HgN2

HgN2 is a semiconducting mercury-nitrogen compound that is thermodynamically unstable and primarily of interest for theoretical structural research.

HgN
Crystal structure of HgN2 (cubic, Fd-3m (No. 227))
Ground-state structure · Materials Project
Overview

About HgN2

HgN2 is a binary compound composed of mercury and nitrogen that exhibits semiconducting electronic behavior. Its structural complexity is highlighted by a significant number of reported configurations within material databases, reflecting ongoing interest in its atomic arrangement despite its challenging synthesis profile. The compound is characterized by its thermodynamic instability, as it resides above the hull in energy landscapes. This positioning suggests that while it can be modeled and studied theoretically, it remains a difficult target for experimental realization under ambient conditions.

At a glance

Key Properties

Cross-validated computational properties for HgN2, aggregated across 3 databases.

Band Gap

0.92 eV
Range across DFT structures · ground state: metal

Energy Above Hull

2.454 eV/atom
Best (lowest) across sources

Stability

Unstable
2 DFT sources

Structures

129
3 databases, 26 space groups
Validation

Cross-Source DFT Agreement

How well independent DFT databases agree on the thermodynamics of HgN2. Tight agreement means computed properties can be trusted without re-running calculations.

Agreement Score

0.00 / 1.00
Trust tier: low

Hull Spread

0.267 eV
EAH spread across sources

Sources Compared

2
materials_project, oqmd

Space Group Consensus

—
Crystallography

Reported Structures

Lowest-energy structures reported for HgN2, ranked by energy above hull.

Space GroupCrystal SystemBand Gap (eV)E above hull (eV/atom)E/atom (eV)Density (g/cm³)
——0.002.45402.454—
Fd-3m (No. 227)cubic0.922.7212-19.8212.89
——0.002.82822.828—
P-1 (No. 2)triclinic———5.64
P1 (No. 1)triclinic———10.53
P1 (No. 1)triclinic———9.98
P1 (No. 1)triclinic———10.05
P1 (No. 1)triclinic———8.59
P1 (No. 1)triclinic———7.92
P1 (No. 1)triclinic———7.12
P1 (No. 1)triclinic———7.54
P1 (No. 1)triclinic———4.89
Reference

Frequently Asked Questions

Common questions about HgN2, answered from cross-validated data.

What is HgN2?

HgN2 is a semiconducting mercury-nitrogen compound that is thermodynamically unstable and primarily of interest for theoretical structural research.

More questions
What is the band gap of HgN2?
HgN2 has a DFT-computed band gap of 0.92 eV across 129 reported structures. Standard DFT underestimates band gaps, so the measured gap is typically larger.
Is HgN2 a metal, semiconductor, or insulator?
DFT predicts a band gap of up to 0.92 eV (a semiconductor). Measured gaps are typically larger.
Is HgN2 thermodynamically stable?
HgN2 has a lowest energy above hull of 2.454 eV/atom (unstable).
What is the crystal structure of HgN2?
The reference structure of HgN2 is cubic symmetry, space group Fd-3m (No. 227).
What is the density of HgN2?
The computed density of the ground-state structure of HgN2 is 2.89 g/cm³.
How many polymorphs of HgN2 are known?
129 structures of HgN2 are reported across 3 databases, spanning 26 distinct space groups.
What elements does HgN2 contain?
HgN2 contains Hg and N (2 elements).
Where does the data for HgN2 come from?
HgN2 data is cross-referenced from oqmd, materials_project, mpaloe.
Comparison

How It Compares

As a unique binary system, HgN2 represents a distinct case study in mercury-nitrogen chemistry. Unlike more stable, naturally occurring binary nitrides, this compound serves as a critical reference point for understanding the limits of structural stability and the electronic consequences of nitrogen-rich bonding in heavy metal systems.

Data sources & attribution
  • oqmd — Data from the OQMD (oqmd.org). Cite: Saal et al., JOM 65, 1501 (2013); Kirklin et al., npj Comp. Mater. 1, 15010 (2015). (CC-BY-4.0)
  • materials_project — Data from the Materials Project (materialsproject.org). Cite: Jain et al., APL Materials 1, 011002 (2013). (CC-BY-4.0)
  • mpaloe — Data from MP-ALOE. Cite: Kuner et al., npj Comput. Mater. (2025), doi:10.1038/s41524-025-01834-9.

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