Pablo Pinacho

Dr. Pablo Pinacho

Química Física y Química Inorgánica, Universidad de Valladolid, Valladolid, Castille-Leon, Spain
orcid

Research Focus & Metrics

Academic Career Length

15Years (2012-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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7 June 2016 in Physical Chemistry Chemical Physics
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Journal Article
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SDSérgio R. Domingos
Sérgio R. Domingos
CPCristobal Perez
Cristobal Perez
CMChris Medcraft
Chris Medcraft
PPPablo Pinacho
Pablo Pinacho
MSMelanie Schnell
Melanie Schnell
High resolution rotational spectroscopy is used to map the conformational landscape and derive conformational relaxation pathways of citronellal.

28 June 2016 in Angewandte Chemie International Edition
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Journal Article
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Susana BlancoSusana Blanco
Susana Blanco
PPPablo Pinacho
Pablo Pinacho
Juan Carlos LópezJuan Carlos López
Juan Carlos López
The rotational spectrum of formamide2–H2O formed in a supersonic jet has been characterized by Fourier‐transform microwave spectroscopy. This adduct provides a simple model of water‐mediated interaction involving the amide linkages, as occur in protein folding or amide‐association processes, showing the interplay between self‐association and solvation. Mono‐substituted 13C, 15N, 18O, and 2H isotopologues have been observed and their data used to investigate the structure. The adduct forms an almost planar three‐body sequential cycle. The two formamide molecules link on one side through an N−H⋅⋅⋅O hydrogen bond and on the other side through a water‐mediated interaction with the formation of C=O⋅⋅⋅H−O and O⋅⋅⋅H−N hydrogen bonds. The analysis of the quadrupole coupling effects of two 14N‐nuclei reveals the subtle inductive forces associated to cooperative hydrogen bonding. These forces are involved in the changes in the C=O and C−N bond lengths with respect to pure formamide.

28 January 2021 in The Journal of Physical Chemistry Letters
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Journal Article
Open access
RSRizalina Tama Saragi
Rizalina Tama Saragi
MJMarcos Juanes
Marcos Juanes
CPCristobal Perez
Cristobal Perez
PPPablo Pinacho
Pablo Pinacho
DTDenis S. Tikhonov
Denis S. Tikhonov
ALAlberto Lesarri
Alberto Lesarri
We used jet-cooled broadband rotational spectroscopy to explore the balance between π-stacking and hydrogen-bonding interactions in the self-aggregation of thiophenol. Two different isomers were detected for the thiophenol dimer, revealing dispersion-controlled π-stacked structures anchored by a long S–H···S sulfur hydrogen bond. The weak intermolecular forces allow for noticeable internal dynamics in the dimers, as tunneling splittings are observed for the global minimum. The large-amplitude motion is ascribed to a concerted inversion motion between the two rings, exchanging the roles of the proton donor and acceptor in the thiol groups. The determined torsional barrier of B2 = 250.3 cm–1 is consistent with theoretical predictions (290–502 cm–1) and the monomer barrier of 277.1(3) cm–1. For the thiophenol trimer, a symmetric top structure was assigned in the spectrum. The results highlight the relevance of substituent effects to modulate π-stacking geometries and the role of the sulfur-centered hydrogen bonds.

5 December 2017 in The Journal of Physical Chemistry Letters
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Journal Article
Closed access
Susana BlancoSusana Blanco
Susana Blanco
PPPablo Pinacho
Pablo Pinacho
Juan Carlos LópezJuan Carlos López
Juan Carlos López

12 September 2012 in Analytical Chemistry
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Journal Article
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GVG. Vidal-De-Miguel
G. Vidal-De-Miguel
MMM. Macía
M. Macía
PPPablo Pinacho
Pablo Pinacho
JBJ. Blanco
J. Blanco

6 April 2021 in Physical Chemistry Chemical Physics
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Journal Article
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DLDonatella Loru
Donatella Loru
ASAmanda Steber
Amanda Steber
PPPablo Pinacho
Pablo Pinacho
SGSébastien Gruet
Sébastien Gruet
BTBerhane Temelso
Berhane Temelso
MSMelanie Schnell
Melanie Schnell
The influence of a nitrogen atom in the backbone of a PAH was revealed by the hydrated clusters of phenanthrene and phenanthridine in a rotational spectroscopy study. Background image credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) – ESA/Hubble Collaboration.