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Homotopically non-trivial maps with small k-dilation
Differential Geometry · Submitted 9 Sep 2007
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We construct homotopically non-trivial maps from S^m to S^n with arbitrarily small 3-dilation for certain pairs (m,n).
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The abstract, sentence by sentence
We construct homotopically non-trivial maps from S^m to S^n with arbitrarily small 3-dilation for certain pairs (m,n). The simplest example is m=4, n=3. Other examples include arbitrarily large values of m and n. We show that a homotopy class in pi_7(S^4) can be represented by maps with arbitrarily small 4-dilation if and only if the class is torsion.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We construct homotopically non-trivial maps from S^m to S^n with arbitrarily small 3-dilation for certain pairs (m,n). | contribution 0.57 | 0.95 | 0.74 | asserted 1.00 |
| s1 | The simplest example is m=4, n=3. | result 0.84 | 0.72 | 0.06 | asserted 1.00 |
| s2 | Other examples include arbitrarily large values of m and n. | result 0.86 | 0.80 | 0.07 | asserted 0.98 |
| s3 | We show that a homotopy class in pi_7(S^4) can be represented by maps with arbitrarily small 4-dilation if and only if the class is torsion. | result 0.98 | 0.90 | 0.36 | asserted 1.00 |
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The paper
Original abstract
We construct homotopically non-trivial maps from S^m to S^n with arbitrarily small 3-dilation for certain pairs (m,n). The simplest example is m=4, n=3. Other examples include arbitrarily large values of m and n. We show that a homotopy class in pi_7(S^4) can be represented by maps with arbitrarily small 4-dilation if and only if the class is torsion.
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The most widely discussed alternative is the direct collapse scenario, in which primordial gas in atomic-cooling haloes ($T_vir≳10^4$ K) avoids fragmentation into stars when H$_2$ cooling is suppressed by a strong Lyman–Werner radiation field, and instead collapses to form a direct collapse black hole (DCBH) seed with $M_seed∼10^4$–$10^6 M_⊙$ [ref] .
Revisiting the Claim for a Direct-Collapse Black Hole in UHZ1 at $z=10.05$ · Introduction · 0.99
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