2001
DOI: 10.4064/fm169-1-2
|View full text |Cite
|
Sign up to set email alerts
|

On invariants for measure preserving transformations

Abstract: Abstract. The classification problem for measure preserving transformations is strictly more complicated than that of graph isomorphism. Preamble.We consider the group M ∞ of all invertible measure preserving transformations either on the unit interval or any other reasonable measure space. It seems natural to say that two of these transformations, σ 1 , σ 2 , are equivalent or isomorphic if there is a third, π, so thatTo what extent can this equivalence relation be considered classifiable? In specific cases-f… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
5

Citation Types

1
25
0

Year Published

2006
2006
2023
2023

Publication Types

Select...
8
2

Relationship

0
10

Authors

Journals

citations
Cited by 34 publications
(26 citation statements)
references
References 22 publications
1
25
0
Order By: Relevance
“…Hjorth ([10]) introduced the notion of turbulence and used it in [11] to show that there is no Borel way of attaching algebraic invariants to ergodic transformations that completely determine isomorphism. Foreman and Weiss [6] improved this result to show that the action of the group of measure preserving transformations on the ergodic transformations is turbulent.…”
Section: Introductionmentioning
confidence: 99%
“…Hjorth ([10]) introduced the notion of turbulence and used it in [11] to show that there is no Borel way of attaching algebraic invariants to ergodic transformations that completely determine isomorphism. Foreman and Weiss [6] improved this result to show that the action of the group of measure preserving transformations on the ergodic transformations is turbulent.…”
Section: Introductionmentioning
confidence: 99%
“…These differences likely reflect the different origin of these events. Indeed, observational evidence allowed the association of LGRBs to core-collapse supernovae (SNe; supporting the so-called "collapsar model", see Hjorth & Bloom 2012;Cano et al 2017, for recent reviews), while the recent detection of a gravitational wave (GW) source with a simultaneous SGRB seems to be the long-sought "smoking gun" that sets mergers of double neutron stars (NS-NS) as the progenitors of these events (Abbott et al 2017;Goldstein et al 2017;Savchenko et al 2017). According to this scenario, called the compact object binary merger, which includes also neutron star-black hole (NS-BH) binary systems (Eichler et al 1989;Nakar 2007), the merging objects originate either from (i) a "primordial" binary (Narayan et al 1992), whose component stars were gravitationally bound since their birth, or (ii) a "dynamical binary", formed by means of dynamical capture and possibly exchange in dense stellar environments (e.g.…”
Section: Introductionmentioning
confidence: 94%
“…The GRB data show a bimodal distribution of long ( 2s) and short bursts, indicating different progenitor systems. The origin of long-duration GRBs has now been established as the core-collapse of massive stars (Woosley 1993) by the association with type Ibc supernovae in a few cases (Hjorth & Bloom 2012). The recent observation of GRB 170817A in association with the gravitational wave GW170817 (Abbott et al 2017a,b) has confirmed the idea that (at least some) short-duration GRB originate from binary neutron star mergers (Paczynski 1986;Eichler et al 1989;Narayan et al 1992).…”
Section: Introductionmentioning
confidence: 96%