Research profile
Lu Yin
Shanghai U.
arXiv endorsement eligibility
arXiv requires established authors to endorse first-time submitters in a subject area. Eligibility depends on papers submitted between three months and five years ago, so it changes over time. These are estimates computed from public arXiv metadata — arXiv does not publish its exact thresholds, and endorsement decisions are private.
Selected publications
The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
2025astro-ph.CO · gr-qc · hep-ph566 citationsarXiv:2504.01669
Is the observable Universe consistent with the cosmological principle?
2022astro-ph.CO · gr-qc · hep-ph · hep-th · physics.hist-ph330 citationsarXiv:2207.05765
Does Hubble tension signal a breakdown in FLRW cosmology?
2021astro-ph.CO · gr-qc · hep-ph · hep-th192 citationsarXiv:2105.09790
Larger <math display="inline"><msub><mi>H</mi><mn>0</mn></msub></math> values in the CMB dipole direction
2021astro-ph.CO · gr-qc · hep-ph · hep-th132 citationsarXiv:2108.13228
Hints of FLRW breakdown from supernovae
2021astro-ph.CO · gr-qc · hep-ph · hep-th126 citationsarXiv:2106.02532
Can dark energy be dynamical?
2021astro-ph.CO · gr-qc · hep-th88 citationsarXiv:2104.01930
How much has DESI dark energy evolved since DR1?
2025astro-ph.CO · hep-ph · hep-th69 citationsarXiv:2504.04417
A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
2015astro-ph.CO51 citationsarXiv:1503.08948
Stochastic Gravitational Waves from Inflaton Decays
2019hep-ph · astro-ph.CO · gr-qc48 citationsarXiv:1905.08510
Reducing the $H_{0}$ tension with generalized Proca theory
2020astro-ph.CO · gr-qc46 citationsarXiv:2002.06782
Inevitable manifestation of wiggles in the expansion of the late Universe
2022astro-ph.CO · gr-qc45 citationsarXiv:2207.10609
Modified Cosmology Models from Thermodynamical Approach
2019astro-ph.CO · gr-qc35 citationsarXiv:1911.06046
Is cosmic birefringence model-dependent?
2023astro-ph.CO · hep-ph29 citationsarXiv:2305.07937
Do high redshift QSOs and GRBs corroborate JWST?
2024astro-ph.CO · gr-qc · hep-ph28 citationsarXiv:2405.19953
Constraints on running vacuum model with $H(z)$ and $f \sigma_8$
2017astro-ph.CO26 citationsarXiv:1704.02136
Observational evidence for early dark energy as a unified explanation for cosmic birefringence and the Hubble tension
2024astro-ph.CO22 citationsarXiv:2408.09521
Reducing the $H_0$ tension with exponential acoustic dark energy
2020astro-ph.CO19 citationsarXiv:2012.13917
A Dark Energy model from Generalized Proca Theory
2021gr-qc · astro-ph.CO17 citationsarXiv:2104.06577
Constraints on a special running vacuum model
2020astro-ph.CO · gr-qc14 citationsarXiv:2001.05092
Joint constraints on cosmic birefringence and early dark energy from ACT, Planck, DESI, and PantheonPlus
2026astro-ph.CO · gr-qc · hep-ph · hep-th14 citationsarXiv:2601.13624
Sources
Identity, affiliation and publication record: INSPIRE-HEP
ORCID: 0000-0002-8289-0814
Endorsement eligibility computed from public arXiv submission metadata.
Last refreshed July 27, 2026.
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