Paper Citation Record · LEDGER

Can recent DESI BAO measurements accommodate a negative cosmological constant?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2406.03395.

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pith.paper-citation-record.v1
2406.03395 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

Observation 7a5b17b4-cdc7-4c6f-af91-4542a83ea8fc · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 118

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Bridge the Cosmological Tensions with Thawing Gravity cites this paper.

Bridge the Cosmological Tensions with Thawing Gravity Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 29

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Observation 1bd9be2e-2d9b-4b8d-a651-52c2d9ee6636 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 93

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Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 30

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Observation ed04b43e-1d42-4fcd-8a9b-1cf5c19b5275 · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 18

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Observation 6604da09-2e80-4a48-a304-ff93cc388737 · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 28

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Observation 8c7a166e-c1d1-4795-b6a1-1e756a39566d · inbound

Phase transition in a doubly holographic model of closed $\mathbf{dS_{2} }$ spacetime cites this paper.

Phase transition in a doubly holographic model of closed $\mathbf{dS_{2} }$ spacetime Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 34

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Observation 55e48f6d-c9b9-48cc-be45-f589c68ad9e3 · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 20

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Cosmological constraints on Galileon dark energy with broken shift symmetry cites this paper.

Cosmological constraints on Galileon dark energy with broken shift symmetry Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 12

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Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 115

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Observation dba7dac3-7acb-4ca5-aed8-e6bdc64e428c · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 196

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Observation e9caea05-7897-42fc-b056-05815ac56eeb · inbound

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 143

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 154

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Observation b9359e0a-216a-405a-879e-c6ef2b5bb293 · inbound

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars cites this paper.

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-07-04T20:10:08.693216Z

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Observation 18cd3ea6-1c14-4bc8-9092-4e308d7aebe9 · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 131

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Observation 66f7ccf2-4c03-4c36-9c28-e96ae356df35 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 21

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