{"arxiv_id":"hep-th/0302219","incoming":{"papers":306,"sentences":353,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"0705.2562","title":"Anthropic prediction in a large toy landscape","url":"/paper/0705.2562","section":"Bubble abundances by perturbation theory","sentence":"In the numerical example of Ref. [ref] $N∼10^7$, while for a realistic string theory landscape we expect $N ∼10^500$ [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"1111.6646","title":"Multi-field inflation with random potentials: field dimension, feature scale and non-Gaussianity","url":"/paper/1111.6646","section":"Trajectory dynamics","sentence":"Using the (perhaps somewhat arbitrary) values of Ref. [ref] , we place an anthropic lower bound on the number of e-folds at 59.5 coming from structure formation and an observational lower bound at $N = 62$ on the curvature from tunnelling.","intent_p":0.91,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1712.09693","title":"Dark energy, $\\alpha$-attractors, and large-scale structure surveys","url":"/paper/1712.09693","section":"Introduction","sentence":"However, unlike the earlier proposed mechanisms [ref] and the string theory landscape scenario [ref] , the quintessence-related mechanism of Ref. [ref] requires fine-tuning of the parameter $|V' |= |γ| ≲10^-120$, in addition to the standard anthropic constraint $|V(ϕ)| ≲10^-120$.","intent_p":0.84,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1810.02095","title":"The swampland conjecture and the Higgs expectation value","url":"/paper/1810.02095","section":"Wilsonian approach","sentence":"These assumptions are justified by the anthropic principle, since otherwise, the vacuum is no more habitable [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":174,"sentences":178,"quotes":[{"arxiv_id":"0711.1656","title":"The Arrow Of Time In The Landscape","url":"/paper/0711.1656","section":"?","sentence":"As is well known —$$ some would say “notorious\" —$$ string theory admits a “very large\" number of internally consistent basic models of the Universe: this is the string Landscape [ref] [ref] [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"2307.08067","title":"Top squarks from the landscape at high luminosity LHC","url":"/paper/2307.08067","section":"Introduction","sentence":"A third effect arises from the string landscape picture [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"0705.4141","title":"Initial Conditions for Bubble Universes","url":"/paper/0705.4141","section":"Section","sentence":"In string theory, the leading approach to the problem of the cosmological constant is given by the Landscape [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"2405.08789","title":"Computing Fundamental Constants in the FLRW Universe using the Hawking Radiation of the Cosmological Horizon","url":"/paper/2405.08789","section":"Introduction","sentence":"It is also possible thanks to the study of the holographic principle and the $AdS/CFT$ correspondence that has been formulated by several authors: [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] and [ref] among others.","intent_p":0.98,"contests_p":null},{"arxiv_id":"1808.09440","title":"The landscape, the swampland and the era of precision cosmology","url":"/paper/1808.09440","section":"Discussion and conclusions","sentence":"The situation changed with the invention of the KKLT scenario [ref] and its various generalizations, such as KL [ref] and LVS [ref] , which suggested a multitude of possibilities to describe the present value of the cosmological constant in the context of the string theory landscape [ref] .","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":171},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[{"relation":"contradicts","label":"States a conflicting result","papers":[{"arxiv_id":"astro-ph/0001197","url":"/paper/astro-ph/0001197","title":"The Beginning of the End of the Anthropic Principle","main_claim":"We argue that if string theory as an approach to the fundamental laws of physics is correct, then there is almost no room for anthropic arguments in cosmology.","p":0.85}]}],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":{"arxiv_id":"hep-th/0302219","kind":"model","paper_version":1,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T11:09:03+00:00","loaded_at":"2026-10-28T01:01:53.627383+00:00","evidence":"some","account":[],"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"entries":[{"p":0.91,"quote":null,"citing":[{"self":false,"year":2011,"title":"Multi-field inflation with random potentials: field dimension, feature scale and non-Gaussianity","arxiv_id":"1111.6646"}],"verified":true,"paraphrase":"Used the perhaps somewhat arbitrary values of this paper to place an anthropic lower bound of 59.5 e-folds from structure formation and an observational lower bound of 62 on the curvature from tunnelling."}],"papers_all":2,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"data_used":2,"comparison":1,"supports_this_paper":1},"dropped":{"relied_on":0,"unknown_ids":0,"account_lines":0,"contest_vetoed":0,"below_threshold":0,"contest_drawback":0,"contest_without_basis":0,"contest_not_one_sentence":0,"contest_on_group_citation":0},"papers_read":39,"self_papers":4,"citing_papers":305,"sentences_read":39,"citing_sentences":351,"unambiguous_read":39,"typed_independent":4,"independent_papers":301,"by_kind_independent":{"data_used":2,"comparison":1,"supports_this_paper":1}},"input_sha256":"af1e12f6cec18fd46fcc7b8c697d116d87369212917e715dead7c1bc3e681478","method":"For a paper with five or more citing arXiv papers, Pith selected up to 40 citing sentences its citation classifier typed, read those whose citation markers point at this paper alone, and wrote one paraphrase for each later paper in each group, each resting on one sentence. A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"1 later paper by other authors is listed below: 1 used its data or values."},"_links":{"html":"https://pith.science/paper/hep-th/0302219"}}