of intergalactic space and the physical finality of an event horizon.

Models were divided (2 vs 2 vs 2)