Evidence map›Paper›PMID 42222581›Full record

ArticleMacromolecules2026

Star-Like Microgels vs Star Polymers: Similarities and Differences.

Tommaso Papetti, Elisa Ballin, Francesco Brasili, Emanuela Zaccarelli

Abstract read
In one paragraph

Article in Macromolecules, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

4 authors.

Tommaso PapettiDepartment of Physics, Sapienza University of Rome, Piazzale Aldo Moro 2, Roma 00185, Italy.ORCID https://orcid.org/0009-0001-8526-9468
Elisa BallinDepartment of Physics, Sapienza University of Rome, Piazzale Aldo Moro 2, Roma 00185, Italy.ORCID https://orcid.org/0009-0003-4522-1085
Francesco BrasiliUos Sapienza, CNR Institute of Complex Systems, Piazzale Aldo Moro 2, Roma 00185, Italy.ORCID https://orcid.org/0000-0002-3284-5054
Emanuela ZaccarelliUos Sapienza, CNR Institute of Complex Systems, Piazzale Aldo Moro 2, Roma 00185, Italy.ORCID https://orcid.org/0000-0003-0032-8906

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Star-like microgels have recently emerged as a promising class of thermoresponsive soft colloids that have an internal architecture similar to that of star polymers. Here, we perform extensive monomer-resolved simulations to theoretically establish this analogy. First, we characterize the effective potential between star-like microgels, finding that it is Gaussian for an extended range of distances, in stark contrast to the Hertzian-like potential of standard microgels, but almost identical to that of star polymers with a core partially covered by chains. Next, we investigate the ratio between gyration and hydrodynamic radii across the volume-phase transition, showing qualitative agreement with both star polymers and experimental data. Finally, we estimate the bulk modulus, finding star-like microgels significantly softer than standard microgels and comparable to star polymers. The present work thus demonstrates that star-like microgels behave as ultrasoft particles, akin to star polymers, paving the way for their exploration at high concentrations.

Identifiers

PMID42222581
PMCPMC13217620

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Registered trials

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.